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== | ||
| + | |||
| + | ===X-ray=== | ||
| + | * Lynn | ||
| + | * Catalog of sources | ||
| + | * [[Chandra]] | ||
| + | * (Not sure, but these may be useful for comparing) | ||
===2MASS survey=== | ===2MASS survey=== | ||
| + | * Lynn | ||
* Photometry | * Photometry | ||
* Images | * Images | ||
| − | |||
===Megeath & Wilson=== | ===Megeath & Wilson=== | ||
| + | * Melissa | ||
| + | * (We may not need this in the end with 2MASS, but worth investigating). | ||
* Photometry | * Photometry | ||
* Images? | * Images? | ||
| − | |||
===Spitzer IRAC=== | ===Spitzer IRAC=== | ||
| + | * Melissa | ||
* Photometry | * Photometry | ||
* Images | * Images | ||
| Line 25: | Line 34: | ||
===WISE=== | ===WISE=== | ||
| + | * Peggy | ||
* Photometry | * Photometry | ||
* Images | * Images | ||
| − | |||
===Spitzer/MIPS=== | ===Spitzer/MIPS=== | ||
| + | * Carol | ||
* 24um photometry | * 24um photometry | ||
* 24um Images | * 24um Images | ||
| + | |||
| + | |||
| + | ==Sub-mm== | ||
| + | |||
| + | ===Apex+Saboca/Laboca?=== | ||
| + | * 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. | ||
| + | |||
| + | ===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. | ||
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.
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
- Apex Archive: http://archive.eso.org/wdb/wdb/eso/apex/form
- 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.
