Articles in International Journals, Proceedings and Circulars
- O. Erece, I. M. Khamitov, M. Kaplan, Y. Kilic, H. Lee, M. Kim, I. F. Bikmaev, R. I. Gumerov, and E. N. Irtuganov, “Physical properties of the slow-rotating near-Earth asteroid (2059) Baboquivari from one apparition,” \planss, vol. 232, p. 105698, 2023. doi:10.1016/j.pss.2023.105698
[BibTeX]@ARTICLE{2023P&SS..23205698E, author = {{Erece}, Orhan and {Khamitov}, Irek M. and {Kaplan}, Murat and {Kilic}, Yucel and {Lee}, Hee-Jae and {Kim}, Myung-Jin and {Bikmaev}, Ilfan F. and {Gumerov}, Rustem I. and {Irtuganov}, Eldar N.}, title = "{Physical properties of the slow-rotating near-Earth asteroid (2059) Baboquivari from one apparition}", journal = {\planss}, keywords = {Minor planets, Near-earth asteroids: individual: (2059) Baboquivari, Methods: observational, Techniques: photometry, Polarimetry, Spectroscopy, Earth Science, Astrophysics - Earth and Planetary Astrophysics}, year = 2023, month = aug, volume = {232}, eid = {105698}, pages = {105698}, doi = {10.1016/j.pss.2023.105698}, archivePrefix = {arXiv}, eprint = {2305.05217}, primaryClass = {astro-ph.EP}, adsurl = {https://ui.adsabs.harvard.edu/abs/2023P&SS..23205698E}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - F. ~L. Rommel, F. Braga-Ribas, J. ~L. Ortiz, B. Sicardy, P. Santos-Sanz, J. Desmars, J. ~I. ~B. Camargo, R. Vieira-Martins, M. Assafin, B. ~E. Morgado, R. ~C. Boufleur, G. Benedetti-Rossi, A. ~R. Gomes-Júnior, E. Fernández-Valenzuela, B. ~J. Holler, D. Souami, R. Duffard, G. Margoti, M. Vara-Lubiano, J. Lecacheux, J. ~L. Plouvier, N. Morales, A. Maury, J. Fabrega, P. Ceravolo, E. Jehin, D. Albanese, H. Mariey, S. Cikota, D. Ruvzdjak, A. Cikota, R. Szakáts, D. Baba Aissa, Z. Gringahcene, V. Kashuba, N. Koshkin, V. Zhukov, S. Ficsek, O. cCakir, S. Özer, C. Schnabel, M. Schnabel, F. Signoret, L. Morrone, T. Santana-Ros, C. ~L. Pereira, M. Emilio, A. ~Y. Burdanov, J. de Wit, K. Barkaoui, M. Gillon, G. Leto, A. Frasca, G. Catanzaro, R. Zanmar Sanchez, U. Tagliaferri, M. Di Sora, G. Isopi, Y. Krugly, I. Slyusarev, V. Chiorny, H. Mikuvz, P. Bacci, M. Maestripieri, M. ~D. Grazia, I. de la Cueva, M. Yuste-Moreno, F. Ciabattari, O. ~M. Kozhukhov, M. Serra-Ricart, M. ~R. Alarcon, J. Licandro, G. Masi, R. Bacci, J. ~M. Bosch, R. Behem, J. -P. Prost, S. Renner, M. Conjat, M. Bachini, G. Succi, L. Stoian, A. Juravle, D. Carosati, B. Gowe, J. Carrillo, A. ~P. Zheleznyak, N. Montigiani, C. ~R. Foster, M. Mannucci, N. Ruocco, F. Cuevas, P. Di Marcantonio, I. Coretti, G. Iafrate, V. Baldini, M. Collins, A. Pál, B. Csák, E. Fernández-Garcia, A. ~J. Castro-Tirado, L. Hudin, J. ~M. Madiedo, R. ~M. Anghel, J. ~F. Calvo-Fernández, A. Valvasori, E. Guido, R. ~M. Gherase, S. Kamoun, R. Fafet, M. Sánchez-González, L. Curelaru, C. ~D. V^intdevarua, C. ~A. Danescu, J. -F. Gout, C. ~J. Schmitz, A. Sota, I. Belskaya, M. Rodr’iguez-Marco, Y. Kilic, E. Frappa, A. Klotz, M. Lavayssière, J. Marques Oliveira, M. Popescu, L. ~A. Mammana, E. Fernández-Lajús, M. Schmidt, U. Hopp, R. Komvz’ik, T. Pribulla, D. Tomko, M. Husárik, O. Erece, S. Eryilmaz, L. Buzzi, B. Gährken, D. Nardiello, K. Hornoch, E. Sonbas, H. Er, V. Burwitz, P. Waldemar Sybilski, W. Bykowski, T. ~G. Müller, W. Ogloza, R. Gonccalves, J. ~F. Ferreira, M. Ferreira, M. Bento, S. Meister, M. ~N. Bagiran, M. Tekecs, A. Marciniak, Z. Moravec, P. Delinvcák, G. Gianni, G. ~B. Casalnuovo, M. Boutet, J. Sanchez, B. Klemt, N. Wuensche, W. Burzynski, M. Borkowski, M. Serrau, G. Dangl, O. Klös, C. Weber, M. Urban’ik, L. Rousselot, J. Kubánek, P. André, C. Colazo, J. Spagnotto, A. ~A. Sickafoose, R. Hueso, A. Sánchez-Lavega, R. ~S. Fisher, A. ~W. Rengstorf, C. Perelló, M. Dascalu, M. Altan, K. Gazeas, T. de Santana, R. Sfair, O. ~C. Winter, S. Kalkan, O. Canales-Moreno, J. ~M. Trigo-Rodr’iguez, V. Tsamis, K. Tigani, N. Sioulas, G. Lekkas, D. ~N. Bertesteanu, V. Dumitrescu, A. ~J. Wilberger, J. ~W. Barnes, S. ~K. Fieber-Beyer, R. ~L. Swaney, C. Fuentes, R. ~A. Mendez, B. ~D. Dumitru, R. ~L. Flynn, and D. ~A. Wake, “A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS$_4$ measured from stellar occultations,” arXiv e-prints, p. arXiv:2308.08062, 2023. doi:10.48550/arXiv.2308.08062
[BibTeX]@ARTICLE{2023arXiv230808062R, author = {{Rommel}, F.~L. and {Braga-Ribas}, F. and {Ortiz}, J.~L. and {Sicardy}, B. and {Santos-Sanz}, P. and {Desmars}, J. and {Camargo}, J.~I.~B. and {Vieira-Martins}, R. and {Assafin}, M. and {Morgado}, B.~E. and {Boufleur}, R.~C. and {Benedetti-Rossi}, G. and {Gomes-J{\'u}nior}, A.~R. and {Fern{\'a}ndez-Valenzuela}, E. and {Holler}, B.~J. and {Souami}, D. and {Duffard}, R. and {Margoti}, G. and {Vara-Lubiano}, M. and {Lecacheux}, J. and {Plouvier}, J.~L. and {Morales}, N. and {Maury}, A. and {Fabrega}, J. and {Ceravolo}, P. and {Jehin}, E. and {Albanese}, D. and {Mariey}, H. and {Cikota}, S. and {Ru{\v{z}}djak}, D. and {Cikota}, A. and {Szak{\'a}ts}, R. and {Baba Aissa}, D. and {Gringahcene}, Z. and {Kashuba}, V. and {Koshkin}, N. and {Zhukov}, V. and {Fi{\c{s}}ek}, S. and {{\c{C}}ak{\i}r}, O. and {{\"O}zer}, S. and {Schnabel}, C. and {Schnabel}, M. and {Signoret}, F. and {Morrone}, L. and {Santana-Ros}, T. and {Pereira}, C.~L. and {Emilio}, M. and {Burdanov}, A.~Y. and {de Wit}, J. and {Barkaoui}, K. and {Gillon}, M. and {Leto}, G. and {Frasca}, A. and {Catanzaro}, G. and {Zanmar Sanchez}, R. and {Tagliaferri}, U. and {Di Sora}, M. and {Isopi}, G. and {Krugly}, Y. and {Slyusarev}, I. and {Chiorny}, V. and {Miku{\v{z}}}, H. and {Bacci}, P. and {Maestripieri}, M. and {Grazia}, M.~D. and {de la Cueva}, I. and {Yuste-Moreno}, M. and {Ciabattari}, F. and {Kozhukhov}, O.~M. and {Serra-Ricart}, M. and {Alarcon}, M.~R. and {Licandro}, J. and {Masi}, G. and {Bacci}, R. and {Bosch}, J.~M. and {Behem}, R. and {Prost}, J. -P. and {Renner}, S. and {Conjat}, M. and {Bachini}, M. and {Succi}, G. and {Stoian}, L. and {Juravle}, A. and {Carosati}, D. and {Gowe}, B. and {Carrillo}, J. and {Zheleznyak}, A.~P. and {Montigiani}, N. and {Foster}, C.~R. and {Mannucci}, M. and {Ruocco}, N. and {Cuevas}, F. and {Di Marcantonio}, P. and {Coretti}, I. and {Iafrate}, G. and {Baldini}, V. and {Collins}, M. and {P{\'a}l}, A. and {Cs{\'a}k}, B. and {Fern{\'a}ndez-Garcia}, E. and {Castro-Tirado}, A.~J. and {Hudin}, L. and {Madiedo}, J.~M. and {Anghel}, R.~M. and {Calvo-Fern{\'a}ndez}, J.~F. and {Valvasori}, A. and {Guido}, E. and {Gherase}, R.~M. and {Kamoun}, S. and {Fafet}, R. and {S{\'a}nchez-Gonz{\'a}lez}, M. and {Curelaru}, L. and {V{\^\i}ntdevar{\u{a}}}, C.~D. and {Danescu}, C.~A. and {Gout}, J. -F. and {Schmitz}, C.~J. and {Sota}, A. and {Belskaya}, I. and {Rodr{\'\i}guez-Marco}, M. and {Kilic}, Y. and {Frappa}, E. and {Klotz}, A. and {Lavayssi{\`e}re}, M. and {Marques Oliveira}, J. and {Popescu}, M. and {Mammana}, L.~A. and {Fern{\'a}ndez-Laj{\'u}s}, E. and {Schmidt}, M. and {Hopp}, U. and {Kom{\v{z}}{\'\i}k}, R. and {Pribulla}, T. and {Tomko}, D. and {Hus{\'a}rik}, M. and {Erece}, O. and {Eryilmaz}, S. and {Buzzi}, L. and {G{\"a}hrken}, B. and {Nardiello}, D. and {Hornoch}, K. and {Sonbas}, E. and {Er}, H. and {Burwitz}, V. and {Waldemar Sybilski}, P. and {Bykowski}, W. and {M{\"u}ller}, T.~G. and {Ogloza}, W. and {Gon{\c{c}}alves}, R. and {Ferreira}, J.~F. and {Ferreira}, M. and {Bento}, M. and {Meister}, S. and {Bagiran}, M.~N. and {Teke{\c{s}}}, M. and {Marciniak}, A. and {Moravec}, Z. and {Delin{\v{c}}{\'a}k}, P. and {Gianni}, G. and {Casalnuovo}, G.~B. and {Boutet}, M. and {Sanchez}, J. and {Klemt}, B. and {Wuensche}, N. and {Burzynski}, W. and {Borkowski}, M. and {Serrau}, M. and {Dangl}, G. and {Kl{\"o}s}, O. and {Weber}, C. and {Urban{\'\i}k}, M. and {Rousselot}, L. and {Kub{\'a}nek}, J. and {Andr{\'e}}, P. and {Colazo}, C. and {Spagnotto}, J. and {Sickafoose}, A.~A. and {Hueso}, R. and {S{\'a}nchez-Lavega}, A. and {Fisher}, R.~S. and {Rengstorf}, A.~W. and {Perell{\'o}}, C. and {Dascalu}, M. and {Altan}, M. and {Gazeas}, K. and {de Santana}, T. and {Sfair}, R. and {Winter}, O.~C. and {Kalkan}, S. and {Canales-Moreno}, O. and {Trigo-Rodr{\'\i}guez}, J.~M. and {Tsamis}, V. and {Tigani}, K. and {Sioulas}, N. and {Lekkas}, G. and {Bertesteanu}, D.~N. and {Dumitrescu}, V. and {Wilberger}, A.~J. and {Barnes}, J.~W. and {Fieber-Beyer}, S.~K. and {Swaney}, R.~L. and {Fuentes}, C. and {Mendez}, R.~A. and {Dumitru}, B.~D. and {Flynn}, R.~L. and {Wake}, D.~A.}, title = "{A large topographic feature on the surface of the trans-Neptunian object (307261) 2002 MS$_4$ measured from stellar occultations}", journal = {arXiv e-prints}, keywords = {Astrophysics - Earth and Planetary Astrophysics}, year = 2023, month = aug, eid = {arXiv:2308.08062}, pages = {arXiv:2308.08062}, doi = {10.48550/arXiv.2308.08062}, archivePrefix = {arXiv}, eprint = {2308.08062}, primaryClass = {astro-ph.EP}, adsurl = {https://ui.adsabs.harvard.edu/abs/2023arXiv230808062R}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - J. ~L. Ortiz, C. ~L. Pereira, B. Sicardy, F. Braga-Ribas, A. Takey, A. ~M. Fouad, A. ~A. Shaker, S. Kaspi, N. Brosch, M. Kretlow, R. Leiva, J. Desmars, B. ~E. Morgado, N. Morales, M. Vara-Lubiano, P. Santos-Sanz, E. Fernández-Valenzuela, D. Souami, R. Duffard, F. ~L. Rommel, Y. Kilic, O. Erece, D. Koseoglu, E. Ege, R. Morales, A. Alvarez-Candal, J. ~L. Rizos, J. ~M. Gómez-Limón, M. Assafin, R. Vieira-Martins, A. ~R. Gomes-Júnior, J. ~I. ~B. Camargo, and J. Lecacheux, “Changing material around (2060) Chiron revealed by an occultation on December 15, 2022,” åp, vol. 676, p. L12, 2023. doi:10.1051/0004-6361/202347025
[BibTeX]@ARTICLE{2023A&A...676L..12O, author = {{Ortiz}, J.~L. and {Pereira}, C.~L. and {Sicardy}, B. and {Braga-Ribas}, F. and {Takey}, A. and {Fouad}, A.~M. and {Shaker}, A.~A. and {Kaspi}, S. and {Brosch}, N. and {Kretlow}, M. and {Leiva}, R. and {Desmars}, J. and {Morgado}, B.~E. and {Morales}, N. and {Vara-Lubiano}, M. and {Santos-Sanz}, P. and {Fern{\'a}ndez-Valenzuela}, E. and {Souami}, D. and {Duffard}, R. and {Rommel}, F.~L. and {Kilic}, Y. and {Erece}, O. and {Koseoglu}, D. and {Ege}, E. and {Morales}, R. and {Alvarez-Candal}, A. and {Rizos}, J.~L. and {G{\'o}mez-Lim{\'o}n}, J.~M. and {Assafin}, M. and {Vieira-Martins}, R. and {Gomes-J{\'u}nior}, A.~R. and {Camargo}, J.~I.~B. and {Lecacheux}, J.}, title = "{Changing material around (2060) Chiron revealed by an occultation on December 15, 2022}", journal = {\aap}, keywords = {occultations, Kuiper belt: general, comets: general, minor planets, asteroids: individual: Chiron, Astrophysics - Earth and Planetary Astrophysics}, year = 2023, month = aug, volume = {676}, eid = {L12}, pages = {L12}, doi = {10.1051/0004-6361/202347025}, archivePrefix = {arXiv}, eprint = {2308.03458}, primaryClass = {astro-ph.EP}, adsurl = {https://ui.adsabs.harvard.edu/abs/2023A&A...676L..12O}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - C. ~L. Pereira, B. Sicardy, B. ~E. Morgado, F. Braga-Ribas, E. Fernández-Valenzuela, D. Souami, B. ~J. Holler, R. ~C. Boufleur, G. Margoti, M. Assafin, J. ~L. Ortiz, P. Santos-Sanz, B. Epinat, P. Kervella, J. Desmars, R. Vieira-Martins, Y. Kilic, A. ~R. Gomes Júnior, J. ~I. ~B. Camargo, M. Emilio, M. Vara-Lubiano, M. Kretlow, L. Albert, C. Alcock, J. ~G. Ball, K. Bender, M. ~W. Buie, K. Butterfield, M. Camarca, J. ~H. Castro-Chacón, R. Dunford, R. ~S. Fisher, D. Gamble, J. ~C. Geary, C. ~L. Gnilka, K. ~D. Green, Z. ~D. Hartman, C. -K. Huang, H. Januszewski, J. Johnston, M. Kagitani, R. Kamin, J. ~J. Kavelaars, J. ~M. Keller, K. ~R. de Kleer, M. ~J. Lehner, A. Luken, F. Marchis, T. Marlin, K. McGregor, V. Nikitin, R. Nolthenius, C. Patrick, S. Redfield, A. ~W. Rengstorf, M. Reyes-Ruiz, T. Seccull, M. ~F. Skrutskie, A. ~B. Smith, M. Sproul, A. ~W. Stephens, A. Szentgyorgyi, S. Sánchez-Sanjuán, E. Tatsumi, A. Verbiscer, S. -Y. Wang, F. Yoshida, R. Young, and Z. -W. Zhang, “The two rings of (50000) Quaoar,” åp, vol. 673, p. L4, 2023. doi:10.1051/0004-6361/202346365
[BibTeX]@ARTICLE{2023A&A...673L...4P, author = {{Pereira}, C.~L. and {Sicardy}, B. and {Morgado}, B.~E. and {Braga-Ribas}, F. and {Fern{\'a}ndez-Valenzuela}, E. and {Souami}, D. and {Holler}, B.~J. and {Boufleur}, R.~C. and {Margoti}, G. and {Assafin}, M. and {Ortiz}, J.~L. and {Santos-Sanz}, P. and {Epinat}, B. and {Kervella}, P. and {Desmars}, J. and {Vieira-Martins}, R. and {Kilic}, Y. and {Gomes J{\'u}nior}, A.~R. and {Camargo}, J.~I.~B. and {Emilio}, M. and {Vara-Lubiano}, M. and {Kretlow}, M. and {Albert}, L. and {Alcock}, C. and {Ball}, J.~G. and {Bender}, K. and {Buie}, M.~W. and {Butterfield}, K. and {Camarca}, M. and {Castro-Chac{\'o}n}, J.~H. and {Dunford}, R. and {Fisher}, R.~S. and {Gamble}, D. and {Geary}, J.~C. and {Gnilka}, C.~L. and {Green}, K.~D. and {Hartman}, Z.~D. and {Huang}, C. -K. and {Januszewski}, H. and {Johnston}, J. and {Kagitani}, M. and {Kamin}, R. and {Kavelaars}, J.~J. and {Keller}, J.~M. and {de Kleer}, K.~R. and {Lehner}, M.~J. and {Luken}, A. and {Marchis}, F. and {Marlin}, T. and {McGregor}, K. and {Nikitin}, V. and {Nolthenius}, R. and {Patrick}, C. and {Redfield}, S. and {Rengstorf}, A.~W. and {Reyes-Ruiz}, M. and {Seccull}, T. and {Skrutskie}, M.~F. and {Smith}, A.~B. and {Sproul}, M. and {Stephens}, A.~W. and {Szentgyorgyi}, A. and {S{\'a}nchez-Sanju{\'a}n}, S. and {Tatsumi}, E. and {Verbiscer}, A. and {Wang}, S. -Y. and {Yoshida}, F. and {Young}, R. and {Zhang}, Z. -W.}, title = "{The two rings of (50000) Quaoar}", journal = {\aap}, keywords = {methods: data analysis, methods: observational, techniques: photometric, Kuiper belt objects: individual: Quaoar, planets and satellites: rings, Astrophysics - Earth and Planetary Astrophysics}, year = 2023, month = may, volume = {673}, eid = {L4}, pages = {L4}, doi = {10.1051/0004-6361/202346365}, archivePrefix = {arXiv}, eprint = {2304.09237}, primaryClass = {astro-ph.EP}, adsurl = {https://ui.adsabs.harvard.edu/abs/2023A&A...673L...4P}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - Y. Kilic, F. Braga-Ribas, M. Kaplan, O. Erece, D. Souami, M. Dindar, J. Desmars, B. Sicardy, B. ~E. Morgado, M. ~N. Shameoni, F. ~L. Rommel, and A. ~R. Gomes-Júnior, “Occultation portal: A web-based platform for data collection and analysis of stellar occultations,” \mnras, vol. 515, iss. 1, pp. 1346-1357, 2022. doi:10.1093/mnras/stac1595
[BibTeX]@ARTICLE{2022MNRAS.515.1346K, author = {{Kilic}, Y. and {Braga-Ribas}, F. and {Kaplan}, M. and {Erece}, O. and {Souami}, D. and {Dindar}, M. and {Desmars}, J. and {Sicardy}, B. and {Morgado}, B.~E. and {Shameoni}, M.~N. and {Rommel}, F.~L. and {Gomes-J{\'u}nior}, A.~R.}, title = "{Occultation portal: A web-based platform for data collection and analysis of stellar occultations}", journal = {\mnras}, keywords = {methods: data analysis, techniques: image processing, occultations, minor planets, asteroids: general, software: development, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, year = 2022, month = sep, volume = {515}, number = {1}, pages = {1346-1357}, doi = {10.1093/mnras/stac1595}, archivePrefix = {arXiv}, eprint = {2206.09615}, primaryClass = {astro-ph.SR}, adsurl = {https://ui.adsabs.harvard.edu/abs/2022MNRAS.515.1346K}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - P. Santos-Sanz, J. ~L. Ortiz, B. Sicardy, M. Popescu, G. Benedetti-Rossi, N. Morales, M. Vara-Lubiano, J. ~I. ~B. Camargo, C. ~L. Pereira, F. ~L. Rommel, M. Assafin, J. Desmars, F. Braga-Ribas, R. Duffard, J. Marques Oliveira, R. Vieira-Martins, E. Fernández-Valenzuela, B. ~E. Morgado, M. Acar, S. Anghel, E. Atalay, A. Atecs, H. Bakics, V. Bakis, Z. Eker, O. Erece, S. Kaspi, C. Kayhan, S. ~E. Kilic, Y. Kilic, I. Manulis, D. ~A. Nedelcu, M. ~S. Niaei, G. Nir, E. Ofek, T. Ozisik, E. Petrescu, O. Satir, A. Solmaz, A. Sonka, M. Tekes, O. Unsalan, C. Yesilyaprak, R. Anghel, D. Bertecsteanu, L. Curelaru, C. Danescu, V. Dumitrescu, R. Gherase, L. Hudin, A. -M. Stoian, J. ~O. Tercu, R. Truta, V. Turcu, C. Vantdevara, I. Belskaya, T. ~O. Dementiev, K. Gazeas, S. Karampotsiou, V. Kashuba, C. Kiss, N. Koshkin, O. ~M. Kozhukhov, Y. Krugly, J. Lecacheux, A. Pal, C. Püsküllü, R. Szakats, V. Zhukov, D. Bamberger, B. Mondon, C. Perelló, A. Pratt, C. Schnabel, A. Selva, J. ~P. Teng, K. Tigani, V. Tsamis, C. Weber, G. Wells, S. Kalkan, V. Kudak, A. Marciniak, W. Ogloza, T. Özdemir, E. Pakvstiene, V. Perig, and M. Żejmo, “Physical properties of the trans-Neptunian object (38628) Huya from a multi-chord stellar occultation,” åp, vol. 664, p. A130, 2022. doi:10.1051/0004-6361/202141546
[BibTeX]@ARTICLE{2022A&A...664A.130S, author = {{Santos-Sanz}, P. and {Ortiz}, J.~L. and {Sicardy}, B. and {Popescu}, M. and {Benedetti-Rossi}, G. and {Morales}, N. and {Vara-Lubiano}, M. and {Camargo}, J.~I.~B. and {Pereira}, C.~L. and {Rommel}, F.~L. and {Assafin}, M. and {Desmars}, J. and {Braga-Ribas}, F. and {Duffard}, R. and {Marques Oliveira}, J. and {Vieira-Martins}, R. and {Fern{\'a}ndez-Valenzuela}, E. and {Morgado}, B.~E. and {Acar}, M. and {Anghel}, S. and {Atalay}, E. and {Ate{\c{s}}}, A. and {Baki{\c{s}}}, H. and {Bakis}, V. and {Eker}, Z. and {Erece}, O. and {Kaspi}, S. and {Kayhan}, C. and {Kilic}, S.~E. and {Kilic}, Y. and {Manulis}, I. and {Nedelcu}, D.~A. and {Niaei}, M.~S. and {Nir}, G. and {Ofek}, E. and {Ozisik}, T. and {Petrescu}, E. and {Satir}, O. and {Solmaz}, A. and {Sonka}, A. and {Tekes}, M. and {Unsalan}, O. and {Yesilyaprak}, C. and {Anghel}, R. and {Berte{\c{s}}teanu}, D. and {Curelaru}, L. and {Danescu}, C. and {Dumitrescu}, V. and {Gherase}, R. and {Hudin}, L. and {Stoian}, A. -M. and {Tercu}, J.~O. and {Truta}, R. and {Turcu}, V. and {Vantdevara}, C. and {Belskaya}, I. and {Dementiev}, T.~O. and {Gazeas}, K. and {Karampotsiou}, S. and {Kashuba}, V. and {Kiss}, Cs. and {Koshkin}, N. and {Kozhukhov}, O.~M. and {Krugly}, Y. and {Lecacheux}, J. and {Pal}, A. and {P{\"u}sk{\"u}ll{\"u}}, {\c{C}}. and {Szakats}, R. and {Zhukov}, V. and {Bamberger}, D. and {Mondon}, B. and {Perell{\'o}}, C. and {Pratt}, A. and {Schnabel}, C. and {Selva}, A. and {Teng}, J.~P. and {Tigani}, K. and {Tsamis}, V. and {Weber}, C. and {Wells}, G. and {Kalkan}, S. and {Kudak}, V. and {Marciniak}, A. and {Ogloza}, W. and {{\"O}zdemir}, T. and {Pak{\v{s}}tiene}, E. and {Perig}, V. and {{\.Z}ejmo}, M.}, title = "{Physical properties of the trans-Neptunian object (38628) Huya from a multi-chord stellar occultation}", journal = {\aap}, keywords = {Kuiper belt objects: individual: Huya, methods: observational, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics}, year = 2022, month = aug, volume = {664}, eid = {A130}, pages = {A130}, doi = {10.1051/0004-6361/202141546}, archivePrefix = {arXiv}, eprint = {2205.12882}, primaryClass = {astro-ph.EP}, adsurl = {https://ui.adsabs.harvard.edu/abs/2022A&A...664A.130S}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - A. ~R. Gomes-Júnior, B. ~E. Morgado, G. Benedetti-Rossi, R. ~C. Boufleur, F. ~L. Rommel, M. ~V. Banda-Huarca, Y. Kilic, F. Braga-Ribas, and B. Sicardy, “SORA: Stellar occultation reduction and analysis,” \mnras, vol. 511, iss. 1, pp. 1167-1181, 2022. doi:10.1093/mnras/stac032
[BibTeX]@ARTICLE{2022MNRAS.511.1167G, author = {{Gomes-J{\'u}nior}, A.~R. and {Morgado}, B.~E. and {Benedetti-Rossi}, G. and {Boufleur}, R.~C. and {Rommel}, F.~L. and {Banda-Huarca}, M.~V. and {Kilic}, Y. and {Braga-Ribas}, F. and {Sicardy}, B.}, title = "{SORA: Stellar occultation reduction and analysis}", journal = {\mnras}, keywords = {methods: data analysis, software: data analysis, occultations, Astrophysics - Instrumentation and Methods for Astrophysics}, year = 2022, month = mar, volume = {511}, number = {1}, pages = {1167-1181}, doi = {10.1093/mnras/stac032}, archivePrefix = {arXiv}, eprint = {2201.01799}, primaryClass = {astro-ph.IM}, adsurl = {https://ui.adsabs.harvard.edu/abs/2022MNRAS.511.1167G}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - I. Khamitov, …, Y. Kilic, and et al., “Position observations of the SRG spacecraft using the RTT-150 telescope (Antalya) to control its trajectory,” , 2019.
[BibTeX] [Download PDF]@conference{hea_2019, Address = {Moscow, Russia}, Author = {{Khamitov}, I. and {...} and {Kilic}, Y. and et al.}, Booktitle = {High Energy Astrophysics Today and Tomorrow (HEA-2019)}, Month = {December}, Organization = {IAU Focus Meetings (GA)}, Title = {Position observations of the SRG spacecraft using the RTT-150 telescope (Antalya) to control its trajectory}, Year = {2019}, url = {http://heaconf.cosmos.ru/2019/program.php}, } - P. Santos-Sanz and J. L. Ortiz, “The multi-chord stellar occultation by the Transneptunian object (38628) Huya on March 18th 2019,” in EPSC-DPS Joint Meeting 2019, 2019, p. EPSC-DPS2019-666.
[BibTeX] [Download PDF]@INPROCEEDINGS{huya_2019, author = {{Santos-Sanz}, Pablo and {Ortiz}, Jos{\'e} Luis}, title = "{The multi-chord stellar occultation by the Transneptunian object (38628) Huya on March 18th 2019}", booktitle = {EPSC-DPS Joint Meeting 2019}, year = "2019", volume = {2019}, month = "Sep", eid = {EPSC-DPS2019-666}, pages = {EPSC-DPS2019-666}, adsurl = {https://ui.adsabs.harvard.edu/abs/2019EPSC...13..666S}, url = {https://meetingorganizer.copernicus.org/EPSC-DPS2019/EPSC-DPS2019-666-5.pdf}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - K. Halicioglu, M. Albayrak, B. Basoglu, and Y. Kilic, “Modelling star trailed images of DZCS to improve the astro-geodetic geoid of Istanbul,” in EGU General Assembly Conference Abstracts, 2019, p. 11305.
[BibTeX]@INPROCEEDINGS{2019EGUGA..2111305H, author = {{Halicioglu}, Kerem and {Albayrak}, Muge and {Basoglu}, Burak and {Kilic}, Yucel}, title = "{Modelling star trailed images of DZCS to improve the astro-geodetic geoid of Istanbul}", booktitle = {EGU General Assembly Conference Abstracts}, year = "2019", series = {EGU General Assembly Conference Abstracts}, month = "Apr", eid = {11305}, pages = {11305}, adsurl = {https://ui.adsabs.harvard.edu/abs/2019EGUGA..2111305H}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - Ł. Wyrzykowski, P. Mróz, K. ~A. Rybicki, M. Gromadzki, Z. Kołaczkowski, M. Zieli’nski, P. Zieli’nski, N. Britavskiy, A. Gomboc, K. Sokolovsky, S. ~T. Hodgkin, L. Abe, G. ~F. Aldi, A. AlMannaei, G. Altavilla, A. ~A. Qasim, G. ~C. Anupama, S. Awiphan, E. Bachelet, V. Bakis, S. Baker, S. Bartlett, P. Bendjoya, K. Benson, I. ~F. Bikmaev, G. Birenbaum, N. Blagorodnova, S. Blanco-Cuaresma, S. Boeva, A. ~Z. Bonanos, V. Bozza, D. ~M. Bramich, I. Bruni, R. ~A. Burenin, U. Burgaz, T. Butterley, H. ~E. Caines, D. ~B. Caton, S. Calchi Novati, J. ~M. Carrasco, A. Cassan, V. Cepas, M. Cropper, M. Chru’sli’nska, G. Clementini, A. Clerici, D. Conti, M. Conti, S. Cross, F. Cusano, G. Damljanovic, A. Dapergolas, G. D’Ago, J. ~H. ~J. de Bruijne, M. Dennefeld, V. ~S. Dhillon, M. Dominik, J. Dziedzic, O. Erece, M. ~V. Eselevich, H. Esenoglu, L. Eyer, R. Figuera Jaimes, S. ~J. Fossey, A. ~I. Galeev, S. ~A. Grebenev, A. ~C. Gupta, A. ~G. Gutaev, N. Hallakoun, A. Hamanowicz, C. Han, B. Handzlik, J. ~B. Haislip, L. ~K. Hardy, D. ~L. Harrison, V. ~L. Hoette, K. Horne, R. Hudec, M. Hundertmark, N. Ihanec, E. ~N. Irtuganov, R. Itoh, P. Iwanek, M. ~D. Jovanovic, R. Janulis, M. Jelinek, E. Jensen, Z. Kaczmarek, D. Katz, I. ~M. Khamitov, Y. Kilic, J. Klencki, U. Kolb, V. ~V. Kouprianov, K. Kruszy’nska, S. Kurowski, G. Latev, C. Lee, S. Leonini, G. Leto, F. Lewis, Z. Li, A. Liakos, S. ~P. Littlefair, J. Lu, C. ~J. Manser, S. Mao, D. Maoz, M. Maskoliunas, J. ~R. Maund, S. ~S. Melnikov, K. Ment, P. Mikołajczyk, M. Morrell, N. Mowlavi, D. Moździerski, S. Nazarov, H. Netzel, R. Nesci, C. -C. Ngeow, A. ~J. Norton, E. ~O. Ofek, E. Pakstiene, L. Palaversa, A. Pandey, E. Paraskeva, M. Pawlak, M. ~T. Penny, B. ~E. Penprase, A. Piascik, J. ~L. Prieto, J. ~K. ~T. Qvam, C. Ranc, A. Rebassa-Mansergas, D. ~E. Reichart, P. Reig, L. Rhodes, J. -P. Rivet, G. Rixon, D. Roberts, P. Rosi, D. ~M. Russell, R. Zanmar Sanchez, G. Scarpetta, G. Seabroke, B. ~J. Shappee, R. Schmidt, Y. Shvartzvald, M. Sitek, J. Skowron, M. ‘Sniegowska, C. Snodgrass, P. ~S. Soares, Z. ~T. Spetsieri, A. Stankeviciute, I. ~A. Steele, R. ~A. Street, J. Strobl, L. ~M. Tinjaca Ramirez, L. Tomasella, Y. Tsapras, S. Villanueva Jr., O. Vince, J. Wambsganss, K. Wiersema, R. ~W. Wilson, A. Yoldas, R. ~Y. Zhuchkov, D. ~G. Zhukov, J. Zdanavicius, S. Zoła, and A. Zubareva, “Full Orbital Solution for the Binary System in the Northern Galactic Disk Microlensing Event Gaia16aye,” arXiv e-prints, 2019.
[BibTeX] [Download PDF]@article{2019arXiv190107281W, author = {{Wyrzykowski}, {\L}. and {Mr{\'o}z}, P. and {Rybicki}, K.~A. and {Gromadzki}, M. and {Ko{\l}aczkowski}, Z. and {Zieli{\'n}ski}, M. and {Zieli{\'n}ski}, P. and {Britavskiy}, N. and {Gomboc}, A. and {Sokolovsky}, K. and {Hodgkin}, S.~T. and {Abe}, L. and {Aldi}, G.~F. and {AlMannaei}, A. and {Altavilla}, G. and {Qasim}, A.~A. and {Anupama}, G.~C. and {Awiphan}, S. and {Bachelet}, E. and {Bakis}, V. and {Baker}, S. and {Bartlett}, S. and {Bendjoya}, P. and {Benson}, K. and {Bikmaev}, I.~F. and {Birenbaum}, G. and {Blagorodnova}, N. and {Blanco-Cuaresma}, S. and {Boeva}, S. and {Bonanos}, A.~Z. and {Bozza}, V. and {Bramich}, D.~M. and {Bruni}, I. and {Burenin}, R.~A. and {Burgaz}, U. and {Butterley}, T. and {Caines}, H.~E. and {Caton}, D.~B. and {Calchi Novati}, S. and {Carrasco}, J.~M. and {Cassan}, A. and {Cepas}, V. and {Cropper}, M. and {Chru{\'s}li{\'n}ska}, M. and {Clementini}, G. and {Clerici}, A. and {Conti}, D. and {Conti}, M. and {Cross}, S. and {Cusano}, F. and {Damljanovic}, G. and {Dapergolas}, A. and {D'Ago}, G. and {de Bruijne}, J.~H.~J. and {Dennefeld}, M. and {Dhillon}, V.~S. and {Dominik}, M. and {Dziedzic}, J. and {Erece}, O. and {Eselevich}, M.~V. and {Esenoglu}, H. and {Eyer}, L. and {Figuera Jaimes}, R. and {Fossey}, S.~J. and {Galeev}, A.~I. and {Grebenev}, S.~A. and {Gupta}, A.~C. and {Gutaev}, A.~G. and {Hallakoun}, N. and {Hamanowicz}, A. and {Han}, C. and {Handzlik}, B. and {Haislip}, J.~B. and {Hardy}, L.~K. and {Harrison}, D.~L. and {Hoette}, V.~L. and {Horne}, K. and {Hudec}, R. and {Hundertmark}, M. and {Ihanec}, N. and {Irtuganov}, E.~N. and {Itoh}, R. and {Iwanek}, P. and {Jovanovic}, M.~D. and {Janulis}, R. and {Jelinek}, M. and {Jensen}, E. and {Kaczmarek}, Z. and {Katz}, D. and {Khamitov}, I.~M. and {Kilic}, Y. and {Klencki}, J. and {Kolb}, U. and {Kouprianov}, V.~V. and {Kruszy{\'n}ska}, K. and {Kurowski}, S. and {Latev}, G. and {Lee}, C. and {Leonini}, S. and {Leto}, G. and {Lewis}, F. and {Li}, Z. and {Liakos}, A. and {Littlefair}, S.~P. and {Lu}, J. and {Manser}, C.~J. and {Mao}, S. and {Maoz}, D. and {Maskoliunas}, M. and {Maund}, J.~R. and {Melnikov}, S.~S. and {Ment}, K. and {Miko{\l}ajczyk}, P. and {Morrell}, M. and {Mowlavi}, N. and {Mo{\'z}dzierski}, D. and {Nazarov}, S. and {Netzel}, H. and {Nesci}, R. and {Ngeow}, C.-C. and {Norton}, A.~J. and {Ofek}, E.~O. and {Pakstiene}, E. and {Palaversa}, L. and {Pandey}, A. and {Paraskeva}, E. and {Pawlak}, M. and {Penny}, M.~T. and {Penprase}, B.~E. and {Piascik}, A. and {Prieto}, J.~L. and {Qvam}, J.~K.~T. and {Ranc}, C. and {Rebassa-Mansergas}, A. and {Reichart}, D.~E. and {Reig}, P. and {Rhodes}, L. and {Rivet}, J.-P. and {Rixon}, G. and {Roberts}, D. and {Rosi}, P. and {Russell}, D.~M. and {Zanmar Sanchez}, R. and {Scarpetta}, G. and {Seabroke}, G. and {Shappee}, B.~J. and {Schmidt}, R. and {Shvartzvald}, Y. and {Sitek}, M. and {Skowron}, J. and {{\'S}niegowska}, M. and {Snodgrass}, C. and {Soares}, P.~S. and {Spetsieri}, Z.~T. and {Stankeviciute}, A. and {Steele}, I.~A. and {Street}, R.~A. and {Strobl}, J. and {Tinjaca Ramirez}, L.~M. and {Tomasella}, L. and {Tsapras}, Y. and {Villanueva}, Jr., S. and {Vince}, O. and {Wambsganss}, J. and {Wiersema}, K. and {Wilson}, R.~W. and {Yoldas}, A. and {Zhuchkov}, R.~Y. and {Zhukov}, D.~G. and {Zdanavicius}, J. and {Zo{\l}a}, S. and {Zubareva}, A.}, title = "{Full Orbital Solution for the Binary System in the Northern Galactic Disk Microlensing Event Gaia16aye}", journal = {arXiv e-prints}, archivePrefix = "arXiv", eprint = {1901.07281}, primaryClass = "astro-ph.SR", keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics}, year = 2019, month = jan, adsurl = {http://adsabs.harvard.edu/abs/2019arXiv190107281W}, Url = {https://arxiv.org/pdf/1901.07281.pdf}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - M. Albayrak, K. Halicioglu, B. Basoglu, and Y. Kilic, “Investigating the Function of the Star Trails to Improve the Determination of Gravity Field,” in AGU Fall Meeting Abstracts, 2018, p. G51F-0529.
[BibTeX]@inproceedings{2018AGUFM.G51F0529A, author = {{Albayrak}, M. and {Halicioglu}, K. and {Basoglu}, B. and {Kilic}, Y.}, title = "{Investigating the Function of the Star Trails to Improve the Determination of Gravity Field}", keywords = {1217 Time variable gravity, GEODESY AND GRAVITYDE: 1219 Gravity anomalies and Earth structure, GEODESY AND GRAVITYDE: 1244 Standards and absolute measurements, GEODESY AND GRAVITYDE: 1294 Instruments and techniques, GEODESY AND GRAVITY}, booktitle = {AGU Fall Meeting Abstracts}, year = "2018", volume = {2018}, month = "Dec", eid = {G51F-0529}, pages = {G51F-0529}, adsurl = {https://ui.adsabs.harvard.edu/abs/2018AGUFM.G51F0529A}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - Y. Kilic, M. Kaplan, and Z. Eker, “A new pipeline for astrometry and photometry of asteroids,” Proceedings of the International Astronomical Union, vol. 14, iss. A30, p. 43–43, 2018. doi:10.1017/S1743921319003417
[BibTeX]@article{klc_kaplan_eker_2018, title={A new pipeline for astrometry and photometry of asteroids}, volume={14}, DOI={10.1017/S1743921319003417}, number={A30}, journal={Proceedings of the International Astronomical Union}, publisher={Cambridge University Press}, author={Kilic, Y. and Kaplan, M. and Eker, Z.}, year={2018}, pages={43–43}} - Y. Kilic, M. Dindar, T. Ozisik, M. ~T. Ozkan, and S. Ozdemir, “GRB180809B TUG T60 observations.,” GRB Coordinates Network, Circular Service, No.~23127, \#1 (2018/August-0), vol. 23127, 2018.
[BibTeX]@article{2018GCN.23127....1K, author = {{Kilic}, Y. and {Dindar}, M. and {Ozisik}, T. and {Ozkan}, M.~T. and {Ozdemir}, S.}, title = "{GRB180809B TUG T60 observations.}", journal = {GRB Coordinates Network, Circular Service, No.~23127, \#1 (2018/August-0)}, year = 2018, volume = 23127, adsurl = {http://adsabs.harvard.edu/abs/2018GCN.23127....1K}, adsnote = {Provided by the SAO/NASA Astrophysics Data System} } - Y. Kilic, O. Erece, and M. Kaplan, “Astrometry with A-Track Using Gaia DR1 Catalogue,” Proceedings of the International Astronomical Union, vol. 12, iss. S330, p. 94–95, 2017. doi:10.1017/S174392131700552X
[BibTeX]@article{kılıç_erece_kaplan_2017, title={Astrometry with A-Track Using Gaia DR1 Catalogue}, volume={12}, DOI={10.1017/S174392131700552X}, number={S330}, journal={Proceedings of the International Astronomical Union}, publisher={Cambridge University Press}, author={Kilic, Yucel and Erece, Orhan and Kaplan, Murat}, year={2017}, pages={94–95}} - M. Shameoni Niaei, Y. Kilic, B. ~E. Yildiran, F. Yüzlükoglu, and C. Yesilyaprak, “A New Effort for Atmospherical Forecast: Meteorological Image Processing Software (MIPS) for Astronomical Observations,” in Revista Mexicana de Astronomia y Astrofisica Conference Series, 2016, pp. 40-41.
[BibTeX] [Abstract] [Download PDF]
We have described a new software (MIPS) about the analysis and image processing of the meteorological satellite (Meteosat) data for an astronomical observatory. This software will be able to help to make some atmospherical forecast (cloud, humidity, rain) using meteosat data for robotic telescopes. MIPS uses a python library for Eumetsat data that aims to be completely open-source and licenced under GNU/General Public Licence (GPL). MIPS is a platform independent and uses h5py, numpy, and PIL with the general-purpose and high-level programming language Python and the QT framework.
@inproceedings{2016RMxAC..48...40S, Abstract = {We have described a new software (MIPS) about the analysis and image processing of the meteorological satellite (Meteosat) data for an astronomical observatory. This software will be able to help to make some atmospherical forecast (cloud, humidity, rain) using meteosat data for robotic telescopes. MIPS uses a python library for Eumetsat data that aims to be completely open-source and licenced under GNU/General Public Licence (GPL). MIPS is a platform independent and uses h5py, numpy, and PIL with the general-purpose and high-level programming language Python and the QT framework.}, Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, Adsurl = {http://adsabs.harvard.edu/abs/2016RMxAC..48...40S}, Author = {{Shameoni Niaei}, M. and {Kilic}, Y. and {Yildiran}, B.~E. and {Y{\"u}zl{\"u}koglu}, F. and {Yesilyaprak}, C.}, Booktitle = {Revista Mexicana de Astronomia y Astrofisica Conference Series}, Date-Added = {2017-02-05 15:48:59 +0000}, Date-Modified = {2017-02-06 21:15:08 +0000}, Keywords = {atmospheric effects , methods: numerical}, Month = dec, Pages = {40-41}, Rating = {5}, Series = {Revista Mexicana de Astronomia y Astrofisica Conference Series}, Title = {{A New Effort for Atmospherical Forecast: Meteorological Image Processing Software (MIPS) for Astronomical Observations}}, Url = {http://www.astroscu.unam.mx/rmaa/RMxAC..48/PDF/RMxAC..48_part-2.3.pdf}, Volume = 48, Year = 2016} - Y. Kilic, M. Shameoni Niaei, F. ~F. Özeren, and C. Yesilyaprak, “MYRaf: A new Approach with IRAF for Astronomical Photometric Reduction,” in Revista Mexicana de Astronomia y Astrofisica Conference Series, 2016, pp. 38-39.
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In this study, the design and some developments of MYRaf software for astronomical photometric reduction are presented. MYRaf software is an easy to use, reliable, and has a fast IRAF aperture photometry GUI tools. MYRaf software is an important step for the automated software process of robotic telescopes, and uses IRAF, PyRAF, matplotlib, ginga, alipy, and Sextractor with the general-purpose and high-level programming language Python and uses the QT framework.
@inproceedings{2016RMxAC..48...38K, Abstract = {In this study, the design and some developments of MYRaf software for astronomical photometric reduction are presented. MYRaf software is an easy to use, reliable, and has a fast IRAF aperture photometry GUI tools. MYRaf software is an important step for the automated software process of robotic telescopes, and uses IRAF, PyRAF, matplotlib, ginga, alipy, and Sextractor with the general-purpose and high-level programming language Python and uses the QT framework.}, Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, Adsurl = {http://adsabs.harvard.edu/abs/2016RMxAC..48...38K}, Author = {{Kilic}, Y. and {Shameoni Niaei}, M. and {{\"O}zeren}, F.~F. and {Yesilyaprak}, C.}, Booktitle = {Revista Mexicana de Astronomia y Astrofisica Conference Series}, Date-Added = {2017-02-05 15:48:59 +0000}, Date-Modified = {2017-02-06 21:15:23 +0000}, Keywords = {methods: data analysis, techniques: photometry}, Month = dec, Pages = {38-39}, Series = {Revista Mexicana de Astronomia y Astrofisica Conference Series}, Title = {{MYRaf: A new Approach with IRAF for Astronomical Photometric Reduction}}, Url = {http://www.astroscu.unam.mx/rmaa/RMxAC..48/PDF/RMxAC..48_part-2.2.pdf}, Volume = 48, Year = 2016} - T. Atay, M. Kaplan, Y. Kilic, and N. Karapinar, “A-Track: A new approach for detection of moving objects in \FITS\ images,” Computer Physics Communications, vol. 207, pp. 524-530, 2016. doi:http://dx.doi.org/10.1016/j.cpc.2016.07.023
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Abstract We have developed a fast, open-source, cross-platform pipeline, called A-Track, for detecting the moving objects (asteroids and comets) in sequential telescope images in \FITS\ format. The pipeline is coded in Python 3. The moving objects are detected using a modified line detection algorithm, called MILD. We tested the pipeline on astronomical data acquired by an SI-1100 \CCD\ with a 1-meter telescope. We found that A-Track performs very well in terms of detection efficiency, stability, and processing time. The code is hosted on GitHub under the \GNU\ \GPL\ v3 license. Program summary Program title: A-TRACK Catalogue identifier: AFBC_v1_0 Program summary URL:http://cpc.cs.qub.ac.uk/summaries/AFBC_v1_0.html Program obtainable from: \CPC\ Program Library, Queen’s University, Belfast, N. Ireland Licensing provisions: \GNU\ General Public Licence Version 3 No. of lines in distributed program, including test data, etc.: 313100 No. of bytes in distributed program, including test data, etc.: 89443558 Distribution format: tar.gz Programming language: Python 3. Computer: Personal Computer. Operating system: Any ØS\ where Python 3 and subprograms are installed. Classification: 14. External routines: Numpy, Pandas, SExtractor, PyFITS, Alipy, f2n, docopt, Imagemagick, git-all, scipy, matplatlib, astroasciidata. Nature of problem: Asteroid and comet detection. Solution method: A multiple image line detection algorithm for sequential \FITS\ images. Running time:∼1 min
@article{Atay2016524, Abstract = {Abstract We have developed a fast, open-source, cross-platform pipeline, called A-Track, for detecting the moving objects (asteroids and comets) in sequential telescope images in \{FITS\} format. The pipeline is coded in Python 3. The moving objects are detected using a modified line detection algorithm, called MILD. We tested the pipeline on astronomical data acquired by an SI-1100 \{CCD\} with a 1-meter telescope. We found that A-Track performs very well in terms of detection efficiency, stability, and processing time. The code is hosted on GitHub under the \{GNU\} \{GPL\} v3 license. Program summary Program title: A-TRACK Catalogue identifier: AFBC_v1_0 Program summary URL:http://cpc.cs.qub.ac.uk/summaries/AFBC_v1_0.html Program obtainable from: \{CPC\} Program Library, Queen's University, Belfast, N. Ireland Licensing provisions: \{GNU\} General Public Licence Version 3 No. of lines in distributed program, including test data, etc.: 313100 No. of bytes in distributed program, including test data, etc.: 89443558 Distribution format: tar.gz Programming language: Python 3. Computer: Personal Computer. Operating system: Any \{OS\} where Python 3 and subprograms are installed. Classification: 14. External routines: Numpy, Pandas, SExtractor, PyFITS, Alipy, f2n, docopt, Imagemagick, git-all, scipy, matplatlib, astroasciidata. Nature of problem: Asteroid and comet detection. Solution method: A multiple image line detection algorithm for sequential \{FITS\} images. Running time:∼1 min }, Author = {T. Atay and M. Kaplan and Y. Kilic and N. Karapinar}, Date-Modified = {2017-02-05 15:57:37 +0000}, Doi = {http://dx.doi.org/10.1016/j.cpc.2016.07.023}, Issn = {0010-4655}, Journal = {Computer Physics Communications}, Keywords = {Image processing}, Month = {October}, Pages = {524 - 530}, Title = {A-Track: A new approach for detection of moving objects in \{FITS\} images}, Url = {//www.sciencedirect.com/science/article/pii/S0010465516302119}, Volume = {207}, Year = {2016}, Bdsk-Url-1 = {//www.sciencedirect.com/science/article/pii/S0010465516302119}, Bdsk-Url-2 = {http://dx.doi.org/10.1016/j.cpc.2016.07.023}} - M. ~S. Niaei, Y. Kilic, and F. ~F. Özeren, “MYRaf: An Easy Aperture Photometry GUI for IRAF,” in Living Together: Planets, Host Stars and Binaries, 2015, p. 299.
[BibTeX] [Abstract] [Download PDF]
We describe the design and development of MYRaf, a GUI (Graphical User Interface) that aims to be completely open-source under General Public License (GPL). MYRaf is an easy to use, reliable, and a fast IRAF aperture photometry GUI tool for those who are conversant with text-based software and command-line procedures in GNU/Linux OSs. MYRaf uses IRAF, PyRAF, matplotlib, ginga, alipy, and SExtractor with the general-purpose and high-level programming language Python, and uses the Qt framework.
@inproceedings{2015ASPC..496..299N, Abstract = {We describe the design and development of MYRaf, a GUI (Graphical User Interface) that aims to be completely open-source under General Public License (GPL). MYRaf is an easy to use, reliable, and a fast IRAF aperture photometry GUI tool for those who are conversant with text-based software and command-line procedures in GNU/Linux OSs. MYRaf uses IRAF, PyRAF, matplotlib, ginga, alipy, and SExtractor with the general-purpose and high-level programming language Python, and uses the Qt framework.}, Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, Adsurl = {http://adsabs.harvard.edu/abs/2015ASPC..496..299N}, Author = {{Niaei}, M.~S. and {Kilic}, Y. and {{\"O}zeren}, F.~F.}, Booktitle = {Living Together: Planets, Host Stars and Binaries}, Date-Added = {2017-02-05 15:48:59 +0000}, Date-Modified = {2017-02-06 21:17:49 +0000}, Editor = {{Rucinski}, S.~M. and {Torres}, G. and {Zejda}, M.}, Month = jul, Pages = {299}, Series = {Astronomical Society of the Pacific Conference Series}, Title = {{MYRaf: An Easy Aperture Photometry GUI for IRAF}}, Url = {http://aspbooks.org/publications/496/299.pdf}, Volume = 496, Year = 2015} - Z. Terzioglu, H. Gursoytrak, G. Saral, N. Bagiran, G. Gokay, Y. Kilic, Y. Demircan, A. Okan, M. ~B. Dogruel, M. Alpsoy, S. Cerit, M. Semuni, C. Yildirim, and B. Gurol, “Minima Times of Some Eclipsing Binary Stars,” Information Bulletin on Variable Stars, vol. 6128, 2015.
[BibTeX] [Abstract] [Download PDF]
We present several CCD minima observations of eclipsing binaries.
@article{2015IBVS.6128....1T, Abstract = {We present several CCD minima observations of eclipsing binaries.}, Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, Adsurl = {http://adsabs.harvard.edu/abs/2015IBVS.6128....1T}, Author = {{Terzioglu}, Z. and {Gursoytrak}, H. and {Saral}, G. and {Bagiran}, N. and {Gokay}, G. and {Kilic}, Y. and {Demircan}, Y. and {Okan}, A. and {Dogruel}, M.~B. and {Alpsoy}, M. and {Cerit}, S. and {Semuni}, M. and {Yildirim}, C. and {Gurol}, B.}, Date-Added = {2017-02-05 15:48:59 +0000}, Date-Modified = {2017-02-06 21:17:44 +0000}, Journal = {Information Bulletin on Variable Stars}, Month = jan, Title = {{Minima Times of Some Eclipsing Binary Stars}}, Url = {http://www.konkoly.hu/cgi-bin/IBVSpdf?6128}, Volume = 6128, Year = 2015} - B. ~B. Gucsav, Y. Kilic, and M. ~N. Shameoni, “ATA50 telescope: software,” in Revista Mexicana de Astronomia y Astrofisica Conference Series, 2014, pp. 30-31.
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We aim to implement a fully autonomous observatory structure for ATA50 telescope. All components of the observatory are currently controlled by manual MS Windows applications. A well designed OCS such as RTS2 might provide us a quick solution. GNU/Linux is our choice for the OS by considering the open-source philosophy and the original development environment of RTS2 (Kubanek et al. 2006). As expected, we have faced absent/painful driver issues for our equipment. The compromise for the above has made for coding the physical component drivers regarding development of a huge and complex OCS.
@inproceedings{2014RMxAC..45...30G, Abstract = {We aim to implement a fully autonomous observatory structure for ATA50 telescope. All components of the observatory are currently controlled by manual MS Windows applications. A well designed OCS such as RTS2 might provide us a quick solution. GNU/Linux is our choice for the OS by considering the open-source philosophy and the original development environment of RTS2 (Kubanek et al. 2006). As expected, we have faced absent/painful driver issues for our equipment. The compromise for the above has made for coding the physical component drivers regarding development of a huge and complex OCS.}, Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, Adsurl = {http://adsabs.harvard.edu/abs/2014RMxAC..45...30G}, Author = {{Gucsav}, B.~B. and {Kilic}, Y. and {Shameoni}, M.~N.}, Booktitle = {Revista Mexicana de Astronomia y Astrofisica Conference Series}, Date-Added = {2017-02-05 15:48:59 +0000}, Date-Modified = {2017-02-06 21:17:22 +0000}, Keywords = {methods: data analysis, techniques: image processing, instrumentation: miscellaneous, telescopes}, Month = dec, Pages = {30-31}, Series = {Revista Mexicana de Astronomia y Astrofisica Conference Series}, Title = {{ATA50 telescope: software}}, Url = {http://www.astroscu.unam.mx/rmaa/RMxAC..45/PDF/RMxAC..45_file1-09.pdf}, Volume = 45, Year = 2014} - C. Yec silyaprak, S. ~K. Yerli, N. Aksaker, Y. Yildiran, Y. Güney, B. ~B. Güc csav, F. ~F. Özeren, Y. Kilic, M. ~N. Shameoni, S. Fic sek, G. Kilic cerkan, \. I. Nasirou glu, E. ~E. Özbaldan, and E. Yac sar, “ATA50 telescope: hardware,” in Revista Mexicana de Astronomia y Astrofisica Conference Series, 2014, pp. 28-29.
[BibTeX] [Abstract] [Download PDF]
ATA50 Telescope is a new telescope with RC optics and 50 cm diameter. It was supported by Atatürk University Scientific Research Project (2010) and established at about 2000 meters altitude in city of Erzurum in Turkey last year. The observations were started a few months ago under the direction and control of Atatürk University Astrophysics Research and Application Center (ATASAM). The technical properties and infrastructures of ATA50 Telescope are presented and we have been working on the robotic automation of the telescope as hardware and software in order to be a ready-on-demand candidate for both national and international telescope networks.
@inproceedings{2014RMxAC..45...28Y, Abstract = {ATA50 Telescope is a new telescope with RC optics and 50 cm diameter. It was supported by Atat{\"u}rk University Scientific Research Project (2010) and established at about 2000 meters altitude in city of Erzurum in Turkey last year. The observations were started a few months ago under the direction and control of Atat{\"u}rk University Astrophysics Research and Application Center (ATASAM). The technical properties and infrastructures of ATA50 Telescope are presented and we have been working on the robotic automation of the telescope as hardware and software in order to be a ready-on-demand candidate for both national and international telescope networks.}, Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, Adsurl = {http://adsabs.harvard.edu/abs/2014RMxAC..45...28Y}, Author = {{Ye{\c s}ilyaprak}, C. and {Yerli}, S.~K. and {Aksaker}, N. and {Yildiran}, Y. and {G{\"u}ney}, Y. and {G{\"u}{\c c}sav}, B.~B. and {{\"O}zeren}, F.~F. and {Kilic}, Y. and {Shameoni}, M.~N. and {Fi{\c s}ek}, S. and {Kili{\c c}erkan}, G. and {Nasiro{\u g}lu}, {\.I}. and {{\"O}zbaldan}, E.~E. and {Ya{\c s}ar}, E.}, Booktitle = {Revista Mexicana de Astronomia y Astrofisica Conference Series}, Date-Added = {2017-02-05 15:48:59 +0000}, Date-Modified = {2017-02-06 21:16:31 +0000}, Keywords = {instrumentation: miscellaneous, telescopes}, Month = dec, Pages = {28-29}, Series = {Revista Mexicana de Astronomia y Astrofisica Conference Series}, Title = {{ATA50 telescope: hardware}}, Url = {http://www.astroscu.unam.mx/rmaa/RMxAC..45/PDF/RMxAC..45_file1-08.pdf}, Volume = 45, Year = 2014} - H. Gursoytrak, Y. Demircan, G. Gokay, A. Okan, Z. Terzioglu, G. Saral, M. Semuni, Y. Kilic, S. Cerit, M. Alpsoy, A. Yolkolu, S. Sahin, and B. Gurol, “New times of minima for some eclipsing binary stars,” Information Bulletin on Variable Stars, vol. 6075, 2013.
[BibTeX] [Abstract] [Download PDF]
We present several CCD minima observations of eclipsing binaries.
@article{2013IBVS.6075....1G, Abstract = {We present several CCD minima observations of eclipsing binaries.}, Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, Adsurl = {http://adsabs.harvard.edu/abs/2013IBVS.6075....1G}, Author = {{Gursoytrak}, H. and {Demircan}, Y. and {Gokay}, G. and {Okan}, A. and {Terzioglu}, Z. and {Saral}, G. and {Semuni}, M. and {Kilic}, Y. and {Cerit}, S. and {Alpsoy}, M. and {Yolkolu}, A. and {Sahin}, S. and {Gurol}, B.}, Date-Added = {2017-02-05 15:48:59 +0000}, Date-Modified = {2017-02-06 21:16:46 +0000}, Journal = {Information Bulletin on Variable Stars}, Keywords = {CCD photometry}, Month = sep, Title = {{New times of minima for some eclipsing binary stars}}, Url = {http://www.konkoly.hu/cgi-bin/IBVSpdf?6075}, Volume = 6075, Year = 2013} - Y. Demircan, G. Gokay, A. Okan, H. Gursoytrak, Z. Terzioglu, G. Saral, Y. Kilic, S. Cerit, M. Semuni, E. Aydin, U. Demirhan, and B. Gurol, “Times of Minima of some eclipsing binary stars,” Information Bulletin on Variable Stars, vol. 6041, 2012.
[BibTeX] [Abstract] [Download PDF]
We present several CCD minima observations of eclipsing binaries.
@article{2012IBVS.6041....1D, Abstract = {We present several CCD minima observations of eclipsing binaries.}, Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, Adsurl = {http://adsabs.harvard.edu/abs/2012IBVS.6041....1D}, Author = {{Demircan}, Y. and {Gokay}, G. and {Okan}, A. and {Gursoytrak}, H. and {Terzioglu}, Z. and {Saral}, G. and {Kilic}, Y. and {Cerit}, S. and {Semuni}, M. and {Aydin}, E. and {Demirhan}, U. and {Gurol}, B.}, Date-Added = {2017-02-05 15:48:59 +0000}, Date-Modified = {2017-02-06 21:16:54 +0000}, Journal = {Information Bulletin on Variable Stars}, Keywords = {CCD photometry}, Month = dec, Title = {{Times of Minima of some eclipsing binary stars}}, Url = {http://www.konkoly.hu/cgi-bin/IBVSpdf?6041}, Volume = 6041, Year = 2012} - G. Gokay, Y. Demircan, H. Gursoytrak, Z. Terzioglu, A. Okan, M. ~B. Dogruel, G. Saral, S. Cerit, M. Semuni, Y. Kilic, D. Coker, E. Derman, and B. Gurol, “Minima times of some eclipsing binary stars,” Information Bulletin on Variable Stars, vol. 6039, 2012.
[BibTeX] [Abstract] [Download PDF]
We present several CCD minima observations of eclipsing binaries.
@article{2012IBVS.6039....1G, Abstract = {We present several CCD minima observations of eclipsing binaries.}, Adsnote = {Provided by the SAO/NASA Astrophysics Data System}, Adsurl = {http://adsabs.harvard.edu/abs/2012IBVS.6039....1G}, Author = {{Gokay}, G. and {Demircan}, Y. and {Gursoytrak}, H. and {Terzioglu}, Z. and {Okan}, A. and {Dogruel}, M.~B. and {Saral}, G. and {Cerit}, S. and {Semuni}, M. and {Kilic}, Y. and {Coker}, D. and {Derman}, E. and {Gurol}, B.}, Date-Added = {2017-02-05 15:48:59 +0000}, Date-Modified = {2017-02-06 21:17:00 +0000}, Journal = {Information Bulletin on Variable Stars}, Keywords = {CCD photometry}, Month = nov, Title = {{Minima times of some eclipsing binary stars}}, Url = {http://www.konkoly.hu/cgi-bin/IBVSpdf?6039}, Volume = 6039, Year = 2012}
Articles in National Journals and Proceedings
- M. ~S. Niaei, Y. Kilic, E. Gunseli, T. Cakir, and G. Karagoz, “Astrofotoğrafçılık,” in XVII. Ulusal Astronomi Kongresi Bildiri Kitabı, 2010.
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Bu çalışmada baz uzak gök cisimlerinin Ankara Üniversitesi Gözlemevi’nde bulunan T40 Kreiken Teleskobuna bağlı Apogee ALTA U47+ CCD Kamera ile görüntüleri RGB filtrelerinde alınmıştır. MaximDL programı ile indirgenmiş, Adobe Fits Liberator ile renklendirilmesi yapılmıştır. Üç proje dönemi boyunca toplam beş gün bu proje işin tahsis edilmiştir. Hava şartları dört gün gözlem yapmaya izin vermiştir. Her gözlem döneminde bir öncekinde yapılan hatalardan arındırılmış daha kaliteli veriler alınmış, eksiklikler giderilmiştir. Bu çalışmada renklendirme işleminin nasıl yapıldığı anlatılmıştır. İlave olarak da karşılaşılan renk sapıncı ve uzun süreli takip problemlerinin nasıl giderildiklerine değinilmiştir.
@inproceedings{astrophoto, Abstract = {Bu çalışmada baz uzak g{\"o}k cisimlerinin Ankara {\"U}niversitesi G{\"o}zlemevi'nde bulunan T40 Kreiken Teleskobuna bağlı Apogee ALTA U47+ CCD Kamera ile g{\"o}r{\"u}nt{\"u}leri RGB filtrelerinde alınmıştır. MaximDL programı ile indirgenmiş, Adobe Fits Liberator ile renklendirilmesi yapılmıştır. {\"U}ç proje d{\"o}nemi boyunca toplam beş g{\"u}n bu proje işin tahsis edilmiştir. Hava şartları d{\"o}rt g{\"u}n g{\"o}zlem yapmaya izin vermiştir. Her g{\"o}zlem d{\"o}neminde bir {\"o}ncekinde yapılan hatalardan arındırılmış daha kaliteli veriler alınmış, eksiklikler giderilmiştir. Bu çalışmada renklendirme işleminin nasıl yapıldığı anlatılmıştır. İlave olarak da karşılaşılan renk sapıncı ve uzun s{\"u}reli takip problemlerinin nasıl giderildiklerine değinilmiştir.}, Author = {{Niaei}, M.~S. and {Kilic}, Y. and {Gunseli}, E. and {Cakir}, T. and {Karagoz}, G.}, Booktitle = {XVII. Ulusal Astronomi Kongresi Bildiri Kitabı}, Date-Added = {2017-02-06 22:40:43 +0000}, Date-Modified = {2017-02-07 20:37:20 +0000}, Month = {September}, Title = {Astrofotoğrafçılık}, Url = {https://yadi.sk/i/afsbe7VN3DQAyu}, Year = {2010}, Bdsk-Url-1 = {https://yadi.sk/i/afsbe7VN3DQAyu}} - Y. Kilic, S. Ozdemir, E. Aydin, O. Okuyan, N. Bagiran, and S. Sahin, “DIBRED: Canon 550D Kamerası Görüntülerinden FITS Formatlı Astronomik Görüntülere Dönüşüm ve Fotometri Yazılım,” in XVIII. Ulusal Astronomi ve Uzay Bilimleri Kongresi Bildiri Kitabı, 2012, pp. 449-454.
[BibTeX] [Abstract] [Download PDF]
Bu çalışmada, Diyanet İşleri Başkanlığı ve Ankara Üniversitesi Rektörlüğünce ortak sürdürülen “Ufuk Aydınlanma (Tan ve Fecir) Vakitlerinin Gözlemsel Yolla Belirlenmesi” konulu proje çerçevesinde geliştirilen, bir RAW – FITS dönuşüm ve fotometri modülleri (DIBRED) ayrıntılı olarak tanıtılmaktadır. Bilindiği gibi, astronomik görüntülerin ışıkölçüm amaçlı kullanılabilmesi için FITS formatında kayıt edilmiş olması gereklidir. Fotoğraf makinaları bu ayrıntı düşünülerek üretilmemişlerdir. Oysa fotoğraf makinalarının geniş açı görebilme özelliği, astronomik ışıkölçümünde, özellikle gökyüzü taramalarında, çok aranan bir ozelliktir. Bahsi geçen projede, ufuk aydınlığının zamana bağlı değişim eğrileri, bir Canon 550D DSLR kamerası kullanılarak kaydedilmektedir. Bu bildiride, Canon 550D DSLR kamerasına ait görüntülerin DIBRED yazılımı ile, R, G ve B bantlarına ayrılması, FITS formatlı görüntülere dönüştürülmesi ve bu görüntüler üzerinde uygulanan ışık ölçüm yöntemi açıklanmaktadır.
@inproceedings{dibred, Abstract = {Bu çalışmada, Diyanet İşleri Başkanlığı ve Ankara {\"U}niversitesi Rekt{\"o}rl{\"u}ğ{\"u}nce ortak s{\"u}rd{\"u}r{\"u}len "Ufuk Aydınlanma (Tan ve Fecir) Vakitlerinin G{\"o}zlemsel Yolla Belirlenmesi" konulu proje çerçevesinde geliştirilen, bir RAW - FITS d{\"o}nuş{\"u}m ve fotometri mod{\"u}lleri (DIBRED) ayrıntılı olarak tanıtılmaktadır. Bilindiği gibi, astronomik g{\"o}r{\"u}nt{\"u}lerin ışık{\"o}lç{\"u}m amaçlı kullanılabilmesi için FITS formatında kayıt edilmiş olması gereklidir. Fotoğraf makinaları bu ayrıntı d{\"u}ş{\"u}n{\"u}lerek {\"u}retilmemişlerdir. Oysa fotoğraf makinalarının geniş açı g{\"o}rebilme {\"o}zelliği, astronomik ışık{\"o}lç{\"u}m{\"u}nde, {\"o}zellikle g{\"o}ky{\"u}z{\"u} taramalarında, çok aranan bir ozelliktir. Bahsi geçen projede, ufuk aydınlığının zamana bağlı değişim eğrileri, bir Canon 550D DSLR kamerası kullanılarak kaydedilmektedir. Bu bildiride, Canon 550D DSLR kamerasına ait g{\"o}r{\"u}nt{\"u}lerin DIBRED yazılımı ile, R, G ve B bantlarına ayrılması, FITS formatlı g{\"o}r{\"u}nt{\"u}lere d{\"o}n{\"u}şt{\"u}r{\"u}lmesi ve bu g{\"o}r{\"u}nt{\"u}ler {\"u}zerinde uygulanan ışık {\"o}lç{\"u}m y{\"o}ntemi açıklanmaktadır.}, Author = {{Kilic}, Y. and {Ozdemir}, S. and {Aydin}, E. and {Okuyan}, O. and {Bagiran}, N. and {Sahin}, S.}, Booktitle = {XVIII. Ulusal Astronomi ve Uzay Bilimleri Kongresi Bildiri Kitabı}, Date-Added = {2017-02-06 22:37:13 +0000}, Date-Modified = {2017-02-07 20:36:37 +0000}, Month = {September}, Organization = {İnon{\"u} {\"U}niversitesi}, Pages = {449-454}, Title = {DIBRED: Canon 550D Kamerası G{\"o}r{\"u}nt{\"u}lerinden FITS Formatlı Astronomik G{\"o}r{\"u}nt{\"u}lere D{\"o}n{\"u}ş{\"u}m ve Fotometri Yazılım}, Url = {https://yadi.sk/i/-jnmpcZr3DQGaS}, Year = {2012}, Bdsk-Url-1 = {https://yadi.sk/i/-jnmpcZr3DQGaS}} - Y. Kilic and M. Shameoni Niaei, “EUMETSAT Verilerinin İşletim Sistemi Bağımsız Yorumlanması ve Görüntülenmesi,” in I. Meteorolojik Uzaktan Algılama Çalıştayı Bildiri Kitabı, 2013, pp. 359-367.
[BibTeX] [Abstract] [Download PDF]
EUMETSAT uydusundan gelen verileri almak, işlemek ve gerektiğinde görüntülemek hâli hazırda EumetCast yazılımıyla mümkündür; bununla birlikte alınan verilerin boyutu ve söz konusu yazılımın istemci bilgisayarında kullandığı sistem kaynağı göz önüne alındığında pek iyi bir seçim olmadığı görülebilir. Bu bağlamda, Erdem ERDİ’nin geliştirdiği ve Qt framework ile desteklediği TMet pro (verilerin alınması) ve TMet vis (alınan verilerin görüntülenmesi) yazılımlarını kullanmak daha uygun olur. Söz konusu yazılımlar yalnızca MS Windows türevi işletim sistemlerinde çalıştığından, ATASAM ekibi olarak Python ve Qt kullanılarak TMet vis’in işletim sisteminin bağımsız bir sürümünü, Camiryo’yu geliştirdi. Camiryo, TMet’i esas alıp TMet’in bir alt projesi konumundadır.
@inproceedings{muac, Abstract = {EUMETSAT uydusundan gelen verileri almak, işlemek ve gerektiğinde g{\"o}r{\"u}nt{\"u}lemek h{\^a}li hazırda EumetCast yazılımıyla m{\"u}mk{\"u}nd{\"u}r; bununla birlikte alınan verilerin boyutu ve s{\"o}z konusu yazılımın istemci bilgisayarında kullandığı sistem kaynağı g{\"o}z {\"o}n{\"u}ne alındığında pek iyi bir seçim olmadığı g{\"o}r{\"u}lebilir. Bu bağlamda, Erdem ERDİ'nin geliştirdiği ve Qt framework ile desteklediği TMet pro (verilerin alınması) ve TMet vis (alınan verilerin g{\"o}r{\"u}nt{\"u}lenmesi) yazılımlarını kullanmak daha uygun olur. S{\"o}z konusu yazılımlar yalnızca MS Windows t{\"u}revi işletim sistemlerinde çalıştığından, ATASAM ekibi olarak Python ve Qt kullanılarak TMet vis'in işletim sisteminin bağımsız bir s{\"u}r{\"u}m{\"u}n{\"u}, Camiryo'yu geliştirdi. Camiryo, TMet'i esas alıp TMet'in bir alt projesi konumundadır.}, Author = {{Kilic}, Y. and {Shameoni Niaei}, M.}, Booktitle = {I. Meteorolojik Uzaktan Algılama Çalıştayı Bildiri Kitabı}, Date-Added = {2017-02-06 22:34:08 +0000}, Date-Modified = {2017-02-07 21:09:00 +0000}, Month = {November}, Pages = {359-367}, Publisher = {Meteoroloji Genel M{\"u}d{\"u}rl{\"u}ğ{\"u}}, Title = {EUMETSAT Verilerinin İşletim Sistemi Bağımsız Yorumlanması ve G{\"o}r{\"u}nt{\"u}lenmesi}, Url = {https://yadi.sk/i/WPSZVeoG3DQQju}, Year = {2013}, Bdsk-Url-1 = {https://yadi.sk/i/WPSZVeoG3DQQju}} - I. Nasiroglu, Y. Guney, Y. Kilic, M. Shameoni Niaei, and B. Tozoglu, “Atatürk Üniversitesinde Işık Kirliliği Ölçümü,” in XIX. Ulusal Astronomi Kongresi Bildiri Kitabı, 2015.
[BibTeX] [Abstract] [Download PDF]
Işık kirliliği, astronomide gökyüzü kalitesini etkileyen en önemli nedenlerden birisidir. Işık kirliliği, ışığın yanlış yerde ve zamanda, yanlış miktarda ve yönde kullanılması olarak tanımlanabilir. Işık kirliliğini ölçmek işin SQM (Sky Quality Meter) olarak bilinen ‘Gökyüzü Kalite ölçer’ cihazı kullanılmaktadır. Bu cihaz ile istenilen yöndeki aydınlanma etkisi tespit edilerek astronomik açıdan sönük hangi parlaklıktaki yıldızın gözlenebildiği belirlenebilmektedir. Bu çalışmada, Atatürk Üni. yerleşkesi ve bu yerleşkede yer alan ATA50 (Atatürk üni. Astrofizik Araştırma Teleskobu) teleskobunun çevresinde SQM cihazı kullanılarak gece gökyüzü parlaklığı ölçümleri yapılmıştır.
@inproceedings{isik_kirliligi, Abstract = {Işık kirliliği, astronomide g{\"o}ky{\"u}z{\"u} kalitesini etkileyen en {\"o}nemli nedenlerden birisidir. Işık kirliliği, ışığın yanlış yerde ve zamanda, yanlış miktarda ve y{\"o}nde kullanılması olarak tanımlanabilir. Işık kirliliğini {\"o}lçmek işin SQM (Sky Quality Meter) olarak bilinen 'G{\"o}ky{\"u}z{\"u} Kalite {\"o}lçer' cihazı kullanılmaktadır. Bu cihaz ile istenilen y{\"o}ndeki aydınlanma etkisi tespit edilerek astronomik açıdan s{\"o}n{\"u}k hangi parlaklıktaki yıldızın g{\"o}zlenebildiği belirlenebilmektedir. Bu çalışmada, Atat{\"u}rk {\"U}ni. yerleşkesi ve bu yerleşkede yer alan ATA50 (Atat{\"u}rk {\"u}ni. Astrofizik Araştırma Teleskobu) teleskobunun çevresinde SQM cihazı kullanılarak gece g{\"o}ky{\"u}z{\"u} parlaklığı {\"o}lç{\"u}mleri yapılmıştır.}, Author = {{Nasiroglu}, I. and {Guney}, Y. and {Kilic}, Y. and {Shameoni Niaei}, M. and {Tozoglu}, B.}, Booktitle = {XIX. Ulusal Astronomi Kongresi Bildiri Kitabı}, Date-Added = {2017-02-06 22:27:14 +0000}, Date-Modified = {2017-02-07 20:36:25 +0000}, Month = {February}, Organization = {METU}, Title = {Atat{\"u}rk {\"U}niversitesinde Işık Kirliliği {\"O}lç{\"u}m{\"u}}, Url = {https://yadi.sk/i/mWdita0h3DQHwL}, Year = {2015}, Bdsk-Url-1 = {https://yadi.sk/i/mWdita0h3DQHwL}}
Master’s Thesis
- Y. Kilic, “Bazı Beta Lyrae Türü Örten Değişen Çift Yıldızların Fotometrisi, Işık Eğrisi ve Dönem Analizi,” Master Thesis, Ankara Üniversitesi Fen Bilimleri Enstitüsü Astronomi ve Uzay Bilimleri Anabilim Dalı, 2013.
[BibTeX] [Abstract] [Download PDF]
Bu çalışmada Beta Lyrae türü örten değişen olarak sınıflandırılan CP Cam (GSC 04057-02457, HIP 15321, TYC 4057-2457-1), DZ Lyn (GSC 02979-02218, HD 67894, TYC 2979-2218-1) ve EG Cep (HD 194089, SAO 9710, GSC 04585-00063, TYC 4585-63-1) sistemlerinin geometrik ve fiziksel parametreleri elde edilmiştir. Fotometrik gözlemleri Ankara Üniversitesi Gözlemevi (AÜG)’nde bulunan 0.4m çaplı Kreiken Teleskobu (T40) ve ona bağlı Apogee ALTA U47+ CCD kamerası kullanılarak, Johnson BVRI filtrelerinde gerçekleştirilmiştir. Literatürde EB-türü olarak sınıflandırılan bu sistemlerin literatürde mevcut minimum zamanları ve kendi gözlemlerimizden hesaplanan minimum zamanları ile birlikte (O-C) analizi gerçekleştirilmiş ve olası açıklamalarda bulunulmuştur. Sistemlerin yeni ışık elemanları belirlenerek ışık ve mümkün olması durumunda ise dikine hız eğrileri birlikte analiz edilmiştir. Dikkate alınan sistemlerin standart sistemdeki parlaklık ve renk eğrileri yine bu çalışmada elde edilmiştir. Gerçekleştirilen çalışma sonucunda ele alınan sistemlere ilişkin geometrik ve fiziksel parametreler hesaplanmış ve sistemlerin evrimsel durumları tartışılmıştır. Gözlemsel verilerin indirgenmesi IRAF (Image Reduction and Analysis Facility) programı kullanılarak gerçekleştirilmiştir. Işık ve dikine hız eğrisi analizlerinde ise Wilson-Devinney 2007 sürümünü kullanan PHOEBE (PHysics Of Eclipsing Binaries) 0.31a programı ve sistemlerden birinde ise Nisan 2013’de yayınlanmış bulunan Wilson-Devinney programının 2013 sürümü kullanılmıştır.
@mastersthesis{yl_tez, Abstract = {Bu çalışmada Beta Lyrae türü örten değişen olarak sınıflandırılan CP Cam (GSC 04057-02457, HIP 15321, TYC 4057-2457-1), DZ Lyn (GSC 02979-02218, HD 67894, TYC 2979-2218-1) ve EG Cep (HD 194089, SAO 9710, GSC 04585-00063, TYC 4585-63-1) sistemlerinin geometrik ve fiziksel parametreleri elde edilmiştir. Fotometrik gözlemleri Ankara Üniversitesi Gözlemevi (AÜG)'nde bulunan 0.4m çaplı Kreiken Teleskobu (T40) ve ona bağlı Apogee ALTA U47+ CCD kamerası kullanılarak, Johnson BVRI filtrelerinde gerçekleştirilmiştir. Literatürde EB-türü olarak sınıflandırılan bu sistemlerin literatürde mevcut minimum zamanları ve kendi gözlemlerimizden hesaplanan minimum zamanları ile birlikte (O-C) analizi gerçekleştirilmiş ve olası açıklamalarda bulunulmuştur. Sistemlerin yeni ışık elemanları belirlenerek ışık ve mümkün olması durumunda ise dikine hız eğrileri birlikte analiz edilmiştir. Dikkate alınan sistemlerin standart sistemdeki parlaklık ve renk eğrileri yine bu çalışmada elde edilmiştir. Gerçekleştirilen çalışma sonucunda ele alınan sistemlere ilişkin geometrik ve fiziksel parametreler hesaplanmış ve sistemlerin evrimsel durumları tartışılmıştır. Gözlemsel verilerin indirgenmesi IRAF (Image Reduction and Analysis Facility) programı kullanılarak gerçekleştirilmiştir. Işık ve dikine hız eğrisi analizlerinde ise Wilson-Devinney 2007 sürümünü kullanan PHOEBE (PHysics Of Eclipsing Binaries) 0.31a programı ve sistemlerden birinde ise Nisan 2013'de yayınlanmış bulunan Wilson-Devinney programının 2013 sürümü kullanılmıştır.}, Address = {Ankara Üniversitesi Fen Bilimleri Enstitüsü Astronomi ve Uzay Bilimleri Anabilim Dalı}, Author = {{Kilic}, Y.}, Date-Added = {2017-02-07 21:35:54 +0000}, Date-Modified = {2017-02-07 21:43:03 +0000}, Keywords = {{\c C}ift yıldızlar, Binary stars}, Month = {June}, School = {Ankara {\"U}niversitesi}, Title = {Bazı Beta Lyrae Türü Örten Değişen Çift Yıldızların Fotometrisi, Işık Eğrisi ve Dönem Analizi}, Url = {https://tez.yok.gov.tr/UlusalTezMerkezi/TezGoster?key=vVNzTGHHhjH-u3WMToxQ-uweGc5WfnRh365D0RMndue3FNoHr35VRB5KdERT6sAJ}, Year = {2013}}
PhD Thesis
- Y. Kilic, “Investigation of solar system bodies by stellar occultation technique,” PhD Thesis, Akdeniz University, Institute of Natural and Applied Sciences, Space Science and Technologies Department.
[BibTeX] [Abstract] [Download PDF]
The importance of minor planets in the Solar System is increasing day by day in order to understand the evolution of the Solar System. Especially with the developing high technology, the enormous advances in the ground and space-based telescopes and detectors are rapidly increasing the number of discovered asteroids. These developments significantly increase the interest in Near-Earth Asteroids are also the subject of various space missions, such as protecting the Earth from potentially hazardous asteroids or asteroids mining, as well as the current interest in asteroids in the main belt. However, studies on objects beyond Neptune also attract the attention of researchers as these objects contain essential information about the early stages of the Solar System. For this purpose, in this thesis, the stellar occultation observation technique, which can reveal extremely detailed information about the size, shape, atmospheric structure, and existence of rings and satellites of minor planets in the Solar System, is described in detail. A web-based platform called Occultation Portal (OP) has been developed for the analysis, archiving and visualization of the data obtained by this observation technique, and the operation and architecture of this platform are explained in detail. Finally, the observations of (28978) Ixion (2001 KX76), a Trans-Neptune Object on which campaign observations were made on this platform, dated October 13, 2020, and April 28, 2021, were examined in detail for the first time with this study, and its physical parameters were determined and discussed in the thesis. In addition, the stellar diameter of the occulted star was obtained by analyzing the observation data dated October 13, 2020, and our findings were compared with previous studies.
@phdthesis{phd_thesis, Abstract = {The importance of minor planets in the Solar System is increasing day by day in order to understand the evolution of the Solar System. Especially with the developing high technology, the enormous advances in the ground and space-based telescopes and detectors are rapidly increasing the number of discovered asteroids. These developments significantly increase the interest in Near-Earth Asteroids are also the subject of various space missions, such as protecting the Earth from potentially hazardous asteroids or asteroids mining, as well as the current interest in asteroids in the main belt. However, studies on objects beyond Neptune also attract the attention of researchers as these objects contain essential information about the early stages of the Solar System. For this purpose, in this thesis, the stellar occultation observation technique, which can reveal extremely detailed information about the size, shape, atmospheric structure, and existence of rings and satellites of minor planets in the Solar System, is described in detail. A web-based platform called Occultation Portal (OP) has been developed for the analysis, archiving and visualization of the data obtained by this observation technique, and the operation and architecture of this platform are explained in detail. Finally, the observations of (28978) Ixion (2001 KX76), a Trans-Neptune Object on which campaign observations were made on this platform, dated October 13, 2020, and April 28, 2021, were examined in detail for the first time with this study, and its physical parameters were determined and discussed in the thesis. In addition, the stellar diameter of the occulted star was obtained by analyzing the observation data dated October 13, 2020, and our findings were compared with previous studies.}, Address = {Akdeniz University, Institute of Natural and Applied Sciences, Space Science and Technologies Department}, Author = {{Kilic}, Y.}, Date-Added = {2023-03-03 16:44:54 +0000}, Date-Modified = {2023-03-03 16:44:54 +0000}, Keywords = {Asteroids, Solar System, Astronomical image processing, Data analysis, Data archiving system, Minor planets, Stellar occultations, trans-Neptunian object}, Month = {January}, School = {Akdeniz University}, Title = {Investigation of solar system bodies by stellar occultation technique}, Url = {https://tez.yok.gov.tr/UlusalTezMerkezi/TezGoster?key=kIrIdtdJ31bRgjb6fHvMUQDUenHnLZY0dD5PDCSDIuS5omcU6HbG5AMOCVYVUyVj}, language = "Turkish" Year = {2023}}
Talks & Lectures
- Y. Kilic, F. Braga-Ribas, and M. Kaplan, “OccultPortal: a web-based platform for data collection and analysis of stellar occultations,” , 2020.
[Bibtex]@talk{esop2020, title = {OccultPortal: a web-based platform for data collection and analysis of stellar occultations}, author = {{Kilic}, Y. and {Braga-Ribas}, F. and {Kaplan}, M.}, event = {39th European Symposium on Occultation Projects (ESOP)}, year = {2020}, institution = {International Occultation Timing Association/European Section (IOTA/ES)}, month = aug, day = 20, note = {Speaker}, language = "English", URL= {https://iota-es.de/esop39/seiten/programm.php}, } - Y. Kilic, O. Okuyan, and I. Khamitov, “Lisansüstü Öğrencileri Yaz Programı (LÜYP),” , 2020.
[Bibtex]@talk{luyp_2020, title = {Lisansüstü Öğrencileri Yaz Programı (LÜYP)}, author = {{Kilic}, Y. and {Okuyan}, O. and {Khamitov}, I.}, event = {Lisansüstü Öğrencileri Yaz Programı (LÜYP)}, year = {2020}, institution = {TÜBİTAK Ulusal Gözlemevi}, month = jul, language = "Turkish", note = {Instructor}, URL= {https://tug.tubitak.gov.tr/tr/faaliyetalanlarimiz/lisansustu-ogrencileri-yaz-programi-luyp}, } - Y. Kilic, I. Khamitov, and O. Okuyan, “Asteroid 2059 (Baboquivari)’nin Fiziksel Parametlerinin TUG Teleskopları ile Araştırılması,” , 2019.
[Bibtex]@talk{astmet2019, title = {Asteroid 2059 (Baboquivari)'nin Fiziksel Parametlerinin TUG Teleskopları ile Araştırılması}, author = {{Kilic}, Y. and {Khamitov}, I. and {Okuyan}, O.}, event = {III. Asteroit Madenciliği ve Meteor Bilimi Çalıştayı}, year = {2019}, institution = {Ege Üniversitesi}, month = dec# "~16,", note = {Invited speaker}, language = Turkish, URL= {http://www.ozanunsalan.com/2019/09/astminmet/}, } - Y. Kilic, “Güneş Sistemi’nden Evrene,” , 2019.
[Bibtex]@talk{antalya_koleji_konyaalti_2019, title = {Güneş Sistemi'nden Evrene}, author = {{Kilic}, Y.}, event = {Antalya}, year = {2019}, institution = {Özel Antalya Koleji - Konyaaltı Kampüsü}, month = oct# "~11,", language = Turkish, note = {Invited speaker}, URL= {http://www.antalyakoleji.k12.tr/duyurular.php?id=4656&cid=2&bid=8}, } - Y. Kilic and M. S. Shemoni, “IRAF ve MYRaf ile Işıkölçüm Analizi,” , 2019.
[Bibtex]@talk{alup_2019, title = {IRAF ve MYRaf ile Işıkölçüm Analizi}, author = {{Kilic}, Y. and {Shemoni}, M.S.}, event = {Atatürk Üniversitesi Lisansüstü Bilgilendirme ve Uygulama Programı 2019}, year = {2019}, institution = {Atatürk University ATASAM}, month = sep# "~26--28,", language = Turkish, note = {Invited speaker}, URL= {http://atasam.atauni.edu.tr/duyurular/alup/2019-2/}, } - Y. Kilic and H. A. Kayihan, “Müfredat Çerçevesinde Astronomi Konulu Söyleşi ve Öğretmen Sorularına Cevaplar,” , 2019.
[Bibtex]@talk{astronomi_semineri_2019, title = {Müfredat Çerçevesinde Astronomi Konulu Söyleşi ve Öğretmen Sorularına Cevaplar}, author = {{Kilic}, Y. and {Kayihan}, H.A.}, event = {Antalya Bilim Söyleşileri}, year = {2019}, institution = {Antalya Büyükşehir Belediyesi}, month = sep# "~16,", note = {Invited speaker}, language = Turkish, } - Y. Kilic, M. Kaplan, and O. Erece, “A-Track: a Tool for Detecting Moving Objects from Astronomical Images,” , 2019.
[Bibtex]@talk{asteroid2019, title = {A-Track: a Tool for Detecting Moving Objects from Astronomical Images}, author = {{Kilic}, Y. and {Kaplan}, M. and {Erece}, O.}, event = {Dynamics and Physics Of Asteroids, TNOs and Natural Satellites in the New Era of GAIA Data}, year = {2019}, institution = {Akdeniz University}, month = sep# "~4--6,", note = {Speaker}, language = English, URL= {https://asteroid2019.space}, } - Y. Kilic, “Robotik T60 Teleskobu ile Asteroit Gözlemi,” , 2019.
[Bibtex]@talk{uggs2019, title = {Robotik T60 Teleskobu ile Asteroit Gözlemi}, author = {{Kilic}, Y.}, event = {22. Ulusal Gökyüzü Gözlem Şenliği}, year = {2019}, institution = {TÜBİTAK Ulusal Gözlemevi}, month = aug# "~2--3,", note = {Speaker}, language = Turkish, URL= {http://senlik.tug.tubitak.gov.tr/wp-content/uploads/2019/07/SenlikProgram.pdf}, } - Y. Kilic, “Temel Astronomi,” , 2016.
[Bibtex]@talk{uggs2016, title = {Temel Astronomi}, author = {{Kilic}, Y.}, event = {18. Ulusal Gökyüzü Gözlem Şenliği}, year = {2016}, institution = {TÜBİTAK Ulusal Gözlemevi}, month = jul# "~29,", note = {Invited speaker}, language = Turkish, URL= {http://senlik.tug.tubitak.gov.tr/wp-content/uploads/2015/03/Senlik_programı.pdf}, } - Y. Kilic, “Eğitim-Öğretim’de Astronomi Topluluklarının Önemi ve Gerekliliği,” , 2015.
[Bibtex]@talk{okulgozlemevleri2015 , title = {Eğitim-Öğretim’de Astronomi Topluluklarının Önemi ve Gerekliliği}, author = {{Kilic}, Y.}, event = {Okul Gözlemevileri Sempozyumu}, year = {2015}, institution = {T.C. Milli Eğitim Bakanlığı - TÜBİTAK Ulusal Gözlemevi}, month = nov# "~13--15,", note = {Invited speaker}, language = Turkish, URL= {https://turgutlu.meb.gov.tr/www/okul-gozlemevleri-sempozyumu/icerik/3334}, }