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• Coherent ideas of what to do with these pieces
  People want *anything* having to do with black holes. AGN light curves?
  7 KB (1,074 words) - 16:32, 6 October 2022
• SED plots introduction
  ...es (often with downward-pointing arrows to denote upper limits), the solid black line are the IRS ''spectroscopic'' points (error most apparent near the red
  8 KB (1,406 words) - 17:05, 31 July 2020
• Working with the LLAMMa data
  ...rcles = mean (average) IRAC from YSOVAR light curves. Black stars = WISE. Black box (near the IRAC points) = MIPS. longer wavelength SEDs continue: asteris
  40 KB (7,042 words) - 20:26, 27 July 2016
• Lynds Target Selection
  ...per (see sections 4.2 and 4.3) about whether some objects found in the LDN black parts are real YSOs or not, and they conclude based on available evidence t black parts are real YSOs or not, and they conclude based on available evidence t
  30 KB (5,075 words) - 14:04, 2 May 2008
• Working with the IC 417 data
  ...means that bright is ok). Black diamonds = 2MASS. Green squares = UKIDSS. black stars = WISE. blue circles = IRAC.
  38 KB (6,763 words) - 01:50, 18 June 2015
• How do I download data from WISE?
  ...t image window. At the top right of the image window, you can click on the black arrows to expand that image to fill your full screen, or click on the tools
  11 KB (2,080 words) - 03:38, 25 January 2013
• Studying Young Stars
  ...The x-axis is wavelength, and the y-axis is energy. It looks like a cold black body; all of the emission comes from the dust and gas in the cloud. The mas
  13 KB (2,128 words) - 22:21, 23 March 2023
• Aperture Photometry Overview
  ...agine the difference between finding bright single point sources on a flat black background, versus trying to find a wide variety of point source brightness
  15 KB (2,585 words) - 02:23, 31 July 2020
• Working with the C-WAYS data
  ...e Spitzer sources that are possible, or not? Why?) Why is there a patch of black in BRC 38 (hint: Beltran et al.)? ...y see. at "12:00", i really don't see any sources (or many sources) in the black in between sources. it's even doing a pretty good job finding sources on to
  47 KB (8,224 words) - 19:56, 24 July 2012
• C-WAYS Proposal
  ...ts to; star formation mechanism and stellar life cycle, spectral analysis, black body curves, and photometry. In the fall of 2012, the weekly meetings will
  17 KB (2,838 words) - 18:10, 6 May 2012
• Herschel Space Observatory
  ...ow in the mid infrared and we’re brightest at about 10 microns wavelength (black line in the graph). These days we are all familiar with infrared imaging,
  19 KB (3,099 words) - 21:16, 2 February 2013
• Identification of Previously Known Objects on Candidate List
  ...ture papers, plus ours, in BRC 27. Ogura 8 additionally indicated by large black star, since source density is high right there. [[file:brc27lit.png]] ...nates from Shevchenko, and the positions precessed to 2000 coordinates (in black). Look how big that shift is.
  46 KB (7,970 words) - 17:38, 16 September 2011
• PP Proposal
  ...FERMI, SWIFT, and XMM-Newton. Because of their work, there were part of a black hole special aired by National Geographic and NOVA.
  20 KB (3,148 words) - 02:08, 12 June 2011
• CephC-LABS Resolution Worksheet
  ...asonable amount of sky at all, you'll get a tiny 2MASS image surrounded by black, blank sky. In order to get big 2MASS images, you need to get them some oth
  32 KB (5,692 words) - 16:18, 13 April 2017
• L1688 Resolution Worksheet
  ...asonable amount of sky at all, you'll get a tiny 2MASS image surrounded by black, blank sky. In order to get big 2MASS images, you need to get them some oth
  35 KB (6,288 words) - 15:39, 11 April 2018
• C-CWEL Proposal
  ...396 complex. brc 38 is at the top of the 'ring', one of the less prominent black fingers at the top.
  35 KB (5,742 words) - 23:27, 27 February 2013
• Working with the C-CWEL data
  ...talog? Why are the Spitzer sources where they are? Why is there a patch of black in the center of the plot on the left (hint: Beltran et al.)?
  46 KB (8,082 words) - 17:21, 7 August 2013

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