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NHSC SPIRE Data Processing Webinars 8th Feb 2012 Overview of SPIRE Photometer Pipeline C. Kevin Xu (NHSC/IPAC) page ‹#› PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 Goals: • Show how SPIRE Photometer pipeline works (functionalities of major modules). • Explain what is new in HIPE 8. • Brief summary of remaining issues. • Will concentrate on scan map “user pipelines” (covering small map, large map, SPIRE/PACS parallel mode). page ‹#› PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 User Pipelines • User pipelines (Jython scripts): Simplified version of Standard Product Generation (SPG) pipelines. • You can find these “user pipelines” in HIPE: page ‹#› PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 SPIRE Pipeline & Data Products 5’ (in HIPE) Our focus (“user pipelines”) page ‹#› PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 Scan Map Pipeline Flow Chart A “reversed sequence” relative to the chain of data acquisition place-holder • FFT based • Default: concurrent deglitcher + wavelet deglitcher • Alternative: σ-κ deglitcher FFT based (run after deglitch & repair to avoid ringing) • Telescope pointing & orientation • SPIRE detectors positions Choices: • Default: scan median baseline removal Include: • Advanced : polynomial baseline removal (1) Non-linearity correction (2) Volt to Jy/beam conversion• Most advanced: an iterative destriper Remove 1/f noise due to T-drift Baseline removal + Mapper • Default: naïve mapper • Alternative: madmapper page ‹#› PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 Scan-By-Scan Processing • The pipeline processes timelines scan by scan (to ease the demand on RAM). • Problem: ringing at the two ends of each scan due to FFT based modules. • Solution: (1) Before the process, attaching “turn-around” data blocks to ends of the scan. (2) During the process, the ringing is confined to the “turn-around” data. (3) After the process, cut-off the “turn-around” data blocks from the scan. Uniform scan speed distance Turnaround page ‹#› PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 Highlights of a User Pipeline (Jython Script) New in HIPE 8.0 (for extended source, optional) page ‹#› PACS Signal “Jump” NHSC SPIRE Data Processing Webinars 8th Feb 2012 • Sudden (spontaneous?) jump in the timeline of a single channel. • Mostly seen in thermistors (see below). Very rarely seen in detectors. • The average frequency is ~ 1/day ( a few hundred instances since launch). • The cause is still unknown. • Effect: The pipeline uses thermistor timelines in the correction for detector signal drift due to bath temperature drift (major source of 1/f noise for SPIRE). A thermistor “jump” affects this correction, introducing artificial stripes in the final map. Jump page ‹#› Stripe caused by the jump PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 New module Jump Detector (automatically identify & mask any thermistor affected by a jump) Thermistor Jump Solution (in HIPE 8.0) • a “reversed sequence” relative to the chain of data acquisition • scan by scan processing Destriper + Mapper Exclude masked thermistors page ‹#› PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 Status of SPIRE Scan Map Pipeline in HIPE 8.0. SPIRE 3-color map of NGC 5315 (a planetary nebula) • General assessment: In many cases, data from HSA are already science quality! • The official calibration accuracy is ±7% (5% from model, 2% RMS). • An example (on the right): The image from HSA looks good. Caveat: detailed inspections show thin stripes (can be improved using a more advanced baseline remover such as the iterative destriper). • A major issue yet to resolve: stripes due to bias voltage drift (the “burp”) (affecting a few observations) page ‹#› (Public data taken from HSA) PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 Bias Drift in “Burp” Period • Every time when SPIRE is switched on after a cooler recycle, the first ~6 h sees a rapid rise of bias voltage (the “burp”). • This effect has not been corrected in pipeline. • It causes stripes in maps observed during the “burp” period (see example below). • A pipeline module is now being developed to correct this effect (available soon). • For point source surveys, the stripes might be removed by polynomial baseline removal. An example of stripes caused by bias drift Resistor voltage After cooler recycle 1 (~40 h) Bias voltage After cooler recycle 2 (~40 h) bias drift ~10σ “burp” ~ 6h (Standard pipeline product) page ‹#› PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 Summary • Scan-Map pipeline covers nearly all SPIRE PHOT AOTs (small map, large map, map in SPIRE/PACS parallel mode). • It follows a “reversed sequence” relative to the chain of data acquisition. • For a general user, Level0_5 should be the best starting point. • From Level0_5 to Level 1, the pipeline processes any observation data set scan by scan (to ease the demand on the RAM). • The current pipeline (HIPE 8.0.1) does a good job (“science ready”) in general. • However, the pipeline still has some open issues: that (1) Stripes due to the “burp effect” (affecting ~10% observations). (2) Residual stripes (can be corrected by the destriper module in HIPE). (3) Residual glitches in maps (2nd level deglitcher being developed inside the destriper module). page ‹#› PACS NHSC SPIRE Data Processing Webinars 8th Feb 2012 • Home work: Run Photometer Large Map user pipeline (with your own data or NGC 5315 data). • Next: A demo of SPIA (SPIRE Photometer Interactive Analysis), a GUI based data reduction tool (including all pipeline modules and more). page ‹#› PACS