V* ER Cet , the SIMBAD biblio

V* ER Cet , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:05:57

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1998Ap.....41..356G viz 169 6 First Byurakan spectral sky survey. Stars of late spectral types. -11 deg < delta < -7 deg belt. GIGOYAN K.S., HAMBARYAN V.V. and AZZOPARDI M.
2001IBVS.5135....1K 1414 17 The 76th name-list of variable stars. KAZAROVETS E.V., SAMUS N.N. and DURLEVICH O.V.
2002AcA....52..397P viz 14       D               2893 1175 The All Sky Automated Survey. Catalog of variable stars. I. 0h -6h quarter of the Southern hemisphere. POJMANSKI G.
2004AJ....128.2965W viz 15       D               1 8686 106 Identifying red variables in the Northern Sky Variability Survey. WOZNIAK S.J., WILLIAMS P.R., VESTRAND W.T., et al.
2012MNRAS.419.3346G viz 15       D               1 1046 14 Revised and updated catalogue of the first byurakan survey of late-type stars. GIGOYAN K.S. and MICKAELIAN A.M.
2016ApJS..227....6V viz 16       D               1 2892 2 Determination of pulsation periods and other parameters of 2875 stars classified as Mira in the All Sky Automated Survey (ASAS). VOGT N., CONTRERAS-QUIJADA A., FUENTES-MORALES I., et al.
2018AJ....156..241H viz 16       D               1 311106 199 A first catalog of variable stars measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS). HEINZE A.N., TONRY J.L., DENNEAU L., et al.
2019MNRAS.486.1907J viz 16       D               1 8966 183 The ASAS-SN catalogue of variable stars - II. Uniform classification of 412 000 known variables. JAYASINGHE T., STANEK K.Z., KOCHANEK C.S., et al.
2023A&A...674A..15L viz 17       D               1 1720610 15 Gaia Data Release 3 The second Gaia catalogue of long-period variable candidates. LEBZELTER T., MOWLAVI N., LECOEUR-TAIBI I., et al.
2025A&A...700A.187U viz 19       D               1 3121 ~ A population analysis of Galactic Miras with light-curve asymmetries. UTTENTHALER S. and MERCHAN-BENITEZ P.

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