247 datasets found

Tags: Infrared

  • IR spectroscopy of comet Halley

    Measurements of comet Halley in the spectral channel of IKS on board the Vega-1 spacecraft. Data are retrieved from the PDS Small Bodies Node archive (2011 reformatted version)...
  • WISE All-Sky 4-band Single-Exposure Images

    NASA's Wide-field Infrared Survey Explorer (WISE) mapped the sky at 3.4, 4.6, 12, and 22 μm (W1, W2, W3, W4) with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in the...
  • WISE All-Sky 4-band Atlas Coadded Images

    NASA's Wide-field Infrared Survey Explorer (WISE) mapped the sky at 3.4, 4.6, 12, and 22 μm (W1, W2, W3, W4) with an angular resolution of 6.1", 6.4", 6.5", & 12.0" in the...
  • Spitzer Level 1 / Basic Calibrated Data

    Level 1 / Basic Calibration Data (BCD) from Spitzer Space Telescope. BCDs are the individual data frames that emerge [calibrated] from the Spitzer pipeline.
  • Spitzer Level 2 / post Basic Calibrated Data

    Level 2 or post Basic Calibrated Data (PBCD) from Spitzer Space Telescope. This products come from combining the individual data frames or BCDs [such as mosaics of individual...
  • VVV DR4 - VISTA Variables in the Via Lactea survey

    The VVV survey will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D...
  • VVV DR4 - VISTA Variables in the Via Lactea survey

    The VVV survey will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D...
  • VVV DR2 - VISTA Variables in the Via Lactea survey

    The VVV survey will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D...
  • VVV DR1 - VISTA Variables in the Via Lactea survey

    The VVV survey will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D...
  • VVV DR1 - VISTA Variables in the Via Lactea survey

    The VVV survey will perform wide FOV multi-epoch observations of the Galaxy's bulge and part of the disk, providing the astronomical public community with a high resolution 3-D...
  • VMC DR4 - VISTA Magellanic System survey

    The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar...
  • VMC DR4 - VISTA Magellanic System survey

    The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar...
  • VMC DR3 - VISTA Magellanic System survey

    The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar...
  • VMC DR3 - VISTA Magellanic System survey

    The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar...
  • VMC DR2 - VISTA Magellanic System survey

    The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar...
  • VMC DR2 - VISTA Magellanic System survey

    The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar...
  • VMC DR1 - VISTA Magellanic System survey

    The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar...
  • VMC DR1 - VISTA Magellanic System survey

    The VMC survey aims to obtain YJKs band photometry across the system down to Ks=20.3 at S/N=10. This sensitivity corresponds to the bottom of the red giant branch field stellar...
  • VIKING - VISTA Kilo-degree Infrared Galaxy survey Data Release 4

    The VIKING survey is the VISTA counterpart to the VST KIDS survey. The KIDS survey will cover 1500 deg^2 in u,g,r,i divided in two stripes (NGP, centred on equator ; SGP,...
  • VIKING - VISTA Kilo-degree Infrared Galaxy survey Data Release 4

    The VIKING survey is the VISTA counterpart to the VST KIDS survey. The KIDS survey will cover 1500 deg^2 in u,g,r,i divided in two stripes (NGP, centred on equator ; SGP,...