Search results

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
• Variability of the Mid-IR Sky Current Research Activities
  Dr. Rebull put together a list of people, places, things that we should check out at the AAS. Click on your name and document your time wit We will be arriving on Thursday Aug 5, departing Aug 9 in hopes of working the
  9 KB (1,429 words) - 06:27, 6 January 2012
• BRC Spring work
  We need to come up with a short list of papers to read in detail and discuss. We'll rotate through our short list of papers, and each of you will get one to ...cause the analysis we will do for our BRCs is very similar to the analysis we did for IC2118 or CG4.
  22 KB (3,737 words) - 19:10, 15 September 2011
• Luisa's AAS 2012 Scavenger Hunt
  ...­form and open-­ended, but THIS REALLY IS IMPORTANT TO US… we need to show we did not pay for you to come here just to party! <BR><BR> ...e time the meeting starts in earnest on Monday, you should have an idea of what kinds of science your team will be doing. '''FOLKS FINISHING PROJECTS:''' Y
  7 KB (1,284 words) - 07:24, 6 January 2012
• Guide to NITARP participants for use of the wiki
  *and (b) provide a place to save and share the materials we developed to teach each other and teach students. ...n recent years. But there is now a new need for sharing some of the things we have developed.
  9 KB (1,708 words) - 20:59, 29 July 2020
• C-WAYS: follow the bouncing target selection
  OK, so at the AAS we talked about LDN 1548 as a viable option. It had, we thought, good potential for yielding new young stars, it was (in projected ...ad enough that I went and checked the coordinates. More than once. This is what I see. There is not a lot here, and there is going to be a TON of contamina
  26 KB (4,644 words) - 16:18, 8 October 2012
• Finding cluster members
  ...difficult to pick out as a distinct ‘cluster’ of people, especially while we weren’t all physically co-located -- some of us were in line, getting sal ...cteristics of young stars as possible to determine cluster membership, and we will do the same.
  19 KB (3,216 words) - 23:02, 25 January 2024
• Target selection for brc27
  ...ric magnitudes of the disk bearing candidates in BRCs 2, 27 and 13/14 (are we interested in examining this?) ..., 9 February 2011 (PST)) OK, just for comparison, here is a walkthrough of what luisa would do, but for just one of the objects.
  14 KB (2,315 words) - 22:36, 16 February 2011
• C-WAYS Proposal
  As per the instructions for this year's proposal, we need to have: ~10 arcmin radius to look for objects. what other named objects are
  17 KB (2,838 words) - 18:10, 6 May 2012
• Taurus catalog
  ...fact covers such a large region that some of the apparently young stars we found may in fact be members of adjacent star-forming regions (Pleiades, Perseus, ...the objects have fluxes in all bands, so you will need to be careful about what you use. A value of -9 means no data available.
  4 KB (756 words) - 15:06, 11 May 2012
• Jackie BRC 38
  I need a picture in my head. I found these helpful. The first is the one Luisa already put up. The 2nd is from A H2 jets found (Saraceno et al. 1996; Nisini et al. 2001) <br>
  28 KB (4,538 words) - 23:20, 5 March 2012
• Working with the LLAMMa 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.
  40 KB (7,042 words) - 20:26, 27 July 2016
• SED plots introduction
  ...lly blackbodies but the emission from them is very similar to blackbodies. We can "fit" a blackbody curve to the star. Any emission from dust around the ...ge). This is one for blackbody spectra that some NITARP teachers' students found helpful. Most of these have lessons teachers uploaded. Those done by Kathy
  8 KB (1,406 words) - 17:05, 31 July 2020
• Measuring eclipsing binaries in the Kepler data set
  *What types of light curves come from what kind of binaries. *What properties can be determined from light curves.
  18 KB (2,905 words) - 18:00, 13 December 2011
• Measuring Resolutions (2023)
  ...going to be important for our work, let’s explore what spatial resolutions we have in our data. The first goal of this worksheet is to fill out the follo ...-187. Does it look different across the bands in Finder Chart? This is why we are thinking about these issues of spatial resolution.
  8 KB (1,366 words) - 15:51, 16 May 2023
• Working with the HG-WELS 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 ...': Understand which sources have been studied for these three samples, and what has been measured for them. -->
  31 KB (5,458 words) - 20:37, 28 August 2014
• C-CWEL Proposal
  ...paper for these BRCs (otherwise known as SFOs). Also, [[How can I find out what scientists already know about a particular astronomy topic or object?]] and 2/13 - Luisa will be in Boston, and I think Wendi too (we will be [http://www.gk12.org/meetings/ here]); you can have a telecon witho
  35 KB (5,742 words) - 23:27, 27 February 2013
• Identification of Previously Known Objects on Candidate List
  .... Some discussion was started in Spring 2011 on [[BRC Spring work]], where we summarized the literature. Starting the conversation, here is what I sent out Friday about BRC 27.
  46 KB (7,970 words) - 17:38, 16 September 2011
• C-WAYS Spring work
  ...he issues of spatial resolution. I have developed a worksheet for this. '''WE DECIDED TO DO THIS FIRST.''' ...g... ones you might read if you have time ... and ones you can ignore. '''WE SHOULD START ON THIS AFTER THE RESOLUTION STUFF.'''
  34 KB (5,550 words) - 04:03, 6 June 2012
• BRC Proposal
  ...explanation of Star Formation from a textbook. There's more math here than we'll need. [[File:SF.pdf]] STUFF HERE PERTAINS TO SPECIFIC TARGET SELECTION. why we should do one region versus another, why some regions should be dropped. hi
  21 KB (3,168 words) - 16:20, 26 May 2011
• OLD Guide to NITARP participants for use of the wiki
  *and (b) provide a place to save and share the materials we developed to teach each other and teach students. ...be geographically distant, may be a challenge! The only platform on which we have had broad success has been the wiki, because:
  12 KB (2,210 words) - 21:52, 27 July 2020
• C-WAYS 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.
  35 KB (6,201 words) - 21:11, 12 July 2012
• Using the SHA, long version
  ...osition it thinks you've entered, so you can check that it's doing exactly what you want it to do. This is what I see after a generic search for all M31 data:
  16 KB (2,838 words) - 16:11, 10 May 2012
• Working with the BRCs
  ...you comfortable enough to search for your own favorite target, understand what to do with the search results, and download data. ...lts when you search by position. How are they the same/different? Which do we want to download?
  33 KB (5,401 words) - 15:00, 23 September 2011
• Task answer notes from luisa
  ...a quiet few hours, and go through the wiki again with your notes. I knew we'd gone through a lot, very fast, but I also knew that you all had been doin WARNING -- in the process of doing this, i rediscovered the fact that we should not be using the big merged mosaic at MIPS for photometry, because R
  32 KB (4,902 words) - 08:02, 21 December 2010
• Aperture Photometry Overview
  ...the document entitled "Photometry Using IRAF" by Lisa A. Wells, from 1994, found on the [http://iraf.noao.edu/docs/photom.html IRAF photometry documentation #Determine background -- e.g. determine what the signal would be in the aperture if the star was not there. (Usually me
  15 KB (2,585 words) - 02:23, 31 July 2020
• PythonOnSHIPs
  ::* What happens when you add two string variables together? ::* What is the length of the array 'a' created by the following numpy command: a =
  5 KB (734 words) - 23:15, 25 June 2013
• All the NITARP videos in one place
  New for recruiting starting with the class of 2013, we have a [http://www.youtube.com/watch?v=EoJqyzCR2fc&feature=youtu.be 3-minut These were created to help all NITARP participants learn what the wiki is for and how to use it (for learning or contributing).
  8 KB (1,239 words) - 20:38, 16 April 2013
• Color-Magnitude and Color-Color plots Overview
  ''Note that the rest of this page assumes you know what [[Photometry|photometry and magnitudes]] are.'' ...rder to calculate the absolute magnitude from the apparent magnitude. But what if you don't know the distances to the clusters? Wouldn't it be nice to st
  9 KB (1,583 words) - 18:15, 23 June 2021
• Working with CG4+SA101
  ...you comfortable enough to search for your own favorite target, understand what to do with the search results, and download data. ...delivered products, if they exist for the region you want). In this case, we have some special circumstances: one of the observations was taken with clu
  16 KB (2,728 words) - 19:01, 23 November 2010
• How can I make a color composite image using Spitzer and/or other data?
  ..., preferably at least one of which is Spitzer data just because we are who we are here, but really any three bands will work. See [[How do I download da ...at the bottom of this page -- if you find more, please let us know so that we can link them in.
  15 KB (2,609 words) - 16:32, 1 March 2016
• Herschel Space Observatory
  ...tar formation has been gained by studies in our own Galaxy. With Herschel, we can carry out similar studies in relatively nearby galaxies as well. For ex ...t star and galaxy formation commenced relatively early after the Big Bang. We also know that when the Universe was about half its current age, star forma
  19 KB (3,099 words) - 21:16, 2 February 2013
• Photometry Scaffolding
  ...y be coming from the fact that, by eye, you can see the sources *there* so what is the issue, but the gap in understanding has to do with explaining that t ...fine for that. So the aperture photometry was totally good enough for what we were doing… except possibly for a few of the most crowded sources at the
  25 KB (4,424 words) - 03:25, 12 August 2020
• Working with the C-CWEL 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 And, we care about stuff within a ~20 arcmin radius of these positions. (which mean
  46 KB (8,082 words) - 17:21, 7 August 2013
• Working with the C-WAYS data
  And, we care about stuff within a ~20 arcmin radius of these positions. (which mean We have 3 regions we care about, so three places to search on the sky. We need to get the relevant data from both WISE and Spitzer.
  47 KB (8,224 words) - 19:56, 24 July 2012
• CG4 Proposal
  ...target(s) and why. background on subject and target. educated guesses on what you might find. * detailed information on what data are available, and what you plan to do with it (e.g. much more than "i'm sure spitzer observed this
  33 KB (5,123 words) - 17:24, 17 April 2013
• Summaries and questions on discussed papers
  * Today we know it is 100 million years old and 460 LY away. '''QUESTION:''' What is the best way to describe any differences for T Tauri stars and YSOs?
  42 KB (6,796 words) - 20:39, 18 May 2012
• LLAMMa Resolution Worksheet
  ...ns is a very important thing for us to consider in the course of our work. We're using data that come from several different surveys, with different spat ...elescopes, e.g., WISE vs. Spitzer vs. 2MASS resolution; and (2) understand what the challenges will be for us in matching across wavelengths. '''Ancillary
  30 KB (5,370 words) - 04:20, 30 March 2016
• IC 417 Resolution Worksheet
  ...n of WISE channel 1 and 2 with Spitzer GLIMPSE IRAC channel 1 and 2, which we can do in spades for IC417. ...elescopes, e.g., WISE vs. Spitzer vs. 2MASS resolution; and (2) understand what the challenges will be for us in matching across wavelengths. '''Ancillary
  30 KB (5,229 words) - 22:18, 30 March 2015
• CephC-LABS Resolution Worksheet
  ...ns is a very important thing for us to consider in the course of our work. We're using data that come from several different surveys, with different spat ...g., WISE vs. Spitzer vs. 2MASS vs. Herschel resolution; and (2) understand what the challenges will be for us in matching across wavelengths. '''Ancillary
  32 KB (5,692 words) - 16:18, 13 April 2017
• Target selection for brc31
  ...ed as OSP2002 and are the ONLY reference for many of the following objects found in the list: BRC 31 3, 4, 5, 7, 8, 19, 20, 22, 24, 25, 27, 28. ...d a large number (460) of Hα emission stars. A total of 12 new HH objects found. Most are of small apparent size, emphasizing the need for deep searches at
  13 KB (1,918 words) - 03:09, 16 February 2011
• BRC Optical Ground-Based Follow-Up
  ...determine that some of these objects are actually resolved galaxies. Once we add optical photometry to the SEDs, the shape of the SEDs may allow us to d ...we get the best quality data in the least amount of time possible. ("Ooops we screwed up" will not generally get you additional telescope time.)
  29 KB (3,823 words) - 19:30, 9 November 2011