J/A+A/342/313ivo://CDS.VizieR/J/A+A/342/313doi:10.26093/cds/vizier.33420313CDSAussel H.Cesarsky C.J.Elbaz D.Starck J.L.2004-02-02T09:18:31Z2004-02-02T10:18:13ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frinfrared-sourcessurveysWe 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 15{mu}m (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 15{mu}m band at 200{mu}Jy and in the 6.75{mu}m band at 65{mu}Jy, 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 15{mu}m only, 7 at 6.75{mu}m 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.1999A&A...342..313Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/342/313CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/iso : ISO Observation Log of validated data (ISO Data Centre, 2001)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/342/313https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/342/313http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/342/313https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/342/313https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/342/313http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/342/313GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/342/313/isocat (Provisional PRETI catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/342/313/isocat?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/342/313/isocat?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/342/313/isocat?GETtext/xml+votable180.050000true189.13083362.18750.005555555555555556Cone search capability for table J/A+A/342/313/7um (7{mu}m data)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/342/313/7um?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/342/313/7um?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/342/313/7um?GETtext/xml+votable180.050000true189.13083362.18750.005555555555555556Cone search capability for table J/A+A/342/313/15um (15{mu}m data)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/342/313/15um?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/342/313/15um?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/342/313/15um?GETtext/xml+votable180.050000true189.13083362.18750.005555555555555556ISO6/11252https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/342/313?format=asciiInfrareddefaultJ/A+A/342/313/isocatProvisional PRETI cataloguerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCatalogue ID. (1)meta.id;meta.maincharRAJ2000Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000)pos.eq.dec;meta.mainl_7um6.7 micron flux is upper limitmeta.code.errorchar7um? 6.7 micron flux in 3 arcmin apertureuJyphot.flux.density;em.IR.4-8umintnullableE_7um? Upper error bound to 6.7 micron fluxuJystat.errorintnullablee_7um? Lower error bound to 6.7 micron fluxuJystat.errorintnullablel_15um15 micron flux is upper limitmeta.code.errorchar15um15 micron flux in 6 arcsec apertureuJyphot.flux.density;em.IR.8-15umintE_15um? Upper error bound to 15 micron fluxuJystat.errorintnullablee_15um? Lower error bound to 15 micron fluxuJystat.errorintnullableJ/A+A/342/313/7um7{mu}m datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCatalogue ID. (1)meta.id;meta.maincharRAJ2000Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000)pos.eq.dec;meta.mainl_7um6.7 micron flux is upper limitmeta.code.errorchar7um? 6.7 micron flux in 3 arcmin apertureJyphot.flux.densitydoublenullableE_7um? Upper error bound to 6.7 micron fluxJystat.errordoublenullablee_7um? Lower error bound to 6.7 micron fluxJystat.errordoublenullableFreqFrequency of observation (6.7{mu}m)Hzem.freqdoublenullableFWHMBandpass of filter at 6.7{mu}mHzinstr.bandwidthdoublenullableJ/A+A/342/313/15um15{mu}m datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDCatalogue ID. (1)meta.id;meta.maincharRAJ2000Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000)pos.eq.dec;meta.mainl_15um15 micron flux is upper limitmeta.code.errorchar15um15 micron flux in 6 arcsec apertureJyphot.flux.densitydoubleE_15um? Upper error bound to 15 micron fluxJystat.errordoublenullablee_15um? Lower error bound to 15 micron fluxJystat.errordoublenullableFreqFrequency of observation 15{mu}m)Hzem.freqdoublenullableFWHMBandpass of filter at 15{mu}mHzinstr.bandwidthdoublenullable