Hervé Dole et al.
OU-MER - Euclid FR - Jan 2016 - H. Dole IAS 1
Euclid OU-MER
MER tasks – 1. MER photometry strategies – 2. Pipeline Interface Reconciliation Meeting in Rome, December 2015 – 3. Conclusions, perspectives – 4.
Euclid OU-MER Herv Dole et al. MER tasks 1. MER photometry - - PowerPoint PPT Presentation
Euclid OU-MER Herv Dole et al. MER tasks 1. MER photometry strategies 2. Pipeline Interface Reconciliation Meeting in Rome, December 2015 3. Conclusions, perspectives 4. OU-MER - Euclid FR - Jan 2016 - H. Dole IAS 1 1. MER
Hervé Dole et al.
OU-MER - Euclid FR - Jan 2016 - H. Dole IAS 1
MER tasks – 1. MER photometry strategies – 2. Pipeline Interface Reconciliation Meeting in Rome, December 2015 – 3. Conclusions, perspectives – 4.
Background subtraction
Object detection Multiband photometry Mosaics PSF homogenization Object deblending Morphology, source classification MER deliveries
(multiband photometry, classification)
providers customers
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Internal simulations Aperture photometry PSF fitting photometry
Background subtraction
Object detection Multiband photometry Mosaics PSF homogenization Object deblending Morphology, source classification MER products
(multiband photometry, classification)
providers customers
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Internal simulations Aperture photometry PSF fitting photometry MER: total of 13 WP w/ 3 french-led
Aperture Photometry on PSF-homogenized images Multiband PSF-fitting photometry PSF-fitting algorithm (e.g. TPHOT) Optimal PSF-matching Homogeneous PSF-matching
MER multiband photometry
All options require PSF homogenization kernels Homogenization to the largest PSF
Homogenization “band-to-band” for each color Kernel used for model, minimization & check
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Courtesy Alexandre Boucaud
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proximité SWG-OU souhaitable, à l’exemple de CL-SWG–LE3 ? SWG: P-A Duc, M. Huertas
MER-PHZ Data Challenge #2 ongoing/done Protopipeline MER assembled Important Rome December Meeting Morphology: SWG & MER are already working (CEA/AIM, GEPI, IAS, OA Roma); will include VIS
Test of codes; meeting in january;
Next Garage Days will have MER/EXT topics discussed Photometric quality in overdense regions (e.g galaxy clusters) Some challenges
PSF requirements: NIR (undersampling) / VIS (color) > MER > PHZ Background subtraction
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MER: Rome meeting, Dec 2015 outcome
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MER: Rome meeting, Dec 2015 outcome
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MER: Rome meeting, Dec 2015 outcome
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MER: Rome meeting, Dec 2015 outcome
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MER: Rome meeting, Dec 2015 outcome
15
HD, AB, July 2014 - adapted from Santiago Serrano, May 2014
VIS SIR MER EXT PHZ LE3 SHE SPE
Shear EC Catalogue Survey mask Raw VIS Raw NISP-P Raw NISP-S NIR detections VIS images & catalogue Gaia Catalogue Gaia catalogue Coadded images multi-band catalogue Spectroscopic Training Sample Calibrated single-epoch VIS exposures Euclidized Ground Based frames & catalogues Spectra EC Catalogue 2D SIR images 1D SIR spectra NIR + EXT Detections NIR Detections with Photo-z VIS catalogue with source density NIR images & catalogue Photo-z EC Catalogue
Level 1 Level 2 Level 3 Level EXT Image data Catalogue data
Ground Based Raw Images (DES - KIDS + HSC + ...) Ground Based catalogues
NIR
Photo-z EC Catalogue
SIM
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tools -> multiband detection -> multi-wv photometry -> sims -> validation -> red: IAS responsability in OU-MER as of Dec 1st, 2015 OU-MER Lead: IT Co-lead: FR, DE SDC lead: IT FR: IAS, IRAP , APC
VIS NISP h-band NISP j-band NISP y-band
40 x 40 arcsecs
Convolution of input image with the produced kernel to the NISP h-band
premilinary simulated PSF kindly provided by OU-SIM P . Hudelot (IAP) and G. Seidel (MPIA)
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