Difference between revisions of "SHIPsDataAssignments"

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We need to gather data from wavelengths other than Herschel for the following reasons:
 
We need to gather data from wavelengths other than Herschel for the following reasons:
# To prepare the SED of the proto-stars
+
* To prepare the SED of the proto-stars
# To prepare a list of all known pre-main sequence stars (all classes).
+
* To prepare a list of all known pre-main sequence stars (all classes).
# To  
+
* To compare image morphology and distribution of stars, gas, dust and other components of the star-forming region.
 +
 
  
 
==Near Infrared==
 
==Near Infrared==
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===Apex+Saboca/Laboca?===
 
===Apex+Saboca/Laboca?===
 
* Carol
 
* Carol
 +
* Apex Archive: http://archive.eso.org/wdb/wdb/eso/apex/form
 
* This will be an investigation on whether they have looked at NGC 281.
 
* This will be an investigation on whether they have looked at NGC 281.
  

Latest revision as of 21:33, 21 March 2013

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

  • To prepare the SED of the proto-stars
  • To prepare a list of all known pre-main sequence stars (all classes).
  • To compare image morphology and distribution of stars, gas, dust and other components of the star-forming region.


Near Infrared

X-ray

  • Lynn
  • Catalog of sources
  • Chandra
  • (Not sure, but these may be useful for comparing)

2MASS survey

  • Lynn
  • Photometry
  • Images

Megeath & Wilson

  • Melissa
  • (We may not need this in the end with 2MASS, but worth investigating).
  • Photometry
  • Images?

Spitzer IRAC

  • Melissa
  • Photometry
  • Images


Mid Infrared

WISE

  • Peggy
  • Photometry
  • Images

Spitzer/MIPS

  • Carol
  • 24um photometry
  • 24um Images


Sub-mm

Apex+Saboca/Laboca?

Other sources?

  • Peggy
  • This is an investigation into whether any other sub-mm observatories (e.g. ISO, Caltech Submm Observatory) has looked at NGC 281. And, if that data is useful for us.