Difference between revisions of "SHIPsDataAssignments"
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==Sub-mm== | ==Sub-mm== | ||
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===Apex+Saboca/Laboca?=== | ===Apex+Saboca/Laboca?=== | ||
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===Other sources?=== | ===Other sources?=== | ||
* Peggy | * Peggy | ||
| − | * This is an investigation into whether any other sub-mm observatories (e.g. Caltech Submm Observatory) has looked at NGC 281. And, if that data is useful for us. | + | * 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. |
Revision as of 21:19, 15 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
Contents
Near Infrared
X-ray
- Lynn
- Catalog of sources
- (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.
