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| − | Bright-rimmed Clouds Things to do
| + | =[[Marcella's July List of Things To Do]]= |
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| − | 1. Read Chauhan (Chauhan N, Pandey A.K., Ogura K., Ojha D.K., Bhatt B.C., Ghosh S.K., Rawat P.S., 2009, MNRAS, 396, 964.)[http://adsabs.harvard.edu/abs/2009MNRAS.396..964C |link to paper]
| + | =[[BRC Optical Ground-Based Follow-Up]]= |
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| − | 2. Read CG4 [http://lanl.arxiv.org/PS_cache/arxiv/pdf/1105/1105.1180v1.pdf |link to paper]
| + | =[[Identification of Previously Known Objects on Candidate List]]= |
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| − | 3. Feedback form by Sunday 7/17 to your teacher
| + | =[[Matching to Spitzer and Weeding the SEDs]]= |
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| − | 4. Make sure that we have all the data available for both clouds.
| + | =[[Please, just put all the BRC data tables in one place]]= |
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| − | *a. All the known objects
| + | I put the "check photometry on BRC 27" table on this page... |
| − | *b. All the “unknown objects”
| + | --[[User:CJohnson|CJohnson]] 15:56, 21 October 2011 (PDT) |
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| − | 5. Finish BRC 27 then work on BRC 34.
| + | =Posters!!= |
| | + | [[File:education poster.pptx]] |
| | + | --[[User:Linahan|Linahan]] 11:21, 21 December 2011 (PST) |
| | + | [[file:brceduposter.pdf]] pdf version |
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| − | 6. Answer all the questions in the Working with the BRCs. Type them up if necessary.
| + | [[File:SciPoster_BRC.ppt]] ... rough, rough, rough draft |
| | + | --[[User:CJohnson|CJohnson]] 15:29, 21 December 2011 (PST) |
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| − | 7. Post the URL’s for the different bands on the Wiki in the relevant links section.
| + | [[File:SciPoster_BRC2.ppt]] ... second ... |
| | + | --[[User:CJohnson|CJohnson]] 08:52, 28 December 2011 (PST) |
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| − | 8. Watch the YouTube videos for each section.
| + | [[File:SciPoster_BRC3.ppt]] ... third ... includes changes talked about in today's telecon + color-color, color-magnitude diagrams. Comments welcome. Sorry, can't find room for a yak but I'll keep working on the NASA logo. |
| − | | + | --[[User:CJohnson|CJohnson]] 09:51, 28 December 2011 (PST) |
| − | 9. Where is the BRC? What is a point source? What is the BRC? What is a foreground star?
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| − | 10. Under Previously identified sources, checking the duplicates.
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| − | 11. What is photometry? What is it measured in? What do we convert it into?
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| − | 12. What does APT really do for you?
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| − | 13. Why does the MOPEX source pick up wrong objects and miss others?
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| − | 14. Working with the data tables: Save files in a standard format
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| − | *a. BRC number
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| − | *b. Cand or known
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| − | *c. Underscore
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| − | *d. Initials
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| − | *e. underscore
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| − | *f. Two-number date
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| − | *g. Three letter month code
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| − | *h. Example: 27cand_chj_09jul.xls
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| − | 15. Data tables:
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| − | *a. Make SEDS with the all 38 candidate objects.
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| − | 16. Color-color diagram
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| − | 17. Color-magnitude diagram
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| − | Long-term goals:
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| − | 1. “Pretty pictures” for poster. Three-color images of BRC-27 and BRC-34.
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| − | 2. Science poster
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| − | 3. Education poster
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| − | 4. paper?
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| − | --[[User:Linahan|Linahan]] 14:20, 9 July 2011 (PDT)
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| − | Extra notes:
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| − | Powerpoint 1:
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| − | NASA has some great observatories.
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| − | Why do we need to use different telescopes?
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| − | 1. “To see different things”
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| − | *a. X-rays vs. gamma rays
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| − | *b. Atmosphere absorbs certain wavelengths
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| − | *c. Atmosphere is opaque to certain wavelengths
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| − | *d. Dusty regions are not seen in optical, can’t see through it
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| − | 2. Why are we using archival data?
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| − | *a. Data does need to be sorted but by the computers but
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| − | *b. Cryogen is gone.
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| − | *c. Surpassed its lifetime.
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| − | *d. 3 & 4 and MIPS is gone but lots of data just haven’t been looked at
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| − | *e. Hotter objects shorter waves
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| − | Powerpoint 2:
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| − | 1. What is SSC?
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| − | *a. Spitzer Science Center
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| − | 2. Wavelengths and bands
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| − | *a. Bands are x number across but numbers correspond to center
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| − | 3. Using heritage data
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| − | 4. Hopefully use WISE data
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| − | 5. Good to look through the rest of packet
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| − | 6. P. 34 jail bars and instrument artifacts. Washed out some of the things around it. Messy.
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| − | | |
| − | *a. If we found this, we could smooth it out not scientific information
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| − | 7. Chemistry and elements used
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| − | Powerpoint 3:
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| − | 1. Star formation. Major topic on top of page 3.
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| − | *a. Small stars and stars with dusty disk
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| − | *b. Phase 0 yee hah yakky yak
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| − | *c. Probably won’t be able to pin down the age of the object but will not be able to pin down the distance.
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| − | *d. Links and files to movies
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| − | 2. Extrasolar planets are hot topic
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| − | *a. Iphone app to let you know when new planets are found
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| − | PowerPoint 4:
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| − | 1. Most important. Goals:
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| − | *a. Science poster
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| − | **i. Paper written
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| − | *b. Education poster:
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| − | **i. How can we bring this to other students?
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| − | **ii. How has it opened new doors for you?
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| − | **iii. STEM careers
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| − | **iv. Writing
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| − | *c. Other teams will have at least 2 posters
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| − | 2. Classes on pg. 7 and how it relates to SEDs
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| − | *a. How is the energy distributed over different wavelengths
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| − | 3. Blackbodies
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| − | *a. Perfect radiators
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| − | *b. Give off all the energy that they produce
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| − | 4. SEDs
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| − | *a. Slopes: left and right
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| − | 5. Color-color diagrams p. 15
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| − | *a. Magnitudes
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| − | *b. Reddening of the object
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| − | 6. Photometry
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| − | *a. Not using the MOPEX program
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| − | --[[User:Linahan|Linahan]] 14:20, 9 July 2011 (PDT) | |
