Catalog of Variable Stars in the WD 0009\(\boldsymbol{+}\)501 and GRW \(\boldsymbol{+}\)708247 Fields Based on Photometric Survey Data on Transiting Exoplanets
O. Ya. Yakovlev, A. F. Valeev, G. G. Valyavin, V. N. Aitov, G. Sh. Mitiani, T. A. Fathullin, G. M. Beskin, A. V. Tavrov, O. I. Korablev, G. A. Galazutdinov, V. V. Vlasyuk, E. V. Emelianov, V. V. Sasyuk, A. V. Perkov, S. F. Bondar, T. E. Burlakova, S. N. Fabrika, I. I. Romanyuk
{"title":"Catalog of Variable Stars in the WD 0009\\(\\boldsymbol{+}\\)501 and GRW \\(\\boldsymbol{+}\\)708247 Fields Based on Photometric Survey Data on Transiting Exoplanets","authors":"O. Ya. Yakovlev, A. F. Valeev, G. G. Valyavin, V. N. Aitov, G. Sh. Mitiani, T. A. Fathullin, G. M. Beskin, A. V. Tavrov, O. I. Korablev, G. A. Galazutdinov, V. V. Vlasyuk, E. V. Emelianov, V. V. Sasyuk, A. V. Perkov, S. F. Bondar, T. E. Burlakova, S. N. Fabrika, I. I. Romanyuk","doi":"10.1134/S1990341323600400","DOIUrl":null,"url":null,"abstract":"<p>The light curves for almost 50 thousand stars with magnitudes <span>\\(m\\in[11\\overset{\\textrm{m}}{.}5,19\\overset{\\textrm{m}}{.}5]\\)</span> have been obtained over 2.5 years at SAO RAS in the process of conducting an exoplanet survey in roughly <span>\\(1\\overset{\\circ}{.}5\\)</span>-sized fields around the white dwarfs WD 0009<span>\\(+\\)</span>501 and GRW <span>\\(+\\)</span>708247. In this paper we present a catalog of variable stars that have been found in the considered regions. Periodogram analysis was used as the main variation search method. The catalog includes 150 periodic variable stars: 113 of them have been known previously, and for the remaining 37 variations have been discovered for the first time. These stars were classified according to the nature of the variations into four eclipsing variable and three pulsating types, as well as rotating stars. We present the periods and variation amplitudes in the range of <span>\\(P\\in[0\\overset{\\textrm{d}}{.}036,32\\overset{\\textrm{d}}{.}14]\\)</span> and <span>\\(\\Delta m\\in[0\\overset{\\textrm{m}}{.}0064,1\\overset{\\textrm{m}}{.}45]\\)</span>, determined from the investigated data.</p>","PeriodicalId":478,"journal":{"name":"Astrophysical Bulletin","volume":"79 1","pages":"126 - 136"},"PeriodicalIF":1.3000,"publicationDate":"2024-05-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astrophysical Bulletin","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1134/S1990341323600400","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
The light curves for almost 50 thousand stars with magnitudes \(m\in[11\overset{\textrm{m}}{.}5,19\overset{\textrm{m}}{.}5]\) have been obtained over 2.5 years at SAO RAS in the process of conducting an exoplanet survey in roughly \(1\overset{\circ}{.}5\)-sized fields around the white dwarfs WD 0009\(+\)501 and GRW \(+\)708247. In this paper we present a catalog of variable stars that have been found in the considered regions. Periodogram analysis was used as the main variation search method. The catalog includes 150 periodic variable stars: 113 of them have been known previously, and for the remaining 37 variations have been discovered for the first time. These stars were classified according to the nature of the variations into four eclipsing variable and three pulsating types, as well as rotating stars. We present the periods and variation amplitudes in the range of \(P\in[0\overset{\textrm{d}}{.}036,32\overset{\textrm{d}}{.}14]\) and \(\Delta m\in[0\overset{\textrm{m}}{.}0064,1\overset{\textrm{m}}{.}45]\), determined from the investigated data.
Abstract The light curves for almost 50 thousand stars with magnitudes (m/in[11\verset{textrm{m}}{.}5,19\verset{textrm{m}}{.}5]\) have been obtained over 2.在白矮星 WD 0009\(+\)501 和 GRW\(+\)708247 周围的大约 \(1\verset\{circ}{.}5\)大小的场中进行系外行星巡天的过程中,在 SAO RAS 进行了为期 5 年的观测。在本文中,我们介绍了在所考虑的区域内发现的变星星表。周期图分析被用作主要的变星搜索方法。星表中包括150颗周期变星:其中113颗是以前已知的,其余37颗变星是首次发现的。根据变异的性质,这些恒星被分为四种蚀变型和三种脉动型,以及旋转型恒星。我们给出了根据调查数据确定的周期和变幅范围(P\in[0\verset{textrm{d}}{.}036,32\verset{textrm{d}}{.}14]\)以及(\Delta m\in[0\verset{textrm{m}}{.}0064,1\overset{\textrm{m}}{.}45]\ )。
期刊介绍:
Astrophysical Bulletin is an international peer reviewed journal that publishes the results of original research in various areas of modern astronomy and astrophysics, including observational and theoretical astrophysics, physics of the Sun, radio astronomy, stellar astronomy, extragalactic astronomy, cosmology, and astronomy methods and instrumentation.