TWiki> Public Web>PacsCalibrationWeb (revision 43)EditAttach

PACS instrument and calibration web pages

Introduction

This page provides up-to-date information about using the PACS instrument: from preparing observations to reducing your data. This page also provides you with the latest calibration accuracies and known PACS calibration issues.

Observing with PACS

  • AOT Release Notes: dedicated release notes per AOT (the astronomer's observing template, i.e. planning your observing time). These contain information about how the standard observing blocks work, transmission functions, sensitivity, etc.

Reducing PACS data

  • HIPE (Herschel Interactive Processing Environment): The latest User Release HCSS version that you should use for reducing PACS data is HIPE v7.0.0. It can be downloaded from: http://herschel.esac.esa.int/HIPE_download.shtml. FYI: this corresponds to the so-called CIB (continuous integration build) HIPE 7.0 build 1931.

  • We also provide access to the latest stable developer build (a.k.a latest stable CIB), used by the instrument experts at the ICC.
    Beware
    These developer builds do not undergo the same in-depth testing as the user releases do. The current latest stable developer build is identical to the latest User Release (HIPE 7.0 build 1931).

  • Within HIPE you can access all the PACS data reduction and HIPE-use documentation. For those who wish to read the PACS Data Reduction Guide (PDRG) in PDF form, we provide that here: PDRG version 7. This version can be used with HIPE v7.0.0 as well as all track 7 and track 8 of the CIBs. (Note that within the PDF version, document links will not work.) The PDRG follows the pipeline scripts (see "Cookbooks" below) and also explains what you are doing as you pipeline process.

  • The very latest version of the PACS Pipeline Reference manual, which can also be used with HIPE track 7 and 8, is also provided in PDF format here: PPR version 5 (Jun 2011). (Note that with PDFs, document links will not work.) The PPR includes the more advanced topics of reducing PACS data, things you will want to know after you have become familiar with the PACS pipelines, and also explains more about how PACS data products are organised and how they can be inspected.

Cookbooks

  • Our version of cookbooks are the pipeline scripts, because (i) we recommend you rereduce your data in any case and (ii) these scripts are heavily commented to guide you through the data reduction process. These data reduction scripts are available in HIPE under the menu: Pipeline --> PACS --> Photometer/Spectrometer

PACS calibration file versions

  • When starting HIPE, you will be informed if new calibration files are available. Clicking on 'show details' will show you the release note of the new calibration set, with details about the changes. This is all also explained in the PDRG (chap 3: spectroscopy; chap 5: photometry)

PACS calibration and performance

Photometer calibration in scan maps.

  • Point Spread Function: PACS Photometer Point Spread function (5.5 M), version 1.01, 3 November 2010. A detailed document of the in-flight observed PSF. The accompanying tarball can be found here (31 Mb).

  • Herschel/PACS modelled point spread functions (3.1 Mb) is a related document presenting Zemax modelled point spread functions for both an `ideal' and an 'as built' Herschel telescope model. Tarballs with corresponding broad-band and monochromatic PSFs for these two cases are at http://pacs.ster.kuleuven.ac.be/pubtool/PSF. These are useful in addition to the observed PSFs but cannot replace them, since the models do not capture all effects found in the observed PSFs.

  • Point-source photometry: PACS uses 5 stars as primary calibrators with fluxes ranging from 0.6 to 15 Jy, plus fainter stars and asteroids as secondary calibrators. A new responsivity calibration (version) is deployed on the HCSS 7 track (this is explained in the internal report PICC-ME-TN-033 v1.01, where the associated encircled energy fraction [EEF] is given). This improves the accuracy of photometry to 3% in the blue channel and 5% in the red channel. The new calibration is described in detail in the technical note "PACS photometer point-source flux calibration (3.1 Mb) (PICC-ME-TN-037), version 1.0, 12 April 2011.

  • Point-source observations:
    • We refer to: PACS Photometer: chop/nod point-source & mini-scan map AOT release note: (2 Mb) version 2.0, 12 November 2010. We recommend you use the mini scan-map technique in all science cases related to point-sources, compact sources and also in cases of faint extended emission around point-sources. The chop/nod mode is no longer recommended for use.
    • However, for a technical assessment of the original chop/nod mode sensitivity intended for point-sources, we refer to SAp-PACS-MS-0711-09 (5.5 Mb).

PACS spectrometer calibration

  • PACS Spectrometer performance and calibration: The PACS Spectrometer Calibration Document v2.3 (31-May-2011) provides details on the calibration accuracy and the necessary information to optimally interpret PACS spectroscopy observations. New issues of this document will be released with new versions of the pipeline and new versions of the calibration tree provided in the Herschel interactive data analysis system.

  • Data processing known issues of standard products: Browse quality Level 2 products are provided in the Herschel Science Archive. This summary page describes typical problems and caveats the observer needs to be familiar when looking at these preview products. Aspects of product quality which can be further optimised by interactive processing are also summarised here. The document refers to the version of data processing pipeline currently being used for processing of incoming Herschel data (version number provided therein).

Interest Groups and Scripts

Links

  • Scanamorphos by H. Roussel can be used to build maps from scan observations made with bolometer arrays, in particular with the PACS and SPIRE photometers.
  • Key information of PACS on the NHSC web site.
Topic attachments
I Attachment History Action Size Date Who Comment
PDFpdf ExtSrcPhotom.pdf r1 manage 3303.5 K 2011-04-12 - 18:26 BrunoAltieri  
PDFpdf PACSPSF_PICC-ME-TN-029_v2.0.pdf r1 manage 3171.5 K 2010-11-05 - 16:28 BrunoAltieri  
PDFpdf PDRG_Jun2011.pdf r1 manage 5346.0 K 2011-06-07 - 22:27 KatrinaExter PDRG Jun 2011
PDFpdf PICC-NHSC-TN-029.pdf r1 manage 975.7 K 2011-04-12 - 18:30 BrunoAltieri  
PDFpdf PPR_Jun2011.pdf r1 manage 4338.0 K 2011-06-07 - 22:33 KatrinaExter PPR Jun 2011
PDFpdf PacsSpectroscopyPerformanceAndCalibration_31May2011.pdf r1 manage 2329.4 K 2011-06-02 - 13:28 JeanMatagne  
PDFpdf PhotMiniScan_ReleaseNote_20101112.pdf r1 manage 1988.8 K 2011-06-06 - 17:05 BrunoAltieri  
PDFpdf SimulPSP_v1.0.pdf r1 manage 5323.7 K 2010-11-15 - 11:16 BrunoAltieri  
PDFpdf aa14535-10.pdf r1 manage 1571.0 K 2010-11-04 - 16:23 BrunoAltieri  
PDFpdf bolopsfv1.01.pdf r1 manage 5658.9 K 2010-11-05 - 16:27 BrunoAltieri  
PDFpdf cc_report_v1.pdf r1 manage 2578.7 K 2011-04-12 - 18:30 BrunoAltieri  
PDFpdf pacs_bolo_fluxcal_report_v1.pdf r1 manage 3122.3 K 2011-04-12 - 19:40 BrunoAltieri  
Edit | Attach | Watch | Print version | History: r162 | r45 < r44 < r43 < r42 | Backlinks | Raw View | Raw edit | More topic actions...
Topic revision: r43 - 2011-06-09 - BrunoAltieri
 
This site is powered by the TWiki collaboration platform Powered by Perl