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The Goddard-IRAM Superconducting 2mm Observer (GISMO) is a bolometer camera for the IRAM 30m telescope. It has been build by Goddard Space Flight Center, in Greenbelt, Maryland under the lead of Johannes Staguhn. GISMO consists of '''8x16 pixels''' with super conducting transition edge sensors (TES). The TES are read out by time domain SQUID multiplexers built at the National Institute for Standards (NIST), in Boulder, Colorado. . The nominal bandwidth is 140-162GHz (FWHM), pixels are spaced by '''13.75"''', the telescope HPBW is '''16.7"'''. The sensitivity is '''16 mJy sqrt(sec)'''. In the standard observing mode, data are taken while the telescope follows Lissajous curves without switching the secondary. An automated pipeline merges the GISMO data with the telescope data streams to create FITS files which are automatically processed by the reduction software crush to create logs, pointing results, and a first quick view of the data. The Goddard-IRAM Superconducting 2mm Observer (GISMO) is a bolometer camera for the IRAM 30m telescope. It has been build by Goddard Space Flight Center, in Greenbelt, Maryland under the lead of Johannes Staguhn. GISMO consists of '''8x16 pixels''' with super conducting transition edge sensors (TES). The TES are read out by time domain SQUID multiplexers built at the National Institute for Standards (NIST), in Boulder, Colorado. . The nominal bandwidth is 140-162GHz (FWHM), pixels are spaced by '''13.75"''', the telescope HPBW is '''16.7"'''. The sensitivity is '''16 mJy sqrt(sec)''' per beam. The field-of-view is 1.8'x3.7'. In the standard observing mode, data are taken while the telescope follows Lissajous curves without switching the secondary. An automated pipeline merges the GISMO data with the telescope data streams to create FITS files which are automatically processed by the reduction software crush to create logs, pointing results, and a first quick view of the data.
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== Documentation ==
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=== Observations ===
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== People == During the first open observing run in April 2012, observations will be carried out as pooled observations from a dedicated pool account gismow11. M.Gonzalez will provide login information. Progress of observations can be followed via the [[https://herapool.iram.es|pool data base]].
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 * 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 (crush)
 * IRAM/Granada: Guillermo Quintana-Lacaci (bolometer pool manager, <quintana@iram.es>), Nicolas Billot (<billot@iram.es>), Carsten Kramer (station manager, <kramer@iram.es>)		  * GismoHowToObserve (restricted access) <<BR>>
   This page presents pako scripts to be used for observations. They are currently being prepared by J.Abreu and H.Ungerechts.
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== Documentation for the first open call for 30m proposals (September 2011) == === Call for proposals ===
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 * [[http://www.iram-institute.org/EN/content-page-169-7-57-169-0-0.html|Call for proposals]]. The deadline to submit proposals for the winter semester 2011/12 is 22-September-2011.
 * [[attachment:GISMO_TimeEstimator.pdf|Time estimator.]] This document contains guidelines for astronomers to compute observing time estimates for the call for proposals of the Winter 2011 semester.		 In September 2011, GISMO had for the 1st time been offered to the community. Two weeks of dedicated GISMO observations are now planned for April 2012. GISMO will be available again for the summer semester 2012.

 * [[http://www.iram-institute.org/EN/content-page-169-7-57-169-0-0.html|Call for proposals]].
 * [[attachment:GISMO_TimeEstimator.pdf|Time estimator.]] This document contains guidelines for astronomers to compute observing time estimates.
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== Publications == === Publications ===
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== 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 (crush)
 * IRAM/Granada: Carsten Kramer (station manager, <kramer@iram.es>), Nicolas Billot (30m scheduler, <billot@iram.es>)
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=== Draft on how to observe ===
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 * GismoHowToObserve (restricted access) <<BR>>
   This page presents pako commands for the various types of observations. Revised pako commands are in preparation. The page will be made publicly available in time before the next observing run.		 === Test runs 2007-2012 ===
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=== Test runs 2007-2011 === ==== 1st observing run, April 2012 ====

[[GismoObsRun1|Go to the April 2012 page]]

==== 5th alignment run, March 2012 ====

[[GismoRun5|Go to the 5th run Wiki page]] (installation of GISMO at a permanent position with new optics, baffle and new filter)

GISMO

This page is maintained by CK, SL, and the GISMO team

Contents

  1. GISMO
    1. Overview
    2. Documentation
      1. Observations
      2. Call for proposals
      3. Publications
    3. People
    4. Internal pages
      1. Planned changes
      2. Test runs 2007-2012
        1. 1st observing run, April 2012
        2. 5th alignment run, March 2012
        3. 4th test run, April 2011
        4. 3rd test run, April 2010
        5. 2nd test run, October 2008
        6. 1st test run, November 2007

Overview

The Goddard-IRAM Superconducting 2mm Observer (GISMO) is a bolometer camera for the IRAM 30m telescope. It has been build by Goddard Space Flight Center, in Greenbelt, Maryland under the lead of Johannes Staguhn. GISMO consists of 8x16 pixels with super conducting transition edge sensors (TES). The TES are read out by time domain SQUID multiplexers built at the National Institute for Standards (NIST), in Boulder, Colorado. . The nominal bandwidth is 140-162GHz (FWHM), pixels are spaced by 13.75", the telescope HPBW is 16.7". The sensitivity is 16 mJy sqrt(sec) per beam. The field-of-view is 1.8'x3.7'. In the standard observing mode, data are taken while the telescope follows Lissajous curves without switching the secondary. An automated pipeline merges the GISMO data with the telescope data streams to create FITS files which are automatically processed by the reduction software crush to create logs, pointing results, and a first quick view of the data.

The 2mm spectral range provides a unique terrestrial window enabling ground-based observations of the earliest active dusty galaxies in the universe and thereby allowing a better constraint on the star formation rate in these objects.

Documentation

Observations

During the first open observing run in April 2012, observations will be carried out as pooled observations from a dedicated pool account gismow11. M.Gonzalez will provide login information. Progress of observations can be followed via the pool data base.

  • GismoHowToObserve (restricted access)

    • This page presents pako scripts to be used for observations. They are currently being prepared by J.Abreu and H.Ungerechts.

Call for proposals

In September 2011, GISMO had for the 1st time been offered to the community. Two weeks of dedicated GISMO observations are now planned for April 2012. GISMO will be available again for the summer semester 2012.

Publications

  1. Dwek, Staguhn et al. 2011 ApJ,
    Star and dust formation activities in AzTEC-3: A starburst galaxy at z = 5.3

  2. Arendt et al. 2011 ApJ,
    The Radio - 2 mm Spectral Index of the Crab Nebula Measured with GISMO

  3. Capack et al. 2011 Nature,
    A massive proto-cluster of galaxies at a redshift of z~5.3

  4. Dicker et al. 2009 ApJ,
    90GHz and 150GHz observations of the Orion M42 region. A sub-millimeter to radio analysis

  5. Benford, Moseley, Zmuidzinas 2009 Journal of Physics
    Direct detectors for the Einstein inflation probe

  6. IRAM Newsletter 2/2009
    GISMO - The Goddard-IRAM Superconducting 2 Millimeter Observer tested at the IRAM 30m observatory

  7. 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

People

Internal pages

Planned changes

  • GismoToDoList (restricted access)

    • This important page discusses between Goddard and IRAM the required changes to prepare for the run in spring 2012

Test runs 2007-2012

1st observing run, April 2012

Go to the April 2012 page

5th alignment run, March 2012

Go to the 5th run Wiki page (installation of GISMO at a permanent position with new optics, baffle and new filter)

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

Go to the 3rd run Wiki page

2nd test run, October 2008

Go to the 2nd run Wiki page

1st test run, November 2007

Go to the 1st run Wiki page

GoddardIramSuperconductingTwoMillimeterCamera (last edited 2014-03-31 13:30:45 by gra-lx17)