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• Background/general reference
  =Starting from the very beginning= [[How science works and other philosophical musings]]
  3 KB (543 words) - 20:10, 11 August 2020
• OLD main page
  ...or the NASA IPAC Teacher Archive Research Program (NITARP) [used to be the Spitzer Teachers Research Project]'''</big> = What is the NASA IPAC Teacher Archive Research Program (NITARP)?=
  6 KB (938 words) - 21:51, 27 July 2020
• Skill development
  ...of doing scientific research! This page has information both on searching and reading literature. [[Viewing FITS files]] -- using tools (e.g., IRSA tools or ds9) to view and manipulate FITS images
  5 KB (832 words) - 23:55, 13 November 2020
• What is an archive and why do we need archives?
  .../5/83-why-we-archive-with-dr-rebull?rq=rebull February 05, 2017 episode of the Spacepod podcast]].'' ...ing those data, and we don't want to lose the data! But today's post is on the wider question of why we have archives of astronomy data.
  7 KB (1,208 words) - 22:15, 29 July 2020
• Herschel Space Observatory
  '''A Brief History of the Herschels:''' ...d discovered infrared radiation. His sister Caroline helped him to develop the modern mathematical approach to astronomy.
  19 KB (3,099 words) - 21:16, 2 February 2013
• How can I make a color composite image using Spitzer and/or other data?
  ==Don't forget to try and answer the "Questions to think about ..." at the bottom of this page!== ...erent wavelengths because different elements and compounds absorb and emit light at different wavelengths.
  15 KB (2,609 words) - 16:32, 1 March 2016
• Working with L1688
  ...inish, with the products already done so that you can step into and out of the process as you want or need. ...ng, creating mosaics), the rest are customized to this goal of finding old and new YSOs.
  23 KB (3,988 words) - 20:11, 20 October 2010
• Working with the BRCs
  ...ing with CG4+SA101]] pages, and was developed and updated specifically for the 2011 BRC team visit. Please note: NONE of these pages are meant to be used FOR REFERENCE: [[BRC Bigger Picture and Goals]]
  33 KB (5,401 words) - 15:00, 23 September 2011
• PP Proposal
  National Optical Astronomical Observatory, Tucson, AZ and NASA Ames Research Center, Moffett Field, CA. NASA Exoplanet Science Institute, Infrared Processing and Analysis Center, Pasadena, CA.
  20 KB (3,148 words) - 02:08, 12 June 2011
• BRC Proposal
  STUFF HERE IS GENERAL OVERVIEW OF STAR FORMATION IN GENERAL. textbooks, overview articles ...S 2011 summarizing the NITARP 2010 paper "New Young Star Candidates in CG4 and Sa101", Rebull et all, 2011 [[File:GISS_2011_Legassie_gum_nebula.pptx]]
  21 KB (3,168 words) - 16:20, 26 May 2011
• Working with the C-CWEL data
  ...h L1688]] page. '''This''' page was developed and updated specifically for the 2013 C-CWEL team visit. ...will go back and redo different pieces of this at different stages of your work.
  46 KB (8,082 words) - 17:21, 7 August 2013
• Working with the C-WAYS data
  ...ng with L1688]] page. This page was developed and updated specifically for the 2012 CWAYS team visit. Please note: '''NONE''' of these pages are meant to ...will go back and redo different pieces of this at different stages of your work.
  47 KB (8,224 words) - 19:56, 24 July 2012
• Summaries and questions on discussed papers
  == Barensten 2011 T Tauri candidates and accretion rates using IPHAS:method and application to IC 1396 == * INT is Isaac Newton Telescope (100 inch mirror) in Canary Islands, Spain.
  42 KB (6,796 words) - 20:39, 18 May 2012
• CG4 Proposal
  is here: http://coolcosmos.ipac.caltech.edu/cosmic_classroom/teacher_research/ ...revious proposals are online, linked from the teams' official page. All of the programs are listed here:
  33 KB (5,123 words) - 17:24, 17 April 2013