Difference between revisions of "SHIPsProposal"

Revision as of 20:46, 7 February 2013

A short, one or two paragraph, summary of the main points:

Topics to consider when writing this section.

Background
- What is the scientific context of the work?
- Why is this important?
- What is known, and not known?
This work
- What aspect of the "unknown" will we address in this work?
- Why is this interesting? How will it help?
Target (An important part of carrying on the work).
- What target did we pick?
- Why this target?
- What is known in the literation?

Paper	Title	Description	Comments	Assignment
[[http://adsabs.harvard.edu/abs/1997AJ....113.2116G Guetter & Turner (1997)	IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281
[http://adsabs.harvard.edu/abs/1997AJ....114.1106M Megeath & Wilson (1997)	The NGC 281 west cluster. I. Star formation in photoevaporating clumps.

Specifics about data and what to do with the data.

How will the data be readied for this study? (Technical term: reduced, or processed).
Ancillary data
- Where will we get our data?
- How will we supplement our data?
- How will we combine data?
What tools will we use?
- To work with the data
- To produce the diagnostic plots.

@@ Line 21: / Line 21: @@
 ** Why this target?
 ** What is known in the literation?
+{| class="wikitable"
+|-
+! scope="col"| Paper
+! scope="col"| Title
+! scope="col"| Description
+! scope="col"| Comments
+! scope="coI"| Assignment
+|-
+|[[http://adsabs.harvard.edu/abs/1997AJ....113.2116G Guetter & Turner (1997)
+|IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281
+|
+|
+|
+|-
+|[http://adsabs.harvard.edu/abs/1997AJ....114.1106M Megeath & Wilson (1997)
+|The NGC 281 west cluster. I. Star formation in photoevaporating clumps.
+|
+|
+|
+|}
 ** What do we expect to find based on above?
 * What Observations do we propose to do?