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• IC 417 Bigger Picture and Goals
  We have WISE data for a patch of sky likely to harbor young stars around IC 41 ...rs!!!1!" when in reality 25 of them were found before by someone else, and we are rediscovering them -- rediscovering them independently, mind you, but r
  9 KB (1,543 words) - 22:24, 17 April 2015
• LW discussion of YSOs
  Hey guys, Here's the questions we decided to answer. Write your answers with your signature and list more qu YSOs are almost always found within or near gas and dust in outer space, most often embedded in molecula
  2 KB (369 words) - 21:24, 19 June 2012
• Finding the velocity of a high-proper-motion star in IC2118
  When we were working on finding new YSOs in IC 2118, we found a high proper motion star. ...age proper motion (in RA and Dec directions). Do you get the same numbers we did in section 4.6 of the IC2118 paper?
  3 KB (588 words) - 19:13, 15 June 2023
• SFO Paper Journals Guided Reading
  ...Palomar Sky survey prints that had associated IRAS point sources where all found to have IRAS point sources that were good candidates for being YSOs. Table -what is the flow of all the types of nebulosity that they describe and the cause
  3 KB (423 words) - 16:16, 6 May 2012
• C-CWEL Bigger Picture and Goals
  We have WISE data for a patches of sky likely to harbor young stars around BRC ...rs!!!1!" when in reality 25 of them were found before by someone else, and we are rediscovering them -- rediscovering them independently, mind you, but r
  11 KB (1,936 words) - 16:11, 28 February 2013
• Luisa's BRC task notes
  This is all I found. I only used Skyview for POSS; the rest comes from IRSA: BRC 34, ogura source 2, or what to do if you can't find a counterpart by searching in the 2mass catalog.
  4 KB (662 words) - 17:00, 24 June 2011
• Generating Light Curves - APT and Excel
  ...s IRAC notes [[File:IRAC notes.pdf]] The aperture and background settings we used were We also chose to have APT subtract the background using setting B subtracting
  8 KB (1,289 words) - 20:19, 12 October 2010
• C-CWEL Journal Club
  *what they did was ... (high level summary, no need to get into nitty gritty deta *what they did that I agree with is ...
  10 KB (1,745 words) - 23:54, 3 April 2013
• Variable Stars
  # Specifically, I think the ones we've been studying are considered cepheids, or variable stars with shorter pe You Rock Joey! So if we are looking fore these rapidly varying stars in this study, why might it be
  4 KB (667 words) - 03:52, 31 July 2010
• Lauren BRC 27
  I found one article, published in July of 2011, that is not on the list. The title ...de 'flanking fields' of serendipitous data, when these data are available, we will use the Spitzer data in addition to the WISE data, enabling a better d
  10 KB (1,573 words) - 14:29, 3 March 2012
• Creating RGB images with DS9
  ...ook the best it possibly can. If it looks good, it could look even better. What to do after you load an image: (Scale) There are numerous tools you can use '''What to do after you load an image: (Frame)'''
  4 KB (719 words) - 22:49, 8 January 2011
• Bob BRC 34
  ...was located in the sky. What constellation it was in? (Cepheus the King) What was the nearest bright star? (Alderamin & Deneb) From last year’s NITARP team proposal we have the following information on BRC 34.
  8 KB (1,346 words) - 21:45, 5 March 2012
• Chandra
  Who we are: What we do:
  4 KB (577 words) - 16:02, 16 March 2013
• Studying Young Stars
  ...? hint: not the asteroid belt. out farther than that -- see in the movie, we go out well past a "jupiter".) ...sed on the SED slope are dubbed Class I, II, and III. As we learned more, we created another class called "flat" between Class I and II. The very earli
  13 KB (2,128 words) - 22:21, 23 March 2023
• CG4 Bigger Picture and Goals
  ...s a little squishy, perhaps squishier than you might be comfortable with. What I describe here (and elsewhere on the wiki) is the kind of goal I would giv ...an abstract. BUT we already know enough to write our proposal abstract, so we could write a poster abstract right now.
  8 KB (1,362 words) - 03:34, 20 May 2010
• LLAMMa Bigger Picture and Goals
  ''Most succinct:''  We will be looking for new candidate young stars in Ceph C using X-rays, optic ...ied to date. Our goal is to find new candidate young stars in this region. We have data from:
  10 KB (1,779 words) - 20:19, 18 February 2016
• Getting your feet wet with catalogs and plots at IRSA Hints
  ...distance between your requested position and the position of the source it found in the catalog, and the position angle (in degrees east of north). It does ...inding Alpha Cen! Need to dig into literature to find someone else who has found the EDR3 counterpart to Alpha Cen. This is really turning out to be a MUCH
  8 KB (1,437 words) - 17:48, 5 October 2022
• Windows hints, tips, and tricks
  ...u will need to select the folder to extract to (same as the folder name is what I picked). We are assuming most MOPEX users are on a unix-based (unix, linux, mac) machin
  7 KB (1,206 words) - 20:58, 3 October 2011
• Resolution and YSOs
  We spend a lot of time in the study of YSOs talking about the rings of dust ar ...ou see in the little images here are not among those 10 close-by sources. What you are seeing here is the difference in resolution between IRAC and MIPS,
  6 KB (1,069 words) - 01:42, 28 July 2020
• Science background
  ...barked on a campaign to monitor some of the candidate TTauri stars that we found using Spitzer data. They used ground-based telescopes to see if the stars ...se things? In short, rings of carbon, like the grunge on your grill. But what else are they, and why are they important?
  2 KB (366 words) - 17:02, 16 November 2020

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