Differences between revisions 1 and 16 (spanning 15 versions)
Revision 1 as of 2009-08-28 09:18:17
Size: 260
Editor: visitor7
Comment:
Revision 16 as of 2013-09-10 09:04:27
Size: 3388
Editor: lt-ck
Comment:
Deletions are marked like this. Additions are marked like this.
Line 1: Line 1:
<<TableOfContents(4)>>
Line 3: Line 5:
[[http://www.iram.es/IRAMES/dataarchive/linecal/init.html|Mauersberger et al. 1989]], [[https://gra-lx1.iram.es/mainWiki/CalibratorsAbcd|Line calibrators observed with the ABCD and EMIR receivers in 2009]] Observers should regularly check the line calibration by observing strong, known line calibrators. A simple
onoff, with the off position at e.g. 5arcmin distance from the source, will allow detecting any grave problems,
like tuning to the wrong harmonic, wrong pointing model, spectrometer not working, etc.. Observations can
be compared with standard spectra shown in the Mauersberger catalogue or with more recent data (see below).

The observers should use Xephem to select suitable line calibrators. Xephem reads from the catalogue lines-J2000.sou (see below) which is available on all project directories.

For a detailed check of the intensity and velocity calibration, the observing procedures and off positions used by Mauersberger et al. should be selected.

Observing projects using non-standard frequencies (in frequency surveys or for high-z observations e.g.) may take a look at the line surveys
of standard sources listed in the literature (see belowl).

 * IRAM line calibrator catalog: [[attachment:lines-J2000.sou|lines-J2000.sou]] (v1.0.9 2007-10-18)
 * [[http://www.iram.es/IRAMES/dataarchive/linecal/init.html|Mauersberger et al. 1989]] (paper and 30m data file)
 * [[https://gra-lx1.iram.es/mainWiki/CalibratorsAbcd|Line calibrators observed with the ABCD and EMIR receivers in 2009]] (see bottom of this page)
 * JCMT line calibrators [[http://www.jach.hawaii.edu/JCMT/spectral_line/Standards/standards.html|standard spectra]] (A2: 200-280GHz, B-Band: around 345GHz)
 * APEX line calibrators [[http://www.apex-telescope.org/heterodyne/shfi/het230/calibration/intensity/|standard spectra at 230]]

== Online databases ==

 * [[http://www.astro.uni-koeln.de/cgi-bin/cdmssearch|Cologne Data base]]
 * [[http://physics.nist.gov/cgi-bin/micro/table5/start.pl|Lovas list]]
 * [[http://spec.jpl.nasa.gov/ftp/pub/catalog/catform.html|JPL data base]]

== Line surveys ==

=== 3mm ===

 * IRC+10216 (30m, Cernicharo, Guelin et al. 1995): FreqSurvey3mm10216 (local)
 * !SgrB2 (Turner et al. 1989, ApJL, 70, 539)
 * !SgrB2 (NRAO12m & BIMA, Friedel et al. 2004, ApJ, 600, 234)
 * NGC7027 (ARO12m, HHT, Zhang et al. 2008, ApJ, 678, 328)

=== 2mm ===
 * IRC+10216 (30m, Cernicharo, Guelin et al. 1995): FreqSurvey2mm10216 (local)
 * NGC253 (30m, Martin et al., 2006, ApJ, 164, 450)
 * NGC7027 (ARO12m, HHT, Zhang et al. 2008, ApJ, 678, 328)
 * XX (NRAO12m, [[http://www.cv.nrao.edu/Turner2mmLineSurvey/|Turner et al.]])

=== 1mm ===

 * W3OH (30m, Biver): [[attachment:biver-jul2013-1mm-survey-w3oh.pdf]]
 * XXX (xx, Avery et al. 1992, ApJS, 83, 363)
 * NGC7027 (ARO12m, HHT, Zhang et al. 2008, ApJ, 678, 328)
 * Orion A (OVRO, 247-263GHz, Blake et al. 1986, ApJS, 60, 357)
 * Orion Bar (APEX, selected frequency ranges, [[http://esoads.eso.org/abs/2006A%26A...454L..47L|Leurini et al. 2006]])

=== 0.8mm ===

 * IRC+10216 (JCMT, Avery et al. 1992, ApJS, 83, 363)
 * Orion KL (xxx, 325-360GHz, [[http://esoads.eso.org/abs/1997ApJS..108..301S|Schilke et al. 1997]])
 * XXX (JCMT, 332-373GHz, [[http://esoads.eso.org/abs/2007PASP..119..102P|Plume et al. 2007]])

this page is maintained by CK


[[http://www.iram.es/IRAMES/mainWiki/ScienceSupportGroup|go back to Science Support Group Home Page]]

'''To do''':

 * update source catalogue

Line Calibration at the IRAM 30m telescope

Observers should regularly check the line calibration by observing strong, known line calibrators. A simple onoff, with the off position at e.g. 5arcmin distance from the source, will allow detecting any grave problems, like tuning to the wrong harmonic, wrong pointing model, spectrometer not working, etc.. Observations can be compared with standard spectra shown in the Mauersberger catalogue or with more recent data (see below).

The observers should use Xephem to select suitable line calibrators. Xephem reads from the catalogue lines-J2000.sou (see below) which is available on all project directories.

For a detailed check of the intensity and velocity calibration, the observing procedures and off positions used by Mauersberger et al. should be selected.

Observing projects using non-standard frequencies (in frequency surveys or for high-z observations e.g.) may take a look at the line surveys of standard sources listed in the literature (see belowl).

Online databases

Line surveys

3mm

  • IRC+10216 (30m, Cernicharo, Guelin et al. 1995): FreqSurvey3mm10216 (local)

  • SgrB2 (Turner et al. 1989, ApJL, 70, 539)

  • SgrB2 (NRAO12m & BIMA, Friedel et al. 2004, ApJ, 600, 234)

  • NGC7027 (ARO12m, HHT, Zhang et al. 2008, ApJ, 678, 328)

2mm

  • IRC+10216 (30m, Cernicharo, Guelin et al. 1995): FreqSurvey2mm10216 (local)

  • NGC253 (30m, Martin et al., 2006, ApJ, 164, 450)
  • NGC7027 (ARO12m, HHT, Zhang et al. 2008, ApJ, 678, 328)
  • XX (NRAO12m, Turner et al.)

1mm

  • W3OH (30m, Biver): biver-jul2013-1mm-survey-w3oh.pdf

  • XXX (xx, Avery et al. 1992, ApJS, 83, 363)
  • NGC7027 (ARO12m, HHT, Zhang et al. 2008, ApJ, 678, 328)
  • Orion A (OVRO, 247-263GHz, Blake et al. 1986, ApJS, 60, 357)
  • Orion Bar (APEX, selected frequency ranges, Leurini et al. 2006)

0.8mm

this page is maintained by CK

go back to Science Support Group Home Page

To do:

  • update source catalogue

LineCalibration (last edited 2013-10-11 07:35:22 by lt-ck)