COMPLETE Interactive Coverage Tool screenshot

The COordinated Molecular Probe Line Extinction Thermal Emission Survey of Star Forming Regions (COMPLETE) provides a range of data complementary to the Spitzer Legacy Program "From Molecular Cores to Planet Forming Disks" (c2d) for the Perseus, Ophiuchus and Serpens regions. In combination with the Spitzer observations, COMPLETE will allow for detailed analysis and understanding of the physics of star formation on scales from 500 A.U. to 10 pc.

Our Interactive Coverage Tool allows you to see which areas are covered by which data sets in this World Wide Telescope tool.

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21 to 25 of 25 Results
IRAS Based Thermal Emission Maps of Ophiuchus
IRAS Based Thermal Emission Maps of Ophiuchus
Oct 18, 2012
COMPLETE team, 2011, "IRAS Based Thermal Emission Maps of Ophiuchus", https://doi.org/10.7910/DVN/YVP9C3, Harvard Dataverse, V2
IRAS Based Thermal Emission Maps of Serpens
IRAS Based Thermal Emission Maps of Serpens
Oct 18, 2012
COMPLETE team, 2011, "IRAS Based Thermal Emission Maps of Serpens", https://doi.org/10.7910/DVN/AVSN4C, Harvard Dataverse, V2
IRAS Based Thermal Emission Maps of Taurus
IRAS Based Thermal Emission Maps of Taurus
Oct 18, 2012
COMPLETE team, 2011, "IRAS Based Thermal Emission Maps of Taurus", https://doi.org/10.7910/DVN/0U72NO, Harvard Dataverse, V2
IRAS Based Thermal Emission Maps of Perseus
IRAS Based Thermal Emission Maps of Perseus
Oct 18, 2012
COMPLETE team, 2011, "IRAS Based Thermal Emission Maps of Perseus", https://doi.org/10.7910/DVN/NTT77F, Harvard Dataverse, V2
NH3 and CCS at the GBT in Perseus
NH3 and CCS at the GBT in Perseus
Oct 18, 2012
COMPLETE team, 2011, "NH3 and CCS at the GBT in Perseus", https://doi.org/10.7910/DVN/2XLQ51, Harvard Dataverse, V4
Description: NH3 (1-1) and (2-2) and CCS (2-1) spectra towards (sub-)millimeter cores across Perseus. Positions of pointings are shown as red circles overlaid on a Near-Infrared Extinction map made from 2MASS data. Hover over a red circle for the source name and click to retrieve the spectrum at that position. Beam-sizes are enlarged by a factor of...
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