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#acl GismoTeam:read,write,delete Default = GISMO (Goddard-IRAM Superconducting 2 Millimeter Observer): a Transition Edge Sensors bolometer camera for the IRAM 30m telescope = |
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'''GISMO - The Goddard-IRAM Superconducting 2 Millimeter Observer''' | This page is maintained by CK, SL, and the GISMO team |
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In November 2007, this 8x16 BUG bolometer camera was tested at the 30m telescope. Bandwidth 125-175GHz, 17" beam, 14" pixel offsets. A second test run is currently running (Oct 08). PI is [http://www.astro.umd.edu/people/staguhn.html Johannes Staguhn] [http://gsfctechnology.gsfc.nasa.gov/Detector.htm (Goddard)], [http://www.phys.ufl.edu/tes3/pdfs/Benford_TES_Bolometer_Arrays_Poster.pdf Poster on TES Bolometers] | <<Anchor(beginOfPage)>> |
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* attachment:SPIE_GISMO_Staguhn.pdf * attachment:Staguhn_GISMO_SPIE_08_Rev1.pdf |
<<TableOfContents(5)>> ---- == People == * Overall coordinator: '''Samuel Leclercq''' <leclercq@iram.fr> (IRAM/Grenoble) * GISMO team: Johannes Staguhn <johannes.g.staguhn@nasa.gov> (PI), Elmer Sharp, Steve Maher, Dominic Benford, Dale Fixen, Attila Kovacs * Main contact IRAM/Granada: Carsten Kramer (station manager) == Publications == 1. [[http://arxiv.org/abs/1106.2092|Dwek, Staguhn et al. 2011]] ApJ, '''Star and dust formation activities in AzTEC-3: A starburst galaxy at z = 5.3''' 1. [[http://arxiv.org/abs/1103.6225|Arendt et al. 2011]] ApJ, '''The Radio - 2 mm Spectral Index of the Crab Nebula Measured with GISMO''' 1. [[http://arxiv.org/abs/1101.3586|Capack et al. 2011]] Nature, '''A massive proto-cluster of galaxies at a redshift of z~5.3''' 1. [[http://arxiv.org/abs/0907.1300|Dicker et al. 2009]] ApJ, '''90GHz and 150GHz observations of the Orion M42 region. A sub-millimeter to radio analysis''' 1. [[http://iopscience.iop.org/1742-6596/155/1/012001/pdf/jpconf9_155_012001.pdf||Benford, Moseley, Zmuidzinas]] Journal of Physics '''Direct detectors''' 1. [[http://esoads.eso.org/abs/2008JLTP..151..709S|Staguhn et al. 2008]] Journal of Low Temperature Physics, 151, 3, 709 '''GISMO, a 2 mm Bolometer Camera Optimized for the Study of High Redshift Galaxies''' Other news: 1. [[http://www.iram.fr/IRAMFR/ARN/feb09/node12.html|IRAM Newsletter 2/2009]] 1. see also Samuel's list: [[http://www.iram.fr/~leclercq/GISMO/GismoPage.html|here]] == Things to do for 1st open run == * ToDoList (restricted access) == HOWTO == * HowToObserve (restricted access) ---- == 4th test run, April 2011 == [[GismoRun4|Go to the 4th run Wiki page]] (restricted access, please send an email to SL to obtain the login information) == 3rd test run, April 2010 == [[GismoRun3|Go to the 3rd run Wiki page]] == 2nd test run, October 2008 == [[GismoRun2|Go to the 2nd run Wiki page]] == 1st test run, November 2007 == [[GismoRun1|Go to the 1st run Wiki page]] |
GISMO (Goddard-IRAM Superconducting 2 Millimeter Observer): a Transition Edge Sensors bolometer camera for the IRAM 30m telescope
This page is maintained by CK, SL, and the GISMO team
Contents
People
Overall coordinator: Samuel Leclercq <leclercq@iram.fr> (IRAM/Grenoble)
GISMO team: Johannes Staguhn <johannes.g.staguhn@nasa.gov> (PI), Elmer Sharp, Steve Maher, Dominic Benford, Dale Fixen, Attila Kovacs
- Main contact IRAM/Granada: Carsten Kramer (station manager)
Publications
Dwek, Staguhn et al. 2011 ApJ, Star and dust formation activities in AzTEC-3: A starburst galaxy at z = 5.3
Arendt et al. 2011 ApJ, The Radio - 2 mm Spectral Index of the Crab Nebula Measured with GISMO
Capack et al. 2011 Nature, A massive proto-cluster of galaxies at a redshift of z~5.3
Dicker et al. 2009 ApJ, 90GHz and 150GHz observations of the Orion M42 region. A sub-millimeter to radio analysis
http://iopscience.iop.org/1742-6596/155/1/012001/pdf/jpconf9_155_012001.pdf Journal of Physics Direct detectors
Staguhn et al. 2008 Journal of Low Temperature Physics, 151, 3, 709 GISMO, a 2 mm Bolometer Camera Optimized for the Study of High Redshift Galaxies
Other news:
see also Samuel's list: here
Things to do for 1st open run
ToDoList (restricted access)
HOWTO
HowToObserve (restricted access)
4th test run, April 2011
Go to the 4th run Wiki page (restricted access, please send an email to SL to obtain the login information)
3rd test run, April 2010
2nd test run, October 2008