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Create the page "What We Found" on this wiki! See also the search results found.

• Matt Piper
  ...we don't know about the very beginning of a star's life. We want to know what causes the gasses from the BRC to collapse and form proto-stars, whether th =What I've Done So Far=
  1 KB (225 words) - 21:08, 19 June 2012
• LWN Pipettes Poster AAS 2012
  ...lping us create the most memorable scientific experience we have ever had. We could not have made the trip without you. ...e basics of using Fourier analysis to create light curves. The light curve we presented was that of asteroid 2000 SO1. <BR>
  3 KB (461 words) - 18:24, 27 January 2012
• 2011 and earlier wiki team work
  ...population that might be found there. Much of the background information found below for the IC 2118, Lynds, and CG4 teams also applies to this team as we ...population that might be found there. Much of the background information found above for the IC 2118 and Lynds teams also applies to this team as well.
  5 KB (772 words) - 17:09, 17 April 2013
• BRC Current Research Activities
  This page will be used to assemble the pieces for the proposal we are writing. ...[file: NITARPpreview.docx]] of things to look at before going to SSC … but we will go through all of this in more detail. Links to corresponding wiki pag
  2 KB (264 words) - 23:18, 14 September 2011
• BRC Bigger Picture and Goals
  ...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 ...are and contrast" kind of discussion even within our own results. Ideally, we will also extend this discussion to the rest of the literature.
  4 KB (711 words) - 03:00, 19 May 2011
• HR4AGN Current Research Activities
  This page will be used to assemble the pieces for the proposal we are writing. See [[2012 proposal instructions]] for, well, instructions! Notes from our weekly conference calls can be found here.
  656 bytes (99 words) - 17:22, 22 January 2013
• CG4 Winter Mini-Workshop
  ...p-up workshop in which we (primarily the students) compare notes about how we accomplished tasks. If we have a few minutes of questions, then this should take about an hour to 90
  2 KB (347 words) - 16:14, 7 March 2011
• C-CWEL Current Research Activities
  This page will be used to assemble the pieces for the proposal we are writing. [[2013 proposal instructions]] Several of the things we will be doing are similar, and several will be different.
  2 KB (294 words) - 17:05, 13 January 2014
• Monitoring young stars
  ...barked on a campaign to monitor some of the candidate TTauri stars that we found using Spitzer data. They are using ground-based telescopes to see if the st ==What is time series analysis?==
  5 KB (823 words) - 19:03, 13 May 2011
• C-WAYS Bigger Picture and Goals
  We have WISE data for 3 patches of sky likely to harbor young stars: BRC 27, B ...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
  5 KB (824 words) - 23:33, 26 March 2012
• C-WAYS Current Research Activities
  This page will be used to assemble the pieces for the proposal we are writing. [[2012 proposal instructions]] Several of the things we will be doing are similar, and several will be different.
  2 KB (299 words) - 17:30, 12 July 2012
• CM4Seyferts Current Research Activities
  This page will be used to assemble the pieces for the proposal we are writing. See [[2012 proposal instructions]] for, well, instructions! Notes from our weekly conference calls can be found here.
  829 bytes (118 words) - 18:35, 24 April 2013
• HG-WELS Current Research Activities
  This page will be used to assemble the pieces for the proposal we are writing. [[2014 proposal instructions]] Several of the things we will be doing are similar, and several will be different.
  2 KB (291 words) - 15:37, 6 August 2014
• Stars and How They Form - videos with sign language
  We are Anna McCartney and Lyssa Matsche. We are from the Wisconsin School for the Deaf. We created an ASL video with captions, but no audio, to explain the simulation
  3 KB (481 words) - 22:59, 8 January 2011
• LLAMMa Current Research Activities
  '''WE ARE WORKING ON A FIELD CENTERED ON 23:05:51 +62:30:55''' and probably 10-15 '''WE ARE WORKING ON A FIELD CENTERED ON 23:05:51 +62:30:55''' and probably 10-15
  3 KB (371 words) - 22:35, 12 April 2016
• CephC-LABS Current Research Activities
  '''WE ARE WORKING ON A FIELD CENTERED ON 23:05:51 +62:30:55''' and probably 10-15 '''WE ARE WORKING ON A FIELD CENTERED ON 23:05:51 +62:30:55''' and probably 10-15
  3 KB (391 words) - 16:11, 3 March 2017
• IC 417 Current Research Activities
  Several of the things we will be doing are similar, and several will be different. We talked about traveling June 14, working June 15-18, traveling June 19.
  2 KB (280 words) - 20:15, 3 June 2015
• C-WAYS Useful Links
  ...explanation of Star Formation from a textbook. There's more math here than we'll need. [[File:SF.pdf]] ...! We picked LDN 1548, but if we somehow blow through that one really fast, we can pick another one to do as well.
  3 KB (481 words) - 23:26, 26 January 2012
• Finding the diameter of a region we care about
  So, no matter how we do it exactly, it’s always about 16-18 arcmin. Now, we have a long, thin triangle:
  2 KB (370 words) - 19:33, 31 July 2020
• Instructions for source matching
  ...le 2MASS All-Sky Release Database. The query page that comes up is the one we will be using over and over. ...just use the arrow button on the cell label for column B and choose sort. We only care about the sources that are marked with * in Gregorio. The others
  4 KB (808 words) - 03:55, 1 June 2012
• 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
• How does the Spitzer Telescope work?
  ...nm). Any warm object in space radiates IR energy (infrared energy, which we sense as heat). In fact, "warm" really means any object above absolute zer ...polycyclic aromatic hydrocarbon). PAHs are one of the important molecules found in the interstellar medium (ISM). For more information, check out [[Studyi
  7 KB (1,089 words) - 18:48, 13 May 2011
• C-CWEL Source Matching Work
  ...ge to those of us used to seeing images of these landforms from space, but we have a whole lot more information now than they did then. ...stern explorers were able to attempt to map was the coasts, because that's what they had the most information about...and the most immediate need to know.
  21 KB (3,726 words) - 19:44, 7 March 2013
• HG-WELS Spring work
  ...er *exporting* the file as a plain text file, but you can do that too. And we will. In coming weeks, we will need to be familiar with angles on the sky, so please review [http://l
  9 KB (1,721 words) - 05:00, 18 March 2014
• How science works and other philosophical musings
  *[https://www.youtube.com/watch?v=kIbWKlAgHPM Movie (16:01) on What is Science] by Dr. Luisa Rebull (2016) ...t answers. Real science has a lot of dead ends as we struggle to find out what the ‘right answer’ is.
  3 KB (476 words) - 17:21, 26 October 2020
• What is an archive and why do we need archives?
  ...y developed in 2018 by L. M. Rebull for [https://open.nasa.gov/blog/why-do-we-archive-astronomy-data/ NASA Open Data website]'' ...are also in the [https://www.listentospacepod.com/episodes/2017/2/5/83-why-we-archive-with-dr-rebull?rq=rebull February 05, 2017 episode of the Spacepod
  7 KB (1,208 words) - 22:15, 29 July 2020
• Cold Spotz Current Research Activities
  This page will be used to assemble the pieces for the proposal we are writing. See [[2012 proposal instructions]] for, well, instructions! The paper parts for a Planck model can be found at [http://planck.cf.ac.uk/education/model]. Kat's model (the one furthest
  2 KB (411 words) - 01:12, 25 September 2012
• More information on Spitzer operations
  ...rity over all others, that spacecraft gets whatever antennas it needs, and we have to rearrange our uplink/downlink times accordingly. This operational constraint is why we can't drop everything and make an observation of whatever you want ''right
  10 KB (1,754 words) - 19:09, 13 May 2011
• Working with the IC 417 data
  ...presented as a linear progression because of the nature of this page, but we have already done some things "out of order", and moreover, chances are exc ...or even necessarily at all. But it will give you a deeper understanding of what is going on.
  38 KB (6,763 words) - 01:50, 18 June 2015
• SSW2022 Activities
  ...nts from earlier in the week can be done using IRSA tools, so this is what we have reproduced here. See the SSW website for recordings of the talks that ##What are some things that are the same and different between these two plots? Wh
  11 KB (1,991 words) - 16:42, 6 October 2022
• Studying AGN
  ...urnell discovered neutron stars that, at the time, were the densest matter found through observations. *1970 -- Cygnus X - 1 The first good black hole candidate that astronomers found. It emits x-rays and has a companion smaller than Earth but with a mass gre
  10 KB (1,833 words) - 16:06, 17 February 2014

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