Difference between revisions of "CG4 Fall Work"
m (→Recap) |
m |
||
| Line 5: | Line 5: | ||
Backing up one step to review: | Backing up one step to review: | ||
| − | + | ==Goal & Proposal== | |
| + | the goal here is to look for old and new YSOs using all the archival data we can find. Our original proposal is here: | ||
http://coolcosmos.ipac.caltech.edu/cosmic_classroom/teacher_research/r4-cg4/cg4Proposal.pdf | http://coolcosmos.ipac.caltech.edu/cosmic_classroom/teacher_research/r4-cg4/cg4Proposal.pdf | ||
but also linked from our research activities page | but also linked from our research activities page | ||
| Line 13: | Line 14: | ||
[NB: In practice, by the AAS, i don't think we will get to the X-rays we advertised, nor the spectroscopy, but we will include the optical through 24 um photometry; see below.] | [NB: In practice, by the AAS, i don't think we will get to the X-rays we advertised, nor the spectroscopy, but we will include the optical through 24 um photometry; see below.] | ||
| − | + | ==Deadlines== | |
| + | the deadlines we are working towards are: | ||
#Oct 1 for AAS abstracts to be turned in | #Oct 1 for AAS abstracts to be turned in | ||
#early Jan for poster printing in time for me to carry them to the AAS. | #early Jan for poster printing in time for me to carry them to the AAS. | ||
| − | + | ==What we've done so far== | |
| + | the stuff we did last June is summarized here: | ||
http://coolwiki.ipac.caltech.edu/index.php/Working_with_CG4%2BSA101 | http://coolwiki.ipac.caltech.edu/index.php/Working_with_CG4%2BSA101 | ||
and for each of the big steps, there is an indication of what we did together and what i originally expected for you to continue to do on your own. | and for each of the big steps, there is an indication of what we did together and what i originally expected for you to continue to do on your own. | ||
'''At this point, I'm assuming that you remember and fully understand everything that we did together through the "making color-color and color-magnitude plots" step.''' The stuff below that we still need to complete includes the last two steps from the "working with cg4 and sa101" page: "making seds" and "analyzing seds". If you do NOT understand what we did before, now is the time to go back and review in detail what we did before. If you have specific questions that you can't solve by talking to others and puzzling it out within your sub-group, please let me know and I'll do my best to answer them. | '''At this point, I'm assuming that you remember and fully understand everything that we did together through the "making color-color and color-magnitude plots" step.''' The stuff below that we still need to complete includes the last two steps from the "working with cg4 and sa101" page: "making seds" and "analyzing seds". If you do NOT understand what we did before, now is the time to go back and review in detail what we did before. If you have specific questions that you can't solve by talking to others and puzzling it out within your sub-group, please let me know and I'll do my best to answer them. | ||
Revision as of 18:23, 9 September 2010
This page is to capture the plans and results of our work in Fall.
Recap
Backing up one step to review:
Goal & Proposal
the goal here is to look for old and new YSOs using all the archival data we can find. Our original proposal is here: http://coolcosmos.ipac.caltech.edu/cosmic_classroom/teacher_research/r4-cg4/cg4Proposal.pdf but also linked from our research activities page http://coolwiki.ipac.caltech.edu/index.php/CG4_Current_Research_Activities there is a page on the proposal which links to the final proposal as well.
[NB: In practice, by the AAS, i don't think we will get to the X-rays we advertised, nor the spectroscopy, but we will include the optical through 24 um photometry; see below.]
Deadlines
the deadlines we are working towards are:
- Oct 1 for AAS abstracts to be turned in
- early Jan for poster printing in time for me to carry them to the AAS.
What we've done so far
the stuff we did last June is summarized here: http://coolwiki.ipac.caltech.edu/index.php/Working_with_CG4%2BSA101 and for each of the big steps, there is an indication of what we did together and what i originally expected for you to continue to do on your own. At this point, I'm assuming that you remember and fully understand everything that we did together through the "making color-color and color-magnitude plots" step. The stuff below that we still need to complete includes the last two steps from the "working with cg4 and sa101" page: "making seds" and "analyzing seds". If you do NOT understand what we did before, now is the time to go back and review in detail what we did before. If you have specific questions that you can't solve by talking to others and puzzling it out within your sub-group, please let me know and I'll do my best to answer them.
