Publications

• Dale et al. 2012
• Dale et al. 2017: 28 Mar 2016 17 May 2016 27 Jul 2016 29 Sep 2016 06 Dec 2016 08 Feb 2017
• Comments/responses for 17 May draft Hinz
• Comments/responses for 27 July draft Hunt Boquien
• Comments/responses for 29 Sept draft Brown de Looze Galametz Groves Herrera-Camus Sandstrom
• Referee iteration #1 #2

Panchromatic Global Photometry (Dale et al. 2017)

• Flux tables not corrected for MW corrected for MW
• Uncertainty tables not corrected for MW corrected for MW
• README

PACS and SPIRE Global Photometry (Dale et al. 2012)

• Table of flux densities
• Comparison of PACS and MIPS flux densities
• Overlays of apertures, fg star/bg galaxy editing 2016 2012
• Panchromatic SEDs
• Result figures

IRAC imaging

• Links to the IRAC images

PACS Spectroscopy Integration Estimates

• HSPOT-based June 2007
• Guesstimator-based January 2007

PACS Spectroscopy Individual Raster Flux Sanity Check

• 10 Feb 2012 PDF file

PACS Spectroscopy AORs

• Submitted Oct 2007: all nuc enuc strip single strip
• SDP for just N1097 and N4559 (4.5" and 10" steps)wavelength switching chopping
• SDP for just N1097 (12" steps) wavelength switching "half" of wavelength switching chopping "half" of chopping "half" of chopping with strip split into individual pieces
• SDP for just N4559 (12" steps) wavelength switching "half" of wavelength switching chopping "half" of chopping "half" of chopping with strip split into individual pieces
• Final nuc sample sample sorted by RA; coords and cz's updated 11 Feb 2010
• SPIRE- and MIPS-based off positions
• PACS Spec overlays

Preparing for Science Demonstration Phase (SDP)

• Chopping and Wavelength Switching overlays (JD's website)
• Notes
  Chopper throw options: 1',3',6'
  n1097 is 9.3'x6.3'
  n4559 is 10.7'x4.4'
  Primary SDP 15 Oct -> 30 Nov; Secondary 01 Oct -> 15 Dec
• Comments
  now using HSPOT v4.2
  wavelength switching now requires sky integrations
  n1097+n4559 time budget in hours: 20.6 (v3.4) -> 21.7 (v4.2 w/no offset in sky position) -> 23.4 (v4.2 w/offset); 49.7 (v4.2 w/chop)
  If flux estimates are not provided, bright continua and lines are assumed -> largest integration capacitors used, at risk of lower S/N for faint targets (p.3 HSpot changes doc)
  
• Questions
  Do we select "chop/nod" or "chop/nod (bright lines)"?
  Do we constrain the chop angle (or date of obs)?
  Can we longitudinally dither for strips?