Minute-Cadence Observations of the LAMOST Fields with the TMTS: II. Catalogues of Short-Period Variable Stars from the First Two-Year Surveys
Over the past few years, wide-field time-domain surveys like ZTF and OGLE have led to discoveries of various types of interesting short-period stellar variables, such as ultracompact eclipsing binary white dwarfs, rapidly rotating magnetised white dwarfs (WDs), transitional cataclysmic variables bet...
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| creator | Lin, Jie Wang, Xiaofeng Mo, Jun Gaobo Xi Filippenko, Alexei V Shengyu Yan Brink, Thomas G Yang, Yi Wu, Chengyuan Németh, Péter Li, Gaici Guo, Fangzhou Guo, Jincheng Cai, Yongzhi Xiong, Heran Zheng, WeiKang Liu, Qichun Zhang, Jicheng Jiang, Xiaojun Chen, Liyang Xia, Qiqi Peng, Haowei Chen, Zhihao Li, Wenxiong Lin, Weili Xiang, Danfeng Ma, Xiaoran Liu, Jialian |
| description | Over the past few years, wide-field time-domain surveys like ZTF and OGLE have led to discoveries of various types of interesting short-period stellar variables, such as ultracompact eclipsing binary white dwarfs, rapidly rotating magnetised white dwarfs (WDs), transitional cataclysmic variables between hydrogen-rich and helium accretion, and blue large-amplitude pulsators (BLAPs), which greatly enrich our understandings of stellar physics under some extreme conditions. In this paper, we report the first-two-year discoveries of short-period variables (i.e., P |
| doi_str_mv | 10.48550/arxiv.2303.18050 |
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Catalogues of Short-Period Variable Stars from the First Two-Year Surveys</title><source>Freely Accessible Journals</source><source>arXiv.org</source><creator>Lin, Jie ; Wang, Xiaofeng ; Mo, Jun ; Gaobo Xi ; Filippenko, Alexei V ; Shengyu Yan ; Brink, Thomas G ; Yang, Yi ; Wu, Chengyuan ; Németh, Péter ; Li, Gaici ; Guo, Fangzhou ; Guo, Jincheng ; Cai, Yongzhi ; Xiong, Heran ; Zheng, WeiKang ; Liu, Qichun ; Zhang, Jicheng ; Jiang, Xiaojun ; Chen, Liyang ; Xia, Qiqi ; Peng, Haowei ; Chen, Zhihao ; Li, Wenxiong ; Lin, Weili ; Xiang, Danfeng ; Ma, Xiaoran ; Liu, Jialian</creator><creatorcontrib>Lin, Jie ; Wang, Xiaofeng ; Mo, Jun ; Gaobo Xi ; Filippenko, Alexei V ; Shengyu Yan ; Brink, Thomas G ; Yang, Yi ; Wu, Chengyuan ; Németh, Péter ; Li, Gaici ; Guo, Fangzhou ; Guo, Jincheng ; Cai, Yongzhi ; Xiong, Heran ; Zheng, WeiKang ; Liu, Qichun ; Zhang, Jicheng ; Jiang, Xiaojun ; Chen, Liyang ; Xia, Qiqi ; Peng, Haowei ; Chen, Zhihao ; Li, Wenxiong ; Lin, Weili ; Xiang, Danfeng ; Ma, Xiaoran ; Liu, Jialian</creatorcontrib><description>Over the past few years, wide-field time-domain surveys like ZTF and OGLE have led to discoveries of various types of interesting short-period stellar variables, such as ultracompact eclipsing binary white dwarfs, rapidly rotating magnetised white dwarfs (WDs), transitional cataclysmic variables between hydrogen-rich and helium accretion, and blue large-amplitude pulsators (BLAPs), which greatly enrich our understandings of stellar physics under some extreme conditions. In this paper, we report the first-two-year discoveries of short-period variables (i.e., P<2 hr) by the Tsinghua University-Ma Huateng Telescopes for Survey (TMTS). TMTS is a multi-tube telescope system with a field of view up to 18 deg^2, which started to monitor the LAMOST sky areas since 2020 and generated uninterrupted minute-cadence light curves for about ten million sources within 2 years. Adopting the Lomb-Scargle periodogram with period-dependent thresholds for the maximum powers, we identify over 1 100 sources that exhibit a variation period shorter than 2 hr. Compiling the light curves with the Gaia magnitudes and colours, LAMOST spectral parameters, VSX classifications, and archived observations from other prevailing time-domain survey missions, we identified 1 076 as delta Scuti stars, which allows us study their populations and physical properties in the short-period regime. The other 31 sources include BLAPs, subdwarf B variables (sdBVs), pulsating WDs, ultracompact/short-period eclipsing/ellipsoidal binaries, cataclysmic variables below the period gap, etc., which are highly interesting and worthy of follow-up investigations.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2303.18050</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Cataclysmic variables ; Deposition ; Eclipsing binary stars ; Light curve ; Physical properties ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics ; Sky surveys (astronomy) ; Stellar physics ; Telescopes ; Time domain analysis ; Variable stars ; Variables ; White dwarf stars</subject><ispartof>arXiv.org, 2023-04</ispartof><rights>2023. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,782,786,887,27932</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.2303.18050$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1093/mnras/stad994$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Lin, Jie</creatorcontrib><creatorcontrib>Wang, Xiaofeng</creatorcontrib><creatorcontrib>Mo, Jun</creatorcontrib><creatorcontrib>Gaobo Xi</creatorcontrib><creatorcontrib>Filippenko, Alexei V</creatorcontrib><creatorcontrib>Shengyu Yan</creatorcontrib><creatorcontrib>Brink, Thomas G</creatorcontrib><creatorcontrib>Yang, Yi</creatorcontrib><creatorcontrib>Wu, Chengyuan</creatorcontrib><creatorcontrib>Németh, Péter</creatorcontrib><creatorcontrib>Li, Gaici</creatorcontrib><creatorcontrib>Guo, Fangzhou</creatorcontrib><creatorcontrib>Guo, Jincheng</creatorcontrib><creatorcontrib>Cai, Yongzhi</creatorcontrib><creatorcontrib>Xiong, Heran</creatorcontrib><creatorcontrib>Zheng, WeiKang</creatorcontrib><creatorcontrib>Liu, Qichun</creatorcontrib><creatorcontrib>Zhang, Jicheng</creatorcontrib><creatorcontrib>Jiang, Xiaojun</creatorcontrib><creatorcontrib>Chen, Liyang</creatorcontrib><creatorcontrib>Xia, Qiqi</creatorcontrib><creatorcontrib>Peng, Haowei</creatorcontrib><creatorcontrib>Chen, Zhihao</creatorcontrib><creatorcontrib>Li, Wenxiong</creatorcontrib><creatorcontrib>Lin, Weili</creatorcontrib><creatorcontrib>Xiang, Danfeng</creatorcontrib><creatorcontrib>Ma, Xiaoran</creatorcontrib><creatorcontrib>Liu, Jialian</creatorcontrib><title>Minute-Cadence Observations of the LAMOST Fields with the TMTS: II. Catalogues of Short-Period Variable Stars from the First Two-Year Surveys</title><title>arXiv.org</title><description>Over the past few years, wide-field time-domain surveys like ZTF and OGLE have led to discoveries of various types of interesting short-period stellar variables, such as ultracompact eclipsing binary white dwarfs, rapidly rotating magnetised white dwarfs (WDs), transitional cataclysmic variables between hydrogen-rich and helium accretion, and blue large-amplitude pulsators (BLAPs), which greatly enrich our understandings of stellar physics under some extreme conditions. In this paper, we report the first-two-year discoveries of short-period variables (i.e., P<2 hr) by the Tsinghua University-Ma Huateng Telescopes for Survey (TMTS). TMTS is a multi-tube telescope system with a field of view up to 18 deg^2, which started to monitor the LAMOST sky areas since 2020 and generated uninterrupted minute-cadence light curves for about ten million sources within 2 years. Adopting the Lomb-Scargle periodogram with period-dependent thresholds for the maximum powers, we identify over 1 100 sources that exhibit a variation period shorter than 2 hr. Compiling the light curves with the Gaia magnitudes and colours, LAMOST spectral parameters, VSX classifications, and archived observations from other prevailing time-domain survey missions, we identified 1 076 as delta Scuti stars, which allows us study their populations and physical properties in the short-period regime. The other 31 sources include BLAPs, subdwarf B variables (sdBVs), pulsating WDs, ultracompact/short-period eclipsing/ellipsoidal binaries, cataclysmic variables below the period gap, etc., which are highly interesting and worthy of follow-up investigations.</description><subject>Cataclysmic variables</subject><subject>Deposition</subject><subject>Eclipsing binary stars</subject><subject>Light curve</subject><subject>Physical properties</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><subject>Sky surveys (astronomy)</subject><subject>Stellar physics</subject><subject>Telescopes</subject><subject>Time domain analysis</subject><subject>Variable stars</subject><subject>Variables</subject><subject>White dwarf stars</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotkF9LwzAUxYMgOOY-gE8GfO7Mn2ZNfRvF6WBjQovgU0mbxGV0zUzSzX0Iv7O18-lyL-dczvkBcIfRNOaMoUfhvs1xSiiiU8wRQ1dgRCjFEY8JuQET73cIITJLCGN0BH7Wpu2CijIhVVsruKm8ckcRjG09tBqGrYKr-XqTF3BhVCM9PJmwHc7Fusif4HI5hZkIorGfnRos-da6EL0pZ6yE78IZUTUK5kE4D7Wz-8G8MM4HWJxs9KGEg3nnjursb8G1Fo1Xk_85BsXiucheo9XmZZnNV5FIGYoSTVHKZppKLLlMWUzqlEvOcaJ1v9WCJjiJeVojhLGmrGaSUVqlSlRME6LoGNxf3g6syoMze-HO5R-zcmDWKx4uioOzX32vUO5s59o-U0mSPkMSz2JEfwHMEG41</recordid><startdate>20230403</startdate><enddate>20230403</enddate><creator>Lin, Jie</creator><creator>Wang, Xiaofeng</creator><creator>Mo, Jun</creator><creator>Gaobo Xi</creator><creator>Filippenko, Alexei V</creator><creator>Shengyu Yan</creator><creator>Brink, Thomas G</creator><creator>Yang, Yi</creator><creator>Wu, Chengyuan</creator><creator>Németh, Péter</creator><creator>Li, Gaici</creator><creator>Guo, Fangzhou</creator><creator>Guo, Jincheng</creator><creator>Cai, Yongzhi</creator><creator>Xiong, Heran</creator><creator>Zheng, WeiKang</creator><creator>Liu, Qichun</creator><creator>Zhang, Jicheng</creator><creator>Jiang, Xiaojun</creator><creator>Chen, Liyang</creator><creator>Xia, Qiqi</creator><creator>Peng, Haowei</creator><creator>Chen, Zhihao</creator><creator>Li, Wenxiong</creator><creator>Lin, Weili</creator><creator>Xiang, Danfeng</creator><creator>Ma, Xiaoran</creator><creator>Liu, Jialian</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20230403</creationdate><title>Minute-Cadence Observations of the LAMOST Fields with the TMTS: II. 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Catalogues of Short-Period Variable Stars from the First Two-Year Surveys</atitle><jtitle>arXiv.org</jtitle><date>2023-04-03</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>Over the past few years, wide-field time-domain surveys like ZTF and OGLE have led to discoveries of various types of interesting short-period stellar variables, such as ultracompact eclipsing binary white dwarfs, rapidly rotating magnetised white dwarfs (WDs), transitional cataclysmic variables between hydrogen-rich and helium accretion, and blue large-amplitude pulsators (BLAPs), which greatly enrich our understandings of stellar physics under some extreme conditions. In this paper, we report the first-two-year discoveries of short-period variables (i.e., P<2 hr) by the Tsinghua University-Ma Huateng Telescopes for Survey (TMTS). TMTS is a multi-tube telescope system with a field of view up to 18 deg^2, which started to monitor the LAMOST sky areas since 2020 and generated uninterrupted minute-cadence light curves for about ten million sources within 2 years. Adopting the Lomb-Scargle periodogram with period-dependent thresholds for the maximum powers, we identify over 1 100 sources that exhibit a variation period shorter than 2 hr. Compiling the light curves with the Gaia magnitudes and colours, LAMOST spectral parameters, VSX classifications, and archived observations from other prevailing time-domain survey missions, we identified 1 076 as delta Scuti stars, which allows us study their populations and physical properties in the short-period regime. The other 31 sources include BLAPs, subdwarf B variables (sdBVs), pulsating WDs, ultracompact/short-period eclipsing/ellipsoidal binaries, cataclysmic variables below the period gap, etc., which are highly interesting and worthy of follow-up investigations.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2303.18050</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Cataclysmic variables Deposition Eclipsing binary stars Light curve Physical properties Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics Sky surveys (astronomy) Stellar physics Telescopes Time domain analysis Variable stars Variables White dwarf stars |
| title | Minute-Cadence Observations of the LAMOST Fields with the TMTS: II. Catalogues of Short-Period Variable Stars from the First Two-Year Surveys |
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