J/A+A/456/881       EIS: infrared deep public survey         (Olsen+, 2006)

ESO imaging survey: infrared deep public survey. Olsen L.F., Miralles J.-M., da Costa L., Madejsky R., Jorgensen H.E., Mignano A., Arnouts S., Benoist C., Dietrich J.P., Slijkhuis R., Zaggia S. <Astron. Astrophys. 456, 881 (2006)> =2006A&A...456..881O 2006A&A...456..881O (SIMBAD/NED BibCode)
ADC_Keywords: Surveys ; Infrared sources ; Photometry, infrared Keywords: catalogs - surveys - stars: general - galaxies: general Abstract: This paper is part of the series presenting the final results obtained by the ESO Imaging Survey (EIS) project. It presents new J and Ks data obtained from observations conducted at the ESO 3.5m New Technology Telescope (NTT) using the SOFI camera. These data were taken as part of the Deep Public Survey (DPS) carried out by the ESO Imaging Survey program, significantly extending the earlier optical/infrared EIS-DEEP survey presented in a previous paper of this series. The DPS-IR survey comprises two observing strategies: shallow Ks observations providing nearly full coverage of pointings with complementary multi-band (in general UBVRI) optical data obtained using ESO's wide-field imager (WFI) and deeper J and Ks observations of the central parts of these fields. Currently, the DPS-IR survey provides a coverage of roughly 2.1 square degrees (∼300 SOFI pointings) in Ks with 0.63 square degrees to fainter magnitudes and also covered in J, over three independent regions of the sky. The goal of the present paper is to briefly describe the observations, the data reduction procedures, and to present the final survey products which include fully calibrated pixel-maps and catalogs extracted from them. The astrometric solution with an estimated accuracy of <0.15" is based on the USNO catalog and limited only by the accuracy of the reference catalog. The final stacked images presented here number 89 and 272, in J and Ks, respectively, the latter reflecting the larger surveyed area. The J and Ks images were taken with a median seeing of 0.7" and 0.8". The images reach a median 5 sigma limiting magnitude of J_AB∼23.06 as measured within an aperture of 2", while the corresponding limiting magnitude in Ks_AB is ∼21.41 and ∼22.16mag for the shallow and deep strategies. Although some spatial variation due to varying observing conditions is observed, overall the observed limiting magnitudes are consistent with those originally proposed. The quality of the data has been assessed by comparing the measured magnitude of sources at the bright end directly with those reported by the 2MASS survey and at the faint end by comparing the counts of galaxies and stars with those of other surveys to comparable depth and to model predictions. The final science-grade catalogs together with the astrometrically and photometrically calibrated co-added images are available at CDS. Description: The subdirectory "cat" includes the science grade catalogs extracted for each of the fields covering the 2.1 square degrees discussed in this paper and the log-files associated with each catalog. The data set extends the one presented in Olsen et al., 2006, Cat. J/A+A/452/119. The catalog files are in FITS format containing the primary HDU and 4 tables (MASKS, FILTER, OBJECTS and FIELDS) with the format described in Dietrich et al., 2006, Cat. J/A+A/452/119. The log files contain information about parameters used in the extraction process as well as parameters for quality assessment of the catalogs. The subdirectory "ima" includes the science grade images created for each of the fields covering the 2.1 square degrees discussed in this paper and the log-files associated with each catalog. The data set extends the one presented in Olsen et al., 2006, Cat. J/A+A/452/119. The images are in FITS format with two extensions, the first one giving the actual image and the second one being a weight map. The details of the field naming convention can be found at http://www.eso.org/science/eis File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file fields.dat 127 355 Fields (in 1 or 2 photometric bands) deep1.dat 128 70559 deep1 field selected values, for guidance deep2.dat 128 75659 deep2 field selected values, for guidance deep3.dat 128 77284 deep3 field selected values, for guidance desccat.dat 81 69 Content of the file object in cat/*.cat fits files cat/* . 3 *Science grade catalogs and corresponding logfiles ima/* . 3 *Science grade images and corresponding logfiles -------------------------------------------------------------------------------- Note on cat/*, ima/*: catalog or images are stored in FITS format (extension .fits); log files are stored as gzipped tar files (extension .tgz) -------------------------------------------------------------------------------- See also: http://www.eso.org/eis/ : ESO Imaging Survey home page J/A+A/452/119 : EIS: infrared observations of CDF-S and HDF-S (Olsen+, 2006) J/A+A/379/740 : ESO Imaging Survey (EIS) (Arnouts+, 2001) J/A+A/384/81 : ESO Imaging Survey. CDF-S point sources (Hatziminaoglou+, 2002) J/A+A/392/741 : Stellar Catalogue in the Chandra DFS (Groenewegen+ 2002) J/A+AS/137/75 : ESO Imaging Survey. IV. (Zaggia+, 1999) J/A+AS/137/83 : ESO Imaging Survey. VII. (Scodeggio+, 1999) Byte-by-byte Description of file: fields.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Field Field designation (deepNA_NNN) 12 A1 --- Band [JK] Photometric band 14- 40 A27 --- Cat Catalog file name (in fits) (1) 42- 71 A30 --- Catlog Name of the tar.gz file containing the logs as a series of image files, html and xml files 72- 98 A27 --- Image Image file name (in fits) 100-127 A28 --- Imalog Name of the tar.gz file containing the logs as a series of image files, html and xml files -------------------------------------------------------------------------------- Note (1): Catalogues are stored as FITS files, with 4 extensions in addition to the primary HDU: -- MASKS 1 column -- FILTER 4 columns - filter transmission and response of the entire system -- OBJECTS 69 columns - the actual object list (columns described in the file "desccat.dat") -- FIELDS 109 columns - general information about the field -------------------------------------------------------------------------------- Byte-by-byte Description of file: deep1.dat deep2.dat deep3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 10 A10 --- Field Field designation (deepNA_NNN) 12 A1 --- Band [JK] Photometric band 14 I1 --- --- [1] Field number 16- 19 I4 --- Seq Sequential number 21- 28 F8.4 mag magISO Isophotal magnitude in Band 31- 37 F7.4 mag magAUTO Kron-like elliptical aperture magnitude in Band 39- 49 F11.7 deg RAdeg Right ascension in decimal degrees, J2000 51- 61 F11.7 deg DEdeg Declination in decimal degrees, J2000 63- 69 F7.3 pix A Profile RMS along major axis 71- 76 F6.3 pix B Profile RMS along minor axis 78- 82 F5.1 deg Theta Position angle 84- 88 F5.3 --- Ell Ellipticity (1-B/A) 90- 93 F4.2 --- S/G Star/Galaxy classifier (0 galaxy, 1 star) 95-104 F10.3 pix FluxRad Fraction-of-light radii 106-128 A23 --- File Name of the FITS file containing the complete data, in subdirectory cat -------------------------------------------------------------------------------- Byte-by-byte Description of file: desccat.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 19 A19 --- Param Parameter name 21- 33 A13 --- Unit Unit of the parameter 34- 81 A48 ---- Expla Explanation of the parameter -------------------------------------------------------------------------------- Acknowledgements: Lisbeth Fogh Olsen, LisbethFogh.OLSEN(at)obs-nice.fr, Dark Cosmology Centre, Niels Bohr Institute References: Dietrich et al., Paper I 2006A&A...449..837D 2006A&A...449..837D Olsen et al., Paper II 2006A&A...452..119O 2006A&A...452..119O, Cat. J/A+A/452/119
(End) Patricia Vannier [CDS] 08-Aug-2006
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