Date: Wed, 25 Jan 2006 14:46:15 -0800 (PST) Subject: New/Updated Documentation and S13 Reprocessing Contents of mailing: 1. Spitzer Cycle 3 Proposal Deadline: Thursday, February 16 1:00 PM PST 2. Reprocessing of Spitzer Data with Version 13 Pipelines 3. Updated IRAC and MIPS Data Handbooks Released (or coming soon) 4. Obtaining Spectra of Very Faint Sources with the IRS 5. How to Design IRS Spectral Maps 6. Outline of IRS Data Reduction 7. MIPS 70-micron Sensitivity in Low-Background Fields 1. Spitzer Cycle 3 Proposal Deadline: Thursday February 16 1:00 PM PST Reminder: The deadline for Spitzer Cycle 3 proposals is Thursday February 16 2006 at 1:00 PM Pacific Standard Time. Submitted proposals will automatically be assigned an identification number, in the order received, starting at 30001. If you have any questions regarding submission of a Cycle 3 proposal contact our Helpdesk at help@spitzer.caltech.edu 2. Reprocessing of Spitzer Data with Version 13 Pipelines The SSC has begun reprocessing the IOC/SV and science mission data with version 13 of our pipelines (S13), starting with IRS data. IRS campaigns through 21.3 (May 28 2005) have been reprocessed, archived and released. Campaigns 22-25 are anticipated to be completed and released within one week. Over the next few months IRAC and MIPS campaigns will also be reprocessed, archived, and released. Observers can use Leopard, the Archive interface, to see the pipeline version of their data (the 'Version' column in the query results window). If it is S12.4 or earlier please be patient as it will be replaced with S13 data as we proceed with reprocessing the campaigns. The current processing status of any campaign can be found here (IRS information will be updated in the next day or two): http://ssc.spitzer.caltech.edu/archanaly/status/ 3. Updated IRAC and MIPS Data Handbooks Released (or coming soon) IRAC DH version 3.0 changes include description of the flux calibration history, new text on the creation of uncertainty images, pipeline version S13 changes, description of imask, description of scattered light rings, revised extended source calibration discussion, description of superboresight pointing refinement. Additional small updates to text in many places. Available now here: http://ssc.spitzer.caltech.edu/irac/dh/ MIPS DH version 3.2 changes include updating a variety of items to reflect S13 modifications, including new calibration factors. Available within a week here: http://ssc.spitzer.caltech.edu/mips/dh/ 4. Obtaining Spectra of Very Faint Sources with the IRS A new SSC memo that discusses the observing and data reduction strategies recommended for ultradeep spectroscopy with the IRS http://ssc.spitzer.caltech.edu/irs/documents/irs_ultradeep_memo.pdf http://ssc.spitzer.caltech.edu/irs/documents/irs_ultradeep_aors.aor 5. How to Design IRS Spectral Maps A brief HTML guide to designing IRS spectral maps from which accurate flux intensities and spectral images of extended sources can be obtained. http://ssc.spitzer.caltech.edu/irs/documents/specmap_bop/ 6. Outline of IRS Data Reduction A three page PDF document that discusses in detail the steps that need to be followed to reduce IRS data. http://ssc.spitzer.caltech.edu/irs/documents/IRSDataReductionSteps.pdf 7. MIPS 70-micron Sensitivity in Low-Background Fields Deep observations of HDF-N constrain the confusion level for the MIPS-70 band. The sensitivity for short integration times is consistent with previous measurements (7.2 mJy for 5 sigma in 500 seconds on-source in a low background), and the instrument noise integrates down with nearly square root(t) for long integration times (10ks) for the low background HDF-N field. The sensitivity at intermediate and higher backgrounds is currently being investigated. See the full report here: http://ssc.spitzer.caltech.edu/mips/documents/sens_hdf.pdf