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 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== | ==Near Infrared== | ||
Revision as of 21:00, 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.
Contents
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?
- Carol
- This will be an investigation on whether they have looked at NGC 281.
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.
