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KRATOS: A large suite of N-body simulations to interpret the stellar kinemati...
The Large and Small Magellanic Cloud (LMC and SMC, respectively) are the brightest satellites of the Milky Way (MW) and, for the previous thousands of million years, they have... -
Digitized Sky Survey
The Online Digitized Sky Surveys (DSS1 & 2) server at the ESO/ST-ECF Archive provides access to the CD-ROM set produced by the Space Telescope Science Institute through its... -
CfA Hectospec Spectra
Optical spectra collected with the multi-fiber Hectospec Spectrograph at the MMT 6.5m telescope -
Hopkins Ultraviolet Telescope
The Hopkins Ultraviolet Telescope (HUT) was a shuttle-borne instrument used to obtain ultraviolet spectra in the far ultraviolet region of the spectrum. It was part of the ASTRO... -
International Ultraviolet Explorer
The International Ultraviolet Explorer (IUE) performed spectrophotometry at high (0.1-0.3 Å) and low (6-7 Å) resolution between 1150 Å and 3200 Å. The data cover a... -
Ultraviolet Imaging Telescope
The Ultraviolet Imaging Telescope UIT was one of three ultraviolet telescopes on the ASTRO-1 mission flown on the space shuttle Columbia during 2-10 December 1990. The same... -
Five Supernova Survey Galaxies
VO-compliant publication of the properties of the 3838 galaxies that were monitored for SNe events, including newly determined morphologies and their DENIS and POSS-II/UKST I,... -
Hubble Space Telescope Heritage Press Release Images
WFPC2 and ACS images used to create the Heritage project color composite press releases. The data has been expertly prepared, significantly beyond the standard pipeline... -
Wide Field Planetary Camera 1
The WF/PC-1 was used from April 1990 to November 1993, to obtain high resolution images of astronomical objects over a relatively wide field of view and a broad... -
Wide Field Planetary Camera 2
The WFPC2 is used to obtain high resolution images of astronomical objects over a relatively wide field of view and a broad range of wavelengths (1150 to 11,000 Å). -
LAMOST DR2 survey spectra
LAMOST DR2 SSAP service -
LAMOST DR3 survey spectra
LAMOST DR3 SSAP service -
LAMOST DR1 survey spectra
LAMOST DR1 SSAP service -
Extreme Ultraviolet Explorer
Launched in June, 1992, The Extreme Ultraviolet Explorer (EUVE) conducted the first extreme ultraviolet (70-760 Angstroms) survey of the sky and subsequently began a Guest... -
Hubble Source Catalog Detailed Search
The Hubble Source Catalog (HSC) is designed to optimize science from the Hubble Space Telescope by combining the tens of thousands of visit-based source lists in the Hubble... -
Hubble Source Catalog Summary Search
The Hubble Source Catalog (HSC) is designed to optimize science from the Hubble Space Telescope by combining the tens of thousands visit-based source lists in the Hubble Legacy... -
Far Ultraviolet Spectroscopic Explorer
The Far Ultraviolet Spectroscopic Explorer (FUSE), launched on June 24, 1999, covers the 905-1187 Å spectral region and will obtain high resolution spectra of hot and cool... -
Kepler Data Search
Launched in 2009, the Kepler Mission is surveying a region of our galaxy to determine what fraction of stars in our galaxy have planets and measure the size distribution of... -
SSA service for RCSED spectrophotometric catalog of nearby galaxies
Observed spectra and their fitted models for galaxies from RCSED catalog (derived from cross-match between SDSS, GALEX, and UKIDSS catalogs) -
TAP service for the Reference Catalog of Galaxy SEDs (RCSED)
Spectra and photometry of galaxies derived from cross-match between SDSS, GALEX, and UKIDSS catalogs
