• LambdaOri_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • LambdaOri_CO_10deg.fits.gz image, CO map
  • 25Ori_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • 25Ori_CO_10deg.fits.gz image, CO map
  • BetaPic_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • BetaPic_CO_10deg.fits.gz image, CO map
  • ChaII_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • ChaII_CO_10deg.fits.gz image, CO map
  • EtaChaA_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • EtaChaA_CO_10deg.fits.gz image, CO map
  • IC2391_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • IC2391_CO_10deg.fits.gz image, CO map
  • IC2602_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • IC2602_CO_10deg.fits.gz image, CO map
  • IC348_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • IC348_CO_10deg.fits.gz image, CO map
  • LupusIII_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • LupusIII_CO_10deg.fits.gz image, CO map
  • NGC2362_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • NGC2362_CO_10deg.fits.gz image, CO map
  • NGC2547_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • NGC2547_CO_10deg.fits.gz image, CO map
  • NGC7160_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • NGC7160_CO_10deg.fits.gz image, CO map
  • RCrA_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • RCrA_CO_10deg.fits.gz image, CO map
  • RhoOph_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • RhoOph_CO_10deg.fits.gz image, CO map
  • Serpens_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • Serpens_CO_10deg.fits.gz image, CO map
  • SigmaOri_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • SigmaOri_CO_10deg.fits.gz image, CO map
  • Taurus_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • Taurus_CO_10deg.fits.gz image, CO map
  • TWHya_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • TWHya_CO_10deg.fits.gz image, CO map
  • Tr37_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • Tr37_CO_10deg.fits.gz image, CO map
  • UpSco_IRAS100_10deg.fits.gz image, IRAS 100 micron
  • UpSco_CO_10deg.fits.gz image, CO map
    • CO data taken by two nearly-identical 1.2 m telescopes in Cambridge, MA and on Cerro Tololo, Chile combined into a complete survey of the Milky Way with CO integrated over all velocities.