VizieR

Distance ρ
Position angle θ
Distance (x,y)
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J2000
B1950
Ecl. J2000

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If the access to catalogues with VizieR was helpful for your research work,the following acknowledgment would be appreciated: This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI: 10.26093/cds/vizier). The original description of the VizieR service was published in A&AS 143, 23

	J/A+A/693/A268	-1		Hot sub-luminous and binaries variability (Ranaivomanana+, 2025) ReadMe+ftp 2025A&A...693A.268R Similar Catalogs
	J/A+A/693/A268/tablea4		^(c)Variability of 63 confirmed hot subdwarfs identified from Gaia and TESS (63 rows)
	J/A+A/693/A268/tablea5		^(c)Variability of 78 candidate hot subdwarfs identified from Gaia and TESS (78 rows)
	J/A+A/693/A268/tablea6		^(c)New variables (134) identified from candidate hot subdwarfs with Gaia lightcurves alone (134 rows)
	J/A+A/693/A268/tablea7		^(c)New variables (15) identified from known hot subdwarfs with Gaia lightcurves alone (15 rows)
	J/A+A/693/A268/tablea8		^(c)List of 140 known CVs from Cluster 2 (140 rows)
	J/A+A/693/A268/tablea9		^(c)List of 152 candidate CVs from Cluster 2 identified in this work (152 rows)
	J/MNRAS/489/1556	-1		K2 observations of binaries PHL 457 and EQ Psc (Baran+, 2019) ReadMe+ftp 2019MNRAS.489.1556B Similar Catalogs timeSerie
	J/MNRAS/489/1556/table1		The ALFOSC RV data of PHL 457 (12 rows)
	J/MNRAS/489/1556/table2		The RV data of EQ Psc (39 rows)
	J/MNRAS/489/1556/table3		^(c)Results of a circular orbital fit after folding the RVs of PHL 457 to orbital phase[timeSerie] (1 rows)
	J/MNRAS/489/1556/table4		The results of the SED fit for PHL 457, based on a Gaia distance of 577±21pc and extinction E(B-V)=0.023^+0.016_–0.023 (2 rows)
	J/MNRAS/489/1556/table5		Frequency list of PHL 457 obtained with pre-whitening (60 rows)
	J/MNRAS/489/1556/table6		^(c)Results of a circular orbital fit to the RVs of EQ PSc[timeSerie] (1 rows)
	J/MNRAS/489/1556/table7		Results of the SED fit for EQ Psc based on a Gaia distance 489±25pc and extinction E(B-V)=0.034⁺⁰_–0.031 (2 rows)
	J/MNRAS/489/1556/table8		Frequency list of EQ Psc obtained with pre-whitening (104 rows)
	J/MNRAS/489/1556/table9		^(c)sdB stars with orbital and rotation periods estimated (17 rows)
	J/MNRAS/494/1448	-1		Wide astrometric companions with Gaia DR2 (Igoshev+, 2020) ReadMe+ftp 2020MNRAS.494.1448I Similar Catalogs
	J/MNRAS/494/1448/table2		^(c)Resolved binaries found in the MSWD sample (21 rows)
	J/MNRAS/494/1448/table3		^(c)Wide binaries found in the MSWD sample (42 rows)
	J/MNRAS/494/1448/table4		^(c)The identified sdB systems with wide companions (64 rows)
	J/MNRAS/494/1448/table5		^(c)Wide binaries found in the CVs sample (14 rows)
	J/MNRAS/498/2833	-1		Algol eclipsing binaries in the Catalina Survey (Carmo+, 2020) ReadMe+ftp 2020MNRAS.498.2833C Similar Catalogs
	J/MNRAS/498/2833/table2		Absolute parameters of the stellar components of the low-mass binary system candidates (8 rows)
	J/MNRAS/498/2833/tablea1		^(c)Parameters for the iEA stars identified in this work (87 rows)
	J/MNRAS/498/2833/tableb1		Parameters obtained from the model fits to the light curves (8 rows)
	J/MNRAS/498/2833/tableb2		Parameters obtained from the redone model fits in order to improve parameters (8 rows)
ALL
			^(c) indicates tables which contain celestial coordinates

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