Difference between revisions of "2011 proposal instructions"

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You don't have page limits, but nor do you want the review committee annoyed because you made them read a book.... or tiny fonts.  A professor in grad school always used to annoy me with broad essay questions followed by the instruction "Be brief but specific."  But he's right ...
 
You don't have page limits, but nor do you want the review committee annoyed because you made them read a book.... or tiny fonts.  A professor in grad school always used to annoy me with broad essay questions followed by the instruction "Be brief but specific."  But he's right ...
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'''Science Introductions and Context'''
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The role of Bright Rimmed Clouds (BRC’s) in star-formation processes makes them a topic of ongoing interest.  Whether external ionization shocks compress the neutral gas into compact globules or bright rims, the boundary between neutral gas and gas ionized by incident photons is thought to be rich in potential sites for star formation.  Drawn from the lists of Sugitani, Fukui, and Ogura (1991), Allen and Peterson (2010?) imaged 32 bright-rimmed clouds located at estimated distances d < 1.2 kpc, finding young stellar objects in 75% of the clouds they studied.
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We propose to conduct further examinations of BRC 27 and BRC 34 to search for additional young stellar objects.  BRC 27 is located in the molecular cloud Canis Majoris R1.  BRC 34 has a variety of features worthy of deeper examination; dark nebulae, molecular and IC clouds, emission stars, and IR sources.  Allen and Peterson found one Class I protostar and far more Class II T-Tauri stars in BRC’s 27 and 34.  Beyond that, these two BRC’s have not been well studied.  We believe there is more to find in these BRC’s using Spitzer Space Telescope wavelengths.
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--[[User:Sartore|Sartore]] 18:05, 22 February 2011 (PST)
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(help me out here...Am I citing work correctly?  Finding out anything about these two BRC's was a major effort.  I've got more details, but do not know whether I would be stepping on other parts of the proposal. - Diane)
  
 
= Examples =
 
= Examples =

Revision as of 02:05, 23 February 2011

NITARP proposals due March 21!

We have finally picked a due date for your NITARP proposals! They will be due into us by *****noon Pacific time on Monday, March 21.*****

Short summary

Your team should submit one proposal addressing the research you are going to conduct. Your proposal will be reviewed by a committee consisting of astronomers and educators. You will get comments back, and you will be given an opportunity to revise the proposal before it gets posted on the web.

Instructions

The instructions for writing this proposal are relatively open-ended. In general, good proposals should have:

  • Abstract. This in particular will be posted on the web.
  • Science Introduction and Context. Background on subject. What target(s). How you picked the target(s) and why. What is known in the literature about the target(s). Educated guesses on what you expect to find. (Your readers are both astronomers and educators, so don't assume they know the astronomy basics.)
  • Analysis plan. Detailed information on what data are available, and what you plan to do with them (e.g. more than "I'm sure Spitzer observed this at some point"). How you are going to reduce the data. Kind of analysis planned. Tools you will use.
  • Educational/Outreach plan. What your team plans to do, individually or as a group. No need to link to standards or describe this in great detail. Most of your work should go into the science portion of the proposal; this is mostly to make sure that you have started thinking about the educational aspects of this program.

You don't have page limits, but nor do you want the review committee annoyed because you made them read a book.... or tiny fonts. A professor in grad school always used to annoy me with broad essay questions followed by the instruction "Be brief but specific." But he's right ...

Science Introductions and Context The role of Bright Rimmed Clouds (BRC’s) in star-formation processes makes them a topic of ongoing interest. Whether external ionization shocks compress the neutral gas into compact globules or bright rims, the boundary between neutral gas and gas ionized by incident photons is thought to be rich in potential sites for star formation. Drawn from the lists of Sugitani, Fukui, and Ogura (1991), Allen and Peterson (2010?) imaged 32 bright-rimmed clouds located at estimated distances d < 1.2 kpc, finding young stellar objects in 75% of the clouds they studied.

We propose to conduct further examinations of BRC 27 and BRC 34 to search for additional young stellar objects. BRC 27 is located in the molecular cloud Canis Majoris R1. BRC 34 has a variety of features worthy of deeper examination; dark nebulae, molecular and IC clouds, emission stars, and IR sources. Allen and Peterson found one Class I protostar and far more Class II T-Tauri stars in BRC’s 27 and 34. Beyond that, these two BRC’s have not been well studied. We believe there is more to find in these BRC’s using Spitzer Space Telescope wavelengths. --Sartore 18:05, 22 February 2011 (PST) (help me out here...Am I citing work correctly? Finding out anything about these two BRC's was a major effort. I've got more details, but do not know whether I would be stepping on other parts of the proposal. - Diane)

Examples

Want to see some examples?? All of the previous proposals are online, linked from the teams' individual Cool Cosmos pages. Here are direct links to the proposals from last year:

You can see they vary a lot in style and content! :)

Suggested path from here

We suggest that you appoint one person as the lead for coordinating the proposal, and that you appoint the other people to assemble initial drafts of various proposal sections. We recommend that you do not submit your proposal until your scientist has read it, given you comments, and you have addressed these comments in your proposal. If you don't, almost certainly these same comments will reappear in your proposal feedback!

(NB: In a real proposal call, there will typically be between 3 and 5 times as many proposals as can be supported, and the review committee decides which 20-30% of the proposals get funded or get observing time. In our case, no one is getting rejected. The opportunity to rewrite your proposal in response to referee comments is more akin to writing a scientific article. Anyway.)

We also recommend that you establish regular communication among your team during this process. Telecons (weekly? bi-weekly), email, and the wiki will all be helpful in this. When you are ready with a team nickname, I will set up your wiki area. Just let me know!

Questions? Ask your mentor teacher, your scientist, or Luisa! :)