J/A+A/403/493       H-band observation of Chandra Deep Field South (Moy+, 2003)

H-band observations of the Chandra Deep Field South. Moy E., Barmby P., Rigopoulou D., Huang J.-S., Willner S.P., Fazio G.G. <Astron. Astrophys. 403, 493 (2003)> =2003A&A...403..493M 2003A&A...403..493M
ADC_Keywords: Photometry, infrared ; Infrared sources Keywords: catalogs - surveys - infrared: general - galaxies: general - stars: general - cosmology: observations Abstract: We report preliminary results of our H-band survey of the Chandra Deep Field South (CDFS). The observations were made using SofI on the NTT, and cover 0.027 square degrees with a 50% completeness limit of H=20.5, and 0.17 square degrees with a 50% completeness limit of H=19.8. We used SExtractor to extract sources from our fields. In total we have detected 4819 objects. Star-galaxy separation was performed using the SExtractor parameter "stellarity index". All objects with an index of 0.5 or lower were classified as galaxies. According to this criterion, 80% of our detections are galaxies. We then compare our results with previous observations of the CDFS. Our astrometric solutions are in good agreement with the Las Campanas Infrared Survey (LCIRS), the COMBO-17 and the ESO-EIS surveys. The photometry of our catalog compares satisfactorily with the results of the LCIRS, as well as with the GOODS data. Galaxy number counts are presented and compared with the LCIRS results. The present data are intended to complement the recent and future multi-wavelength observations of the CDFS and will be used, in conjunction with additional multiband photometry, to find counterparts of the upcoming mid-infrared surveys with SIRTF. Description: Photometric parameters for 4819 stars and galaxies in the Chandra Deep Field South are presented. For each objects equatorial coordinates, total, isophotal, aperture (3 arcsec.) H-band magnitudes and errors, and stellarity index are given. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table2.dat 90 4819 Photometric parameters for 4819 stars and galaxies -------------------------------------------------------------------------------- See also: VII/228 : Las Campanas Infrared Survey (Chen+, 2001-2002) J/A+A/379/740 : ESO Imaging Survey (EIS) (Arnouts+, 2001) Byte-by-byte Description of file: table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- --- [CDFSH] 8- 11 I4 --- CDFSH [1/4819] Object identification number 14- 15 I2 --- Field Field number 18- 19 I2 h RAh Right ascension (J2000) 20 A1 --- --- [:] 21- 22 I2 min RAm Right ascension (J2000) 23 A1 --- --- [:] 24- 28 F5.2 s RAs Right ascension (J2000) 31 A1 --- DE- Declination sign 32- 33 I2 deg DEd Declination (J2000) 34 A1 --- --- [:] 35- 36 I2 arcmin DEm Declination (J2000) 37 A1 --- --- [:] 38- 42 F5.2 arcsec DEs Declination (J2000) 45- 49 F5.2 mag HmagT Total H magnitude, as estimated by SExtractor 52- 56 F5.3 mag e_HmagT Error on total H magnitude 59- 63 F5.2 mag HmagI Isophotal H magnitude, as estimated by SExtractor 66- 70 F5.3 mag e_HmagI Error on isophotal H magnitude 73- 77 F5.2 mag HmagA Apertude H magnitude (10 pixels, or 2.9" diameter) 80- 84 F5.3 mag e_HmagA Error on aperture H magnitude 87- 90 F4.2 --- Class SExtractor Stellarity index (1) -------------------------------------------------------------------------------- Note (1): A value close to 1 indicates a star; a value close to zero indicates a galaxy. -------------------------------------------------------------------------------- Acknowledgements: Emmanuel Moy
(End) Patricia Bauer [CDS] 30-May-2003
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line