Computer Science
Scientific paper
Nov 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33420313a&link_type=abstract
VizieR On-line Data Catalog: J/A+A/342/313. Originally published in: 1999A&A...342..313A
Computer Science
Infrared Sources, Surveys
Scientific paper
We have developed a new ISOCAM data reduction technique based on wavelet analysis, especially designed for the detection of faint sources in mid-infrared surveys. This method, the Pattern REcognition Technique for Isocam data (PRETI) has been used to reduce the observations of the Hubble Deep Field (HDF) and flanking fields with ISOCAM at 6.75 (LW2) and 15μm (LW3) (Rowan-Robinson et al. 1997MNRAS.289..490R). Simulations of ISOCAM data allow us to test the photometric accuracy and completeness of the reduction. According to these simulations, the PRETI source list is 95% complete in the 15μm band at 200μJy and in the 6.75μm band at 65μJy, using detection thresholds which minimize the number of false detections. We detect 49 objects in the ISO-HDF at high confidence secure level, 42 in the LW3 filter, 3 in the LW2 filter, and 4 in both filters. An additional, less secure, list of 100 sources is presented, of which 89 are detected at 15μm only, 7 at 6.75μm only and 4 in both filters. All ISO-HDF objects detected in the HDF itself have optical or infrared counterparts, except for one from the additional list. All except one of the radio sources detected in the field by Fomalont et al. (1997ApJ...475L...5F) are detected with ISOCAM. Using a precise correction for the field of view distortion of ISOCAM allows us to separate blended sources. This, together with the fact that PRETI allows to correct data on the tail of cosmic rays glitches, lead us to produce deeper source lists than previous authors. Our list of bright sources agree with those of Desert et al. (1999A&A...342..363D) in both filters, and with those of Goldschmidt et al. (1997MNRAS.289..465G) in the LW3 filter, with systematic difference in photometry.
ISO is an ESA project with instruments funded by ESA Member States (especially the PI countries: France, Germany, The Netherlands and the United Kingdom) and with participation of ISAS and NASA.
(3 data files).
Aussel Herve
Cesarsky Catherine J.
Elbaz David
Starck Jean-Luc
No associations
LandOfFree
ISO HDF observations from PRETI method (Aussel+, 1999) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with ISO HDF observations from PRETI method (Aussel+, 1999), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and ISO HDF observations from PRETI method (Aussel+, 1999) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1194637