Abstract
2017 yılında İstanbul Üniversitesi Bilimsel Araştırma Projeleri Birimi tarafından desteklenen bir Güdümlü Proje ile eksiklikleri giderilen, başta lisans öğrencileri tarafından eğitim ve araştırma amaçları ile kullanılmaya başlanmıştır. Kasım 2017’den beri 100’den fazla gecelik gözlem verisi elde edilmiştir. Bu gözlemlerde 40 farklı cisim gözlenmiştir. Gözlenen cisimlerin %68’i değişen yıldız olmakla birlikte, öte gezegen geçişleri, asteroid ve kuyrukluyıldızlar ile AGN ve benzeri kaynaklar da gözlenmiştir. Bu posterde şimdiye kadar yapılan gözlemlere ait temel istatistikler, elde edilen ilk sonuçlar ve teleskobun performansı ışık eğrileri ile birlikte sunulacaktır.
Keywords
telescopes stars: variables techniques: photometric stars: individual: LR Cam stars: individual: HW Vir
References
- Aliş S., ve diğ., 2020, Turkish Journal of Astronomy and Astrophysics, 1, 759
- Brown-Sevilla S. B., ve diğ., 2021, MNRAS, 506, 2122
- Hroch F., 2014, Munipack: General astronomical image processing software (ascl:1402.006)
- Kwee K. K., van Woerden H., 1956, Bull. Astron. Inst. Netherlands, 12, 327, ADS
- Paunzen E., Vanmunster T., 2016, Astronomische Nachrichten, 337, 239
- Sağlam M. T., ve diğ., 2022, Turkish Journal of Astronomy and Astrophysics, 3, 8
- Stetson P. B., 1987, PASP, 99, 191
- Yang Y.-G., Dai H.-F., 2010, PASJ, 62, 1045
Abstract
The IST40 telescope was started to be used for educational and research purposes, especially by undergraduate students, whose complementary parts are provided by a Guided Project supported by Istanbul University Scientific Research Projects Unit in 2017. More than 100 nights of observational data have been obtained since November 2017. In these observations, 70 different objects were observed. While 78% of the observed objects are variable stars, exoplanet transits, asteroids and comets, AGN and similar sources have also been observed. In this study, the basic statistics of observations made so far, the first results and the performance of the telescope will be presented along with the light curves.
Keywords
telescopes stars: variables techniques: photometric stars: individual: LR Cam stars: individual: HW Vir
References
- Aliş S., ve diğ., 2020, Turkish Journal of Astronomy and Astrophysics, 1, 759
- Brown-Sevilla S. B., ve diğ., 2021, MNRAS, 506, 2122
- Hroch F., 2014, Munipack: General astronomical image processing software (ascl:1402.006)
- Kwee K. K., van Woerden H., 1956, Bull. Astron. Inst. Netherlands, 12, 327, ADS
- Paunzen E., Vanmunster T., 2016, Astronomische Nachrichten, 337, 239
- Sağlam M. T., ve diğ., 2022, Turkish Journal of Astronomy and Astrophysics, 3, 8
- Stetson P. B., 1987, PASP, 99, 191
- Yang Y.-G., Dai H.-F., 2010, PASJ, 62, 1045
Details
| Primary Language | Turkish |
|---|---|
| Subjects | Astronomical Sciences (Other) |
| Journal Section | Conference Paper |
| Authors | |
| Early Pub Date | December 18, 2023 |
| Publication Date | December 31, 2023 |
| Submission Date | November 13, 2022 |
| Acceptance Date | December 30, 2022 |
| Published in Issue | Year 2023 Volume: 4 Issue: 3 - Special Issue: Proceedings of the 22nd National Astronomy Congress |
TJAA is a publication of Turkish Astronomical Society (TAD).