96 datasets found

Keywords: Stars

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  • 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...
  • Kepler Input Catalog

    The KIC, or Kepler Input Catalog, is the primary source of information about objects observed as part of the ground-based Kepler Spectral Classification Program (SCP) in...
  • Kepler Objects of Interest (KOI)

    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...
  • Kepler K2 Ecliptic Plane Input Catalog

    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...
  • VHS DR4 - VISTA Hemisphere Survey Data Release 4

    The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The...
  • VHS DR3 - VISTA Hemisphere Survey Data Release 3

    The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The...
  • VHS DR2 - VISTA Hemisphere Survey Data Release 2

    The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The...
  • VHS DR1 - VISTA Hemisphere Survey Data Release 1

    The VHS will image the entire ~20 000 square degrees of the Southern Sky, with the exception of the areas already covered by the VIKING and VVV surveys, in J and Ks. The...
  • Supporting Materials

    This collection contains supporting materials for the article titled "Direct observations of a complex coronal web driving highly structured slow solar wind". The folder...
  • Berkeley Extreme and Far-UV Spectrometer

    The Berkeley Extreme and Far-UV Spectrometer (BEFS), flew on the Orbiting and Retrievable Far and Extreme Ultraviolet Spectrograph (ORFEUS)-SPAS I and II space...
  • Space Telescope Imaging Spectrograph

    The Space Telescope Imaging Spectrograph (STIS) was installed in HST on Feb. 14, 1997, replacing the GHRS spectrograph. STIS provides spectra and images at...
  • Goddard High Resolution Spectrograph

    GHRS was used to make finely detailed spectroscopic observations of ultraviolet sources, but was removed from HST in February 1997.
  • Near Infrared Camera and Multi Object Spectrograph

    The HST Near Infrared Camera and Multi-Object Spectrometer (NICMOS) provides imaging capabilities in broad, medium, and narrow band filters, broad-band imaging...
  • Faint Object Camera

    The Faint Object Camera (FOC) was one of the 4 original axial instruments on the Hubble Space Telescope (HST). FOC is used to make high-resolution observations...
  • Faint Object Spectrograph

    The Faint Object Spectrograph (FOS) was one of the 4 original axial instruments aboard the Hubble Space Telescope (HST). The FOS was designed to make...
  • Advanced Camera for Surveys

    HST Advanced Camera for Surveys (ACS) - Images: CCD images between 3,700 - 11
  • Hubble Space Telescope

    Hubble Space Telescope (HST) is an orbiting astronomical observatory operating from the near-infrared into the ultraviolet. Launched in 1990 and scheduled to...
  • HST Space Telescope Imaging Spectrograph

    MAST-produced spectral container files for STIS spectra. STIS spectra range from 1150 to 10,300 at low to medium spectral resolution, high spatial resolution...
  • Kepler Confirmed Planets

    The list of currently confirmed exoplanets discovered by Kepler (from data compiled by http://nexsci.caltech.edu).
  • Kepler K2 Data Search Catalog

    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...
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