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  • ...abstract, Debbie's table (wasn't sure where to put it), put some words in for JD's educational stuff. [[Media:CWAYS Proposal 031512.docx]] Initial Skeleton for Proposal [[File:CWAYS Proposal Format.docx]]--Peggy Piper 12:52, 24 Februar
    17 KB (2,838 words) - 18:10, 6 May 2012
  • ...(K-college). This is one for blackbody spectra that some NITARP teachers' students found helpful. Most of these have lessons teachers uploaded. Those done by ..._in_depth.2C_and_SEDs| page on studying young stars]] has examples of SEDs for, you guessed it, young stars.
    8 KB (1,406 words) - 17:05, 31 July 2020
  • ...ons we were studying in those years. Similar worksheets could be developed for any given region. * find rotation periods for set of K2 LCs - throw in periodic/not, noisy/not, sinusoidal/not, single/mu
    7 KB (1,074 words) - 16:32, 6 October 2022
  • ...eriodicity. Determining the periodicity of such stars will provide a basis for later comparison against light curves identified as potential planetary tra While the Kepler Mission was primarily designed to look for exoplanet transits using photometric measurements of a static field of star
    20 KB (3,148 words) - 02:08, 12 June 2011
  • ...Working 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 FOR REFERENCE: [[BRC Bigger Picture and Goals]]
    33 KB (5,401 words) - 15:00, 23 September 2011
  • ...There will be minimal help from me on June 28 as sort of a "training run" for when you go home. (It is also a 'safety valve' if we don't get enough done ...AM 9:15? - intro lectures and activities, then get started on data! (break for lunch circa noon)
    10 KB (1,810 words) - 19:07, 20 July 2016
  • ...There will be minimal help from me on June 19 as sort of a "training run" for when you go home. (It is also a 'safety valve' if we don't get enough done *Wed AM- JPL Tour -- entry at 8:45 for badging, tour starts at 9
    10 KB (1,789 words) - 21:16, 10 June 2015
  • ...ce Telescope takes images at several wavelengths, with different cameras. For example, Spitzer took three separate images of M81: one recording IR radiat ...the different wavelengths, but all of these wavelengths are much too long for human eyes to see. So scientists record these 'invisible' wavelengths and
    15 KB (2,609 words) - 16:32, 1 March 2016
  • ...EW OF STAR FORMATION IN GENERAL. textbooks, overview articles, good things for general knowledge. *[[target selection for brc34]] 21h32m51.2s +58d08m43s DECIDED ON THIS ONE
    21 KB (3,168 words) - 16:20, 26 May 2011
  • ...of various instruments and missions is and will be a very important thing for us to consider in the course of assessing the literature studies of our reg ...general introduction, please start with the main text already on the wiki for [[Resolution]]. Please also look at the examples lower on that page, but yo
    26 KB (4,762 words) - 16:51, 27 March 2012
  • * detailed information on what data are available, and what you plan to do with it (e.g. much more =Background information=
    33 KB (5,123 words) - 17:24, 17 April 2013
  • '''For a comprehensive introduction to APT, please see [http://www.aperturephotome ...urately as possible - the better your initial guess, the easier it will be for the computer to correctly centroid the object.
    17 KB (2,902 words) - 03:49, 7 August 2013
  • the goal here is to look for old and new YSOs using all the archival data we can find. Our original pro #Oct 1 for AAS abstracts to be turned in
    17 KB (2,788 words) - 02:44, 24 January 2011
  • ...of various instruments and missions is and will be a very important thing for us to consider in the course of assessing the literature studies of our reg ...general introduction, please start with the main text already on the wiki for [[Resolution]]. Please also look at the examples lower on that page, but yo
    29 KB (5,314 words) - 18:02, 17 June 2013
  • ...and 2 with Spitzer GLIMPSE IRAC channel 1 and 2, which we can do in spades for IC417. ...itzer vs. 2MASS resolution; and (2) understand what the challenges will be for us in matching across wavelengths. '''Ancillary goals''' (e.g., you can't d
    30 KB (5,229 words) - 22:18, 30 March 2015
  • ...hannel 1 and 2 with Spitzer IRAC channel 1 and 2, but it will matter a lot for the SCUBA data, the Herschel data, and the Chandra X-ray data too. ...itzer vs. 2MASS resolution; and (2) understand what the challenges will be for us in matching across wavelengths. '''Ancillary goals''' (e.g., you can't d
    30 KB (5,370 words) - 04:20, 30 March 2016
  • ...l resolution of various instruments and missions is a very important thing for us to consider in the course of our work. A key goal of ours is to check an ...general introduction, please start with the main text already on the wiki for [[Resolution]]. Please also look at the examples lower on that page, but yo
    30 KB (5,592 words) - 23:31, 31 March 2014
  • ...(and the telescopes are different), but it will matter a lot in particular for the SCUBA and Herschel data. ...SS vs. Herschel resolution; and (2) understand what the challenges will be for us in matching across wavelengths. '''Ancillary goals''' (e.g., you can't d
    32 KB (5,692 words) - 16:18, 13 April 2017
  • ...different). Spatial resolution differences will matter a lot in particular for the Herschel data. ...2MASS vs. Herschel resolution. (3) understand what the challenges will be for us in matching across wavelengths. '''Ancillary goals''' (e.g., you can't d
    35 KB (6,288 words) - 15:39, 11 April 2018
  • ...nking about the issues of spatial resolution. I have developed a worksheet for this. '''WE DECIDED TO DO THIS FIRST.''' ...tronomy and astrophysics background, and/or for the interpretation, and/or for the big picture... ones from which you need to scavenge data, and you need
    34 KB (5,550 words) - 04:03, 6 June 2012

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