Difference between revisions of "SHIPsProposal"

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−
==SHIPs Proposal==
+
==Abstract==
 +
A short, one or two paragraph, summary of the main points:
 +
* Scientific goals of the proposal
 +
* Proposed observations
 +
 
  
−
===Abstract===
+
==Science Introduction and Context==
−
A short, one or two paragraph, summary of the main points:
 
−
* What do we intend to do?
 
−
* Why is it important?
 
−
* How will we do it?
 
  
−
===Science Introduction and Context===
 
 
Topics to consider when writing this section.
 
Topics to consider when writing this section.
−
*Background
+
*Background -- The broad picture.
−
** What is the scientific context of the work?
+
** Why is star-formation important? (LYNN)
−
** Why is this important?
+
** What do we know about star-formation.  We will likely trim this to suit our goals as the proposal matures? (LYNN)
−
** What is known, and not known?
+
** What are the big unknowns? (LYNN)
  
 
{| class="wikitable"
 
{| class="wikitable"
Line 24: Line 23:
 
! scope="coI"| Assignment
 
! scope="coI"| Assignment
 
|-
 
|-
−
|[http://www.annualreviews.org/doi/abs/10.1146/annurev.astro.44.051905.092549?journalCode=astro Zinnecker & Yorke (2007)]
+
|NITARP pages
−
|Toward Understanding Massive Star Formation
+
|Our internal NITARP pages from Luisa, me and others.  These are okay because they are one of your source of knowledge on the subject.
−
|Review article on massive star formation
+
|
−
|May need to get a free copy.
+
|
 +
|
 +
|-
 +
|[http://adsabs.harvard.edu/abs/2007ARA%26A..45..565M McKee & Osteriker (2007)]
 +
|Theory of Star Formation
 +
|Review article
 +
|Available for free via the arXiv link.
 
|
 
|
 
|-
 
|-
−
|[http://adsabs.harvard.edu/abs/2008ApJS..179..249D Dunham et al. (2008)]
+
|[http://arxiv.org/pdf/astro-ph/0306595v2.pdf Larson (2003)]
−
|Identifying the Low-Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores
+
|The physics of star formation.
 +
|Another review with useful points to refer to.
 
|
 
|
 
|
 
|
 +
|}
 +
 +
 +
* This work
 +
** What aspect of star formation will we address in this work? (PEGGY)
 +
** What is star formation rate? (PEGGY)
 +
** How does triggered star formation work?  (PEGGY)
 +
** How is triggered star formation and star formation rates useful in understanding star formation process? (PEGGY)
 +
 +
 +
{| class="wikitable"
 +
|+Reading List
 +
|-
 +
! scope="col"| Paper
 +
! scope="col"| Title
 +
! scope="col"| Description
 +
! scope="col"| Comments
 +
! scope="coI"| Assignment
 +
|-
 +
|[http://adsabs.harvard.edu/abs/1998ASPC..148..150E Elmegreen (1998)]
 +
|Observations and Theory of Dynamical Triggers for Star Formation
 +
|The paper by The author on triggered star-formation.
 
|
 
|
 +
|[[File:Piper Proposal 20130303.docx | Piper Proposal 20130303]]
 
|-
 
|-
 
|[http://adsabs.harvard.edu/abs/2009ApJS..181..321E Evans et al. (2009)]
 
|[http://adsabs.harvard.edu/abs/2009ApJS..181..321E Evans et al. (2009)]
 
|The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes
 
|The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes
 +
|Discussion of efficiencies, rates and lifetimes.
 
|
 
|
−
|
+
|[[File:Piper Evans.docx | Piper Evan's braindump]]
−
|
 
 
|}
 
|}
  
  
−
* This work
+
* This work (cont.)
−
** What aspect of the "unknown" will we address in this work?
+
** What target did we pick? (MELISSA)
−
** Why is this interesting?  How will it help?
+
** What do we know about NGC 281? (MELISSA)
−
* Target (An important part of carrying on the work).
+
** What is the evidence for triggered star formation in NGC 281? (MELISSA)
−
** What target did we pick?
+
** What is the evidence for young stars in NGC 281? (MELISSA)
−
** Why this target?
 
−
** What is known in the literation?
 
  
 
{| class="wikitable"
 
{| class="wikitable"
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! scope="col"| Comments
 
! scope="col"| Comments
 
! scope="coI"| Assignment
 
! scope="coI"| Assignment
 +
|-
 +
|[http://adsabs.harvard.edu/abs/1997AJ....114.1106M Megeath & Wilson (1997)]
 +
|The NGC 281 west cluster. I. Star formation in photoevaporating clumps.
 +
|Establishes NGC 281 as a site of triggered SF.
 +
|[[File:Megeath97.pdf | PDF version]]
 +
|[[File:NITARP Proposal Booker.docx | Melissa's attempt at her section of the proposal]]
 
|-
 
|-
 
|[http://adsabs.harvard.edu/abs/1997AJ....113.2116G Guetter & Turner (1997)]
 
|[http://adsabs.harvard.edu/abs/1997AJ....113.2116G Guetter & Turner (1997)]
 
|IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281
 
|IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281
 +
|The seminal paper on NGC 281.
 
|
 
|
 
|
 
|
 +
|-
 +
|[http://adsabs.harvard.edu/abs/2012ApJ...744..130K Koenig et al (2012)]
 +
|Wide-field Infrared Survey Explorer Observations of the Evolution of Massive Star-forming Regions
 +
|Good use of WISE
 +
|Possibly picked up by Babar for our review
 
|
 
|
 
|-
 
|-
−
|[http://adsabs.harvard.edu/abs/1997AJ....114.1106M Megeath & Wilson (1997)]
+
|[http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2012PASJ...64..107S&db_key=AST&nosetcookie=1 Sharma et al. (2012)]
−
|The NGC 281 west cluster. I. Star formation in photoevaporating clumps.
+
|Multiwavelength Study of the NGC 281 Region
−
|
 
 
|
 
|
 +
|Picked up by Babar
 
|
 
|
 
|}
 
|}
  
  
−
** What do we expect to find based on above?
+
* This work (cont.)
−
* What Observations do we propose to do?
+
** What Observations do we propose to do? (CAROL)
−
** What diagnostics will we use?
+
** What/which properties of NGC 281 do we wish to study? (CAROL)
 +
** What diagnostics will we use? (CAROL)
 +
** How will these diagnostics tell us about our proposed goals/question to study? (CAROL)
 +
 
 +
{| class="wikitable"
 +
|+Reading List
 +
|-
 +
! scope="col"| Paper
 +
! scope="col"| Title
 +
! scope="col"| Description
 +
! scope="col"| Comments
 +
! scope="coI"| Assignment
 +
|-
 +
|[http://adsabs.harvard.edu/abs/2012arXiv1212.1160F Fischer et al. (2012)]
 +
|Results from HOPS: A Multiwavelength Census of Orion Protostars
 +
|Studying protostars with Herschel
 +
|
 +
|[[File:Carol's Proposal Section.docx | ]]
 +
|-
 +
|[http://adsabs.harvard.edu/abs/2009ApJS..181..321E Evans et al. (2009)]
 +
|The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes
 +
|How do we determine efficiencies and rates.
 +
|
 +
|
 +
|-
 +
|[http://adsabs.harvard.edu/abs/2008ApJS..179..249D Dunham et al. (2008)]
 +
|Identifying the Low-Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores
 +
|Why do we need data at Herschel wavelengths.
 +
|
 +
|
 +
|}
  
−
===Analysis plan===  
+
==Analysis plan==  
 
Specifics about data and what to do with the data.
 
Specifics about data and what to do with the data.
 
* How will the data be readied for this study? (Technical term: reduced, or processed).
 
* How will the data be readied for this study? (Technical term: reduced, or processed).
Line 86: Line 155:
 
** How will we supplement our data?   
 
** How will we supplement our data?   
 
** How will we combine data?   
 
** How will we combine data?   
 +
 +
{| class="wikitable"
 +
|+Reading List
 +
|-
 +
! scope="col"| Paper
 +
! scope="col"| Title
 +
! scope="col"| Description
 +
! scope="col"| Comments
 +
! scope="coI"| Assignment
 +
|-
 +
|
 +
|
 +
|
 +
|
 +
|
 +
|}
 +
 +
 
* What tools will we use?
 
* What tools will we use?
 
** To work with the data
 
** To work with the data
 
** To produce the diagnostic plots.
 
** To produce the diagnostic plots.
  
−
===Educational/Outreach plan===   
+
{| class="wikitable"
 +
|+Reading List
 +
|-
 +
! scope="col"| Paper
 +
! scope="col"| Title
 +
! scope="col"| Description
 +
! scope="col"| Comments
 +
! scope="coI"| Assignment
 +
|-
 +
|
 +
|
 +
|
 +
|
 +
|
 +
|}
 +
 
 +
 
 +
==Educational/Outreach plan==   
 
* The education angle for the general public.
 
* The education angle for the general public.
 
* Implication for public education?
 
* Implication for public education?
 
* Press release?
 
* Press release?
 
* Image release?
 
* Image release?
 +
 +
==Current Version of the Proposal==
 +
 +
[[File:SHIPS_Proposal_v03_03b.docx| ]]
 +
 +
[[File:SHIPS_Proposal_v03_04.docx| ]]
 +
 +
[[File:SHIPS_Proposal_v03_04b.docx | Version 9:22pm PST 4-March ]]
 +
 +
[[File:SHIPS_Proposal_v03_04C.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_04C1.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_05a.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_05b.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_05c.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_05d.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_06a.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_06b.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_06C.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_06d.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_06d1.docx|Version with Lynn's Education Outreach]]
 +
 +
[[File:SHIPS_Proposal_v03_07a.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_07b.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_07c.docx]]
 +
 +
[[File:SHIPS_Proposal_v03_07d.docx]]
 +
 +
[[File:SHIPS_Proposal_FINAL.docx]]

Latest revision as of 11:19, 8 March 2013

Abstract

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

  • Scientific goals of the proposal
  • Proposed observations


Science Introduction and Context

Topics to consider when writing this section.

  • Background -- The broad picture.
    • Why is star-formation important? (LYNN)
    • What do we know about star-formation. We will likely trim this to suit our goals as the proposal matures? (LYNN)
    • What are the big unknowns? (LYNN)
Reading List
Paper Title Description Comments Assignment
NITARP pages Our internal NITARP pages from Luisa, me and others. These are okay because they are one of your source of knowledge on the subject.
McKee & Osteriker (2007) Theory of Star Formation Review article Available for free via the arXiv link.
Larson (2003) The physics of star formation. Another review with useful points to refer to.


  • This work
    • What aspect of star formation will we address in this work? (PEGGY)
    • What is star formation rate? (PEGGY)
    • How does triggered star formation work? (PEGGY)
    • How is triggered star formation and star formation rates useful in understanding star formation process? (PEGGY)


Reading List
Paper Title Description Comments Assignment
Elmegreen (1998) Observations and Theory of Dynamical Triggers for Star Formation The paper by The author on triggered star-formation. File:Piper Proposal 20130303.docx
Evans et al. (2009) The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes Discussion of efficiencies, rates and lifetimes. File:Piper Evans.docx


  • This work (cont.)
    • What target did we pick? (MELISSA)
    • What do we know about NGC 281? (MELISSA)
    • What is the evidence for triggered star formation in NGC 281? (MELISSA)
    • What is the evidence for young stars in NGC 281? (MELISSA)
Reading List
Paper Title Description Comments Assignment
Megeath & Wilson (1997) The NGC 281 west cluster. I. Star formation in photoevaporating clumps. Establishes NGC 281 as a site of triggered SF. File:Megeath97.pdf File:NITARP Proposal Booker.docx
Guetter & Turner (1997) IC 1590, A Young Cluster Embedded in the Nebulosity of NGC 281 The seminal paper on NGC 281.
Koenig et al (2012) Wide-field Infrared Survey Explorer Observations of the Evolution of Massive Star-forming Regions Good use of WISE Possibly picked up by Babar for our review
Sharma et al. (2012) Multiwavelength Study of the NGC 281 Region Picked up by Babar


  • This work (cont.)
    • What Observations do we propose to do? (CAROL)
    • What/which properties of NGC 281 do we wish to study? (CAROL)
    • What diagnostics will we use? (CAROL)
    • How will these diagnostics tell us about our proposed goals/question to study? (CAROL)
Reading List
Paper Title Description Comments Assignment
Fischer et al. (2012) Results from HOPS: A Multiwavelength Census of Orion Protostars Studying protostars with Herschel File:Carol's Proposal Section.docx
Evans et al. (2009) The Spitzer c2d Legacy Results: Star-Formation Rates and Efficiencies; Evolution and Lifetimes How do we determine efficiencies and rates.
Dunham et al. (2008) Identifying the Low-Luminosity Population of Embedded Protostars in the c2d Observations of Clouds and Cores Why do we need data at Herschel wavelengths.

Analysis plan

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?
Reading List
Paper Title Description Comments Assignment


  • What tools will we use?
    • To work with the data
    • To produce the diagnostic plots.
Reading List
Paper Title Description Comments Assignment


Educational/Outreach plan

  • The education angle for the general public.
  • Implication for public education?
  • Press release?
  • Image release?

Current Version of the Proposal

File:SHIPS Proposal v03 03b.docx

File:SHIPS Proposal v03 04.docx

File:SHIPS Proposal v03 04b.docx

File:SHIPS Proposal v03 04C.docx

File:SHIPS Proposal v03 04C1.docx

File:SHIPS Proposal v03 05a.docx

File:SHIPS Proposal v03 05b.docx

File:SHIPS Proposal v03 05c.docx

File:SHIPS Proposal v03 05d.docx

File:SHIPS Proposal v03 06a.docx

File:SHIPS Proposal v03 06b.docx

File:SHIPS Proposal v03 06C.docx

File:SHIPS Proposal v03 06d.docx

File:SHIPS Proposal v03 06d1.docx

File:SHIPS Proposal v03 07a.docx

File:SHIPS Proposal v03 07b.docx

File:SHIPS Proposal v03 07c.docx

File:SHIPS Proposal v03 07d.docx

File:SHIPS Proposal FINAL.docx

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