VizieR

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Catalog

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21 catalogs found

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III/39A
(c)
1k
UV Bright Star Spectrophotometric Catalog (Jamar+, 1976)
spectrum/SED
img(gal)
    
III/53
(c)
1k
Stars classified from S2/68 UV line features (Cucchiaro+ 1979)
img(gal)
    
III/115
(c)
1k
IUE Atlas of O-Type Stellar Spectra (Walborn+ 1985)
img(gal)
    
J/ApJ/817/1
(c)
557
Palomar/MSU and SDSS-DR7 M dwarfs with GALEX obs. (Jones+, 2016)
img(gal)
    
J/ApJ/872/199
(c)
894
Candidate spectrophotometric standard DA WDs (Calamida+, 2019)
img(gal)
    
J/ApJ/931/157
(c)
8
UV-to-NIR spectra of 8 Wolf-Rayet stars in LMC (Aadland+, 2022)
spectrum
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J/ApJS/119/83
(c)
1k
IUE sample of binaries with hot component (Parsons+, 1998)
img(gal)
    
J/ApJS/187/149
(c)
544
StarCAT: STIS UV echelle spectra of stars (Ayres, 2010)
spectrum/jpeg
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J/ApJS/234/31
(c)
2k
Carbon stars from LAMOST using machine learning (Li+, 2018)
img(gal)
    
J/ApJS/259/12
(c)
280
Dust extinction law in nearby galaxies. I. M31 (Wang+, 2022)
img(gal)
    
J/ApJS/260/41
(c)
252
Dust extinction law in nearby galaxies. II. M33 (Wang+, 2022)
img(gal)
    
J/ApJS/266/6
(c)
1k
In the Trenches of the solar-stellar connection. VII. (Ayres, 2023)
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J/AJ/143/28
(c)
1k
Analysis of B6-A9 stars from INES UV spectra (Freire+, 2012)
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J/AJ/148/64
(c)
242
HAZMAT. I. FUV and NUV emission in early M stars (Shkolnik+, 2014)
img(gal)
    
J/AJ/154/67
(c)
376
HAZMAT. II. Low-mass stars with GALEX UV observations (Miles+, 2017)
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J/AJ/154/118
(c)
1k
WD+dMs from the SUPERBLINK proper motion survey (Skinner+, 2017)
img(gal)
    
J/AJ/158/192
(c)
283
He II emission from Wolf-Rayet stars in MW & LMC (Leitherer+, 2019)
img(gal)
    
J/PASP/121/634
(c)
332
FUSE observations in Magellanic Clouds (Blair+, 2009)
img(gal)
    
J/MNRAS/493/4570
(c)
456
Coronal mass ejections on solar-like stars (Leitzinger+, 2020)
img(gal)
    
J/MNRAS/509/2674
(c)
8k
White dwarfs in LAMOST DR5 (Guo+, 2022)
img(gal)
    
J/MNRAS/516/4164
(c)
192
+150 OB stars in Sextans A (Lorenzo+, 2022)
img(gal)

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       (c)  indicates tables which contain celestial coordinates 
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