SHIPsDataAssignments

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We need to gather data from wavelengths other than Herschel for the following reasons:

  1. To prepare the SED of the proto-stars
  2. To prepare a list of all known pre-main sequence stars (all classes).
  3. To

Near infrared photometry

  • Source: 2MASS survey
  • Source: J, H, or K- band surveys (Megeath? Who else)


Spitzer IRAC photometry

24um Photometry

  • Source: Spitzer/MIPS camera

=

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