PESSTO PESSTO pipeline in addition to Quality Control Team NTT large Program NTT large Program

PESSTO PESSTO pipeline in addition to Quality Control Team NTT large Program NTT large Program www.phwiki.com

PESSTO PESSTO pipeline in addition to Quality Control Team NTT large Program NTT large Program

Chiodo, Joe, Co-Publisher has reference to this Academic Journal, PHwiki organized this Journal PESSTO Data Reduction PESSTO meeting PESSTO pipeline in addition to Quality Control Team S. Valenti B. Schmidt C. Inserra S. Mattila M. Fraser F. Patat M. Sullivan G. Pignata E. Cappellaro E. Kankare M. Ergon PESSTO meeting Provide Data reduction Pipeline (documentation, pipeline, testing) The Server of data reduction Provide support to the Data reduction Team Check data quality of the reduced data PESSTO meeting

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NTT large Program PESSTO meeting Data reduction QUBA PIPELINE: pre-reduction images EFOSC2, 1.82 ekar, NOT, TNG pre-reduction spectra EFOSC2, 1.82 ekar, NOT, TNG,ISIS reduction spectra EFOSC2, 1.82 ekar, NOT, TNG,ISIS Photometry (a python version of the snoopy-iraf package) NTT (SOFI in addition to EFOSC2), 1.82 ekar, NOT, TNG (NICS in addition to DOLORES) Liverpool Telescope, Calar Alto, FORS1, FORS2, .etc. Python with Pyraf, Pylab, Pyfits Several (but not all) people in the collaboration are using it Try to install the pipeline on the pc of each reducer interested in using the pipeline New version released by me by email in addition to a link where to download the pipeline NTT large Program PESSTO meeting RUN date Observer EFOSC2 SOFI 19-21/10/09 C. Inserra photometry(prered) NOT REDUCED 21-23/11/09 M. Ergon reduced (QUBA) NOT REDUCED 23-25/12/09 E. Kankare NOT REDUCED NOT REDUCED 22-24/01/10 G. Leloudas reduced NOT REDUCED 17-20/02/10 I. Agnoletto NOT REDUCED NOT REDUCED 04-07/03/10 Max/Salgado reduced (QUBA) NOT REDUCED 16-19/04/10 M. Turatto NOT REDUCED (some reduction at the telescope ) 27-28/05/10 M. Miluzio no observations no observations 17-19/06/10 S. Valenti reduced (QUBA) no observations 14-15/09/10 S. Benetti reduced (gasgano) reduced 3-5 /10/10 R. Kotak reduced QUBA no observations 27-29/10/10 M. Ergon NOT REDUCED NOT REDUCED 30-01/12/10 M. Miluzio reduced (QUBA) NOT REDUCED 23-25/01/11 C. Inserra photometry(prered) NOT REDUCED 10-12/02/11 F. Bufano NOT REDUCED NOT REDUCED 24-26/03/11 E. Kankare photometry(prered) NOT REDUCED 9-11/04/11 L.Tomasella photometry(prered) NOT REDUCED 07-09/05/11 N. De la Rosa photometry(prered) reduced(photometry) 23-26/06/11 S. Valenti reduced (QUBA) reduced(photometry) Data reduction PIs prefer to reduce the data of their objects more data have been reduced . (single objects, not full nights) Waste of time in addition to energy NTT large Program Not all the data, (as I would like) are reduced in addition to stored in the archive I’m getting poor feedback on the bugs of the pipeline For most of the reported bugs, my answer is: I fixed that in the last version, did you install it no I still have the old version. New reducer are open to use the pipeline, but old reducer .are not . Pipeline not user-friendly Or not better than the manual reduction PESSTO meeting PESSTO

PESSTO pipeline PYTHON module NTT-pipeline/ Add this directory to your python site-package/ export PYTHONPATH=$PYTHONPATH:path-of-site-package/ Simple python module IRAF, PYRAF, numpy (pywcs) Works from terminal no graphic interphase PESSTO meeting PESSTO meeting But missing 2D-wavelengh calibrated image PESSTO pipeline PESSTO meeting

PESSTO pipeline ~/bin/PESSTOFASTSPEC.py @list-raw-spectra options: -i = interactive mode -d = interactive dispersion line ( as long as nebular spectra) -t = trace with a bright object ( as long as faint objects) -s = use specific sensitivity function -a = use specific arc-ex file (already ext. in addition to wave. calibrated) Trim overscan, extraction (interactive with option –i ) Wavelength calibration (re-identification using data from archive) Check Wavelength calibration (with skylines) Flux calibration (using a median sensitivity curve from archive) PESSTO meeting PESSTO pipeline ~/bin/PESSTOFASTSPEC.py @list-raw-spectra PESSTO meeting Gr11+Free slit1.0 slit1.5 Gr13+Free slit1.0 slit1.5 Gr16+OG530 slit1.0 slit1.5 PESSTO pipeline ~/bin/PESSTOFASTSPEC.py @list-raw-spectra PESSTO meeting Check Wavelength calibration (with skylines) Rigid shift of sky lines to maximize the product of the two spectra Please don’t use the fast reduction as a black box

PESSTO pipeline ~bin/etabase-file.py @list-reduced-spectra Convert fits in asci Produce the asci-file with all the in as long as mation needed as long as ETABASE Obj-name, Ascii-filename, Obs-date [YYYY-MM-DD], Obs-UT [HH:MM:SS], Inst-Id, Observer/s, Exptime, Slit, Reducer, Reduction-date, Spec-Remarks, Publish, Contrib, Airmass, Dichroic, Grism, Grating, Obj-RA, Obj-DEC, IAU-name, Obj-type-Id, Redshift, Host, FITS-filename PESSTO meeting PESSTO pipeline ~/bin/PESSTOstart.py @listafiles Split files in: EFOSC-SPECTRA EFOSC-PHOTOMETRY SOFI-SPECTRA SOFI-PHOTOMETRY PESSTO meeting PESSTO pipeline ~/bin/PESSTOSOFIPHOT.py @lista-SOFI-raw-phot-files option: -f = no flat field correction -l = no illumination correction -x = no crosstalk correction -F = chose flat interactively -L = chose illumination correction interactively -i = interactive mode (not yet useful) -c = chose combine param. as long as combining images [median] -R = chose reject param as long as combining images [minmax] -s = scale zeropoint be as long as e combining images PESSTO meeting No Darks correction Flat field correction SpecFlat-20110516-H.fits (quite stable) Illumination correction Illum-20110516-H.fits (quite stable) Crosstalk correction iraf script provided in the ESO website (included in the pipeline) Combine the single sky-subtracted images

PESSTO pipeline ~/bin/PESSTOSOFIPHOT.py @lista-SOFI-raw-phot-files PESSTO meeting Special Flat field To correct as long as the shading pattern. The effect as long as most observations is small, in addition to manifests itself as a discontinuity of a few percent in the ZP across the center of the array Illumination correction Illumination of the screen can never represent accurately the illumination of the sky. The illumination correction frame refers only to the flat field used to create it. Crosstalk correction A bright source imaged on the array produces a “ghost” that affects all the lines where the source is in addition to all the corresponding lines in the other half of the detector. PESSTO pipeline ~/bin/PESSTOSOFIPHOT.py @lista-SOFI-raw-phot-files PESSTO meeting Small dither (<200 arcsec) N images >= 4 Sky with all (except A) A – = Mask-A A – Mask-C Mask-D Mask-B = Sky with all (except A) PESSTO pipeline ~/bin/PESSTOSOFIPHOT.py @lista-SOFI-raw-phot-files PESSTO meeting Small dither (<200 arcsec) N images >= 4 Sky with all (except A) A – = Mask-A A – Mask-C Mask-D Mask-B = Sky with all (except A)

PESSTO pipeline ~/bin/PESSTOSOFIPHOT.py @lista-SOFI-raw-phot-files PESSTO meeting ON – OFF (extended galaxies) dither >=200 arcsec N(off) >=3 N (on) >=3 Sky with all OFF D – = D E F D E F Mask-D A Sky with all OFF D E F – Mask-D Mask-F = PESSTO pipeline ~/bin/PESSTOSOFIPHOT.py @lista-SOFI-raw-phot-files PESSTO meeting raw Flat field, Illumination, Cross Talks sky-subtracted Providing: single sky-subtracted images PESSTO pipeline PESSTO meeting

PESSTO pipeline PESSTO meeting PESSTO pipeline PESSTO meeting PESSTO pipeline PESSTO meeting

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PESSTO pipeline PESSTO meeting St in addition to ard Objects Sensitivity curve Flux calibrated spectrum Atmosferic features correction (atm. features in the st in addition to ard, scaling an atmospheric model to the SN atm. features) PESSTO pipeline PESSTO meeting Check Wavelength calibration as long as the st in addition to ards(with atmospheric features) 2D-wavelength calibrated spectra PESSTO pipeline PESSTO meeting

PESSTO SOFI SPECTRA reduction (SS) Spectra Flux calibration (FC) Automatic flat SOFI (FS) Automatic fringing (AF) TESTING (T) Documentation (D) Server as long as data reductions (Serv) GUI interface (GUI) 2D-w-calibrated spectra (2D) Astrometry (A) Modify the code (M) Configuration Management (CM) Quality Control (QC) PESSTO meeting S. Valenti (M,T,Serv, .) B. Schmidt (FC) C. Inserra S. Mattila M. Fraser F. Patat M. Sullivan G. Pignata E. Cappellaro E. Kankare M. Ergon (CM) PESSTO PESSTO meeting Gr11+Free slit1.0 slit1.5 Gr13+Free slit1.0 slit1.5 Gr16+OG530 slit1.0 slit1.5 EFOSC2 SOFI < 200 arcsec 4 images < 200 arcsec 6 images (Different Objects name) PESSTO PESSTO meeting PESSTO PESSTO meeting PESSTO PESSTO meeting

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