VizieR

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

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IAU/CDS nomenclature

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/ApJS/266/11	5325		Stellar sp. libraries in Opt-NIR. I. UVES-POP (Borisov+, 2023) ReadMe+ftp 2023ApJS..266...11B Similar Catalogs
	J/ApJS/266/11/table6		^(c)Spectrum fitting results (406 rows)
	J/A+A/462/683	5455		Velocities in SMC field of NGC 330 (Martayan+, 2007) ReadMe+ftp 2007A&A...462..683M Similar Catalogs
	J/A+A/462/683/stars		^(c)Apparent fundamental parameters for stars in the Small Magellanic Cloud (tables 1 and 3 of the paper) (Note) (332 rows)
	J/AJ/142/146	5688		Radial Velocities of Galactic O-type stars I. (Williams+, 2011) ReadMe+ftp 2011AJ....142..146W Similar Catalogs timeSerie
	J/AJ/142/146/table2		^(c)Individual stellar parameters (18 rows)
	J/AJ/142/146/table1		Radial velocity measurements (233 rows)
	J/MNRAS/443/2815	7038		Cerro Armazones spectroscopy of F dwarfs (Pribulla+, 2014) ReadMe+ftp 2014MNRAS.443.2815P Similar Catalogs
	J/MNRAS/443/2815/table3		^(c)RV variations and suitability of the targets for the exoplanet detection (non single-lined stars added at CDS) (187 rows)
	J/MNRAS/443/2815/table1		Journal of the spectroscopic observations and results of the spectroscopic analysis for individual spectra (409 rows)
	J/MNRAS/488/1090	4404		Unclassified B[e] stars in the MW, SMC and LMC (Condori+, 2019) ReadMe+ftp 2019MNRAS.488.1090C Similar Catalogs
	J/MNRAS/488/1090/table1		^(c)Our sample of unclassified B[e] stars and candidates observed with FEROS (30 rows)
	J/MNRAS/488/1090/table2		^(c)Photometric data of our sample collected from the literature (27 rows)
	J/MNRAS/488/1090/table3		^(c)The radial velocity of stars from our sample that do not present sensible spectral variability or for which we have just one spectrum (14 rows)
	J/MNRAS/488/1090/table4		^(c)Radial velocities, derived from permitted absorption and forbidden emission lines, for the objects with strong variability (13 rows)
	J/MNRAS/488/1090/table5a		^(c)Spectral type, luminosity class, intrinsic color index, and effective temperature for some stars of our sample, obtained using method 1 (9 rows)
	J/MNRAS/488/1090/table5b		^(c)Spectral type, intrinsic color index, and effective temperature for some stars of our sample, obtained using method 2 (7 rows)
	J/MNRAS/488/1090/table5c		^(c)Effective temperature for some stars of our sample, obtained using method 3 (3 rows)
	J/MNRAS/488/1090/table6		^(c)Interstellar, circumstellar, and total color excess, E(B-V), and visual interstellar extinction, A_V, for the objects of our sample (12 rows)
	J/MNRAS/488/1090/table7		^(c)Velocities needed for fitting the line profiles for the stars with both [OI] and [CaII] forbidden lines (5 rows)
	J/MNRAS/488/1090/table8		^(c)Velocities needed for fitting the line profiles for the stars with only the [OI] forbidden lines (16 rows)
	J/MNRAS/488/1090/table9		^(c)Physical parameters of the stars of our sample (11 rows)
ALL
			^(c) indicates tables which contain celestial coordinates

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