CzeV - The Czech Variable Star Catalogue

0478757 - FZÚ 2020 RIV CZ eng J - Journal Article
Skarka, M. - Mašek, Martin - Brát, L. - Cagaš, P.A. - Juryšek, J. - Hoňková, K. - Zejda, M. - Šmelcer, L. - Jelínek, Martin - Lomoz, F. - Tylšar, M. - Trnka, J. - Pejcha, O. - Pintr, P. - Lehký, M. - Janík, J. - Červinka, L. - Tylšar, M. - Přibík, V. - Motl, D. - Walter, F. - Zasche, P. - Koss, K. - Hájek, P. - Bílek, F. - Liška, J. - Kučáková, H. - Bodnár, F. - Beránek, J. - Šafář, J. - Moudrá, M. - Oršulák, M. - Pintr, M. - Sobotka, P. - Dřevěný, R. - Juráňová, A. - Polák, J. - Polster, J. - Onderková, K. - Smolka, M. - Auer, R.F. - Kocián, R. - Hladík, B. - Cagaš, P. - Greš, A. - Müller, D. - Čapková, H. - Kyselý, Jan - Hornoch, Kamil - Truparová, S. - Timko, L. - Broz, M. - Bílek, Michal - Šebela, P. - Hanžl, D. - Žampachová, E. - Secká, J. - Pravec, Petr - Mrňák, P. - Svoboda, P. - Ehrenberger, R. - Novotný, F. - Poddaný, S. - Prudil, Z. - Kuchťák, B. - Štegner, D.
CzeV - The Czech Variable Star Catalogue.
Open European Journal on Variable stars. Roč. 185, Sep (2017), s. 1-42. ISSN 1801-5964
R&D Projects: GA MŠMT LM2015038; GA MŠMT LG15014; GA MŠMT LM2015046; GA MŠMT LTT17006; GA MŠMT EF16_013/0001402; GA MŠMT EF16_013/0001403
EU Projects: European Commission(XE) 283783 - GLORIA
Grant - others:OP VVV - AUGER-CZ(XE) CZ.02.1.01/0.0/0.0/16_013/0001402; OP VVV - CTAO-CZ(XE) CZ.02.1.01/0.0/0.0/16_013/0001403
Institutional support: RVO:68378271 ; RVO:67985815 ; RVO:68378289
Keywords : variable stars * eclipsing binaries
OECD category: Astronomy (including astrophysics,space science)
Method of publishing: Open access

We present the first release of the Czech Variable star catalogue that currently contains 1228 stars whose variability was discovered by 60 Czech observers. The catalogue contains confirmed variable stars of various types, but also candidates. We give precise coordinates, cross identification with other catalogues, information about constellation, variability type, brightness, light elements, name of the discoverer and year of discovery. In eighty-eight percent of stars the variability type is estimated, for more than 60 % of the stars the light ephemerides are given.
Permanent Link: http://hdl.handle.net/11104/0274845