II/252              The DENIS database, 2nd Release     (DENIS Consortium, 2003)

Second release of DENIS data (07 April 2003) The DENIS consortium <The DENIS consortium (2003)>
ADC_Keywords: Infrared sources ; Photometry, infrared ; Surveys Keywords: infrared: stars - Galaxy: stellar content - stars: low-mass, brown dwarfs - astronomical data bases: miscellaneous - surveys Description: This catalogue is an intermediate release of the DENIS project. It consists of a set of 195204157 point sources detected by the DENIS survey in 2239 strips (covering each 30 degrees in declination and 12 arcmin in right ascension). The data in this release cover approximately 11000 square degrees of the Southern sky. Multiple detections of single point sources have been merged in image overlaps within individual strips, but sources can have multiple detections in overlapping strips. The complete set of data collected by DENIS in the period 1996-2001 will be released towards the end of 2003. DENIS is the only astronomical survey of the Southern sky made in two near-infrared bands (J at 1.25µm, and Ks at 2.15µm) and one optical band (Gunn-i at 0.82µm), with limiting magnitudes 14.0, 16.5 and 18.5, respectively. It was conducted by a European consortium, using the 1m telescope at ESO, La Silla (Chile). The DENIS instrument is made up of a 3-channel camera built of commercially available detector arrays by the Observatoire de Paris and with major contributions from other European Institutes, notably: the IAS in Frascati, the Observatoire de Grenoble, the University of Innsbruck, the Observatoire de Lyon, and the IAC in Tenerife. The survey is carried out by observing strips of 30° in declination and 12arcminutes in Right Ascension with an overlap of 2arcminutes between consecutive strips. The survey started at the end of 1995 and has been completed up to 97% in 2001. The data have been reduced at the Institut d'Astrophysique de Paris and Observatoire de Paris. The position of a general extracted point source is provided with an accuracy better than 1arcsec and its magnitude to better than 0.1mag. The Centre de Donnees Astronomiques de Strasbourg (CDS) is releasing the final databases and provides access of the processed and calibrated data to the worldwide community. The principal investigator of the DENIS project is N. Epchtein (Observatoire de la Cote d'Azur); the Co-PI in charge of data processing is G. Simon (observatoire de Paris); J. Borsenberger and B. de Batz, with the help of F. Tanguy, S. Begon and P. Texier, processed the data and implemented the working data base at PDAC; S. Derriere is in charge of the data release at CDS. Scientists and engineers from seven European countries and from Brazil are involved in the data qualification and analysis. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . The present file denis.sam 469 1000 Sample of DENIS output -------------------------------------------------------------------------------- See also: http://cdsweb.u-strasbg.fr/denis.html : DENIS documentation II/240 : Preliminary database of DENIS point sources (1999A&A...349..236E 1999A&A...349..236E) J/A+AS/135/133 : First DENIS I-band extragalactic catalog (Vauglin+ 1999) 2000A&AS..141..313F 2000A&AS..141..313F : An Absolute Calibration of DENIS (Fouque et al.) Nomenclature Notes: The recommended way to designate the DENIS sources is DENIS JHHMMSS.s-DDMMSS Byte-by-byte Description of output: denis.sam -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 16 A16 --- DENIS DENIS name, identifier 18- 27 F10.6 deg RAJ2000 Right ascension (J2000) 29- 38 F10.6 deg DEJ2000 Declination (J2000) 40- 46 I7 --- Image DENIS image number (1) 48- 52 I5 --- Strip DENIS strip number 54- 59 F6.3 mag Imag ?Magnitude in I band from PSF fit 61- 64 F4.2 mag e_Imag ?Magnitude error in I band from PSF fit 66- 71 F6.3 mag Jmag ?Magnitude in J band from PSF fit 73- 76 F4.2 mag e_Jmag ?Magnitude error in J band from PSF fit 78- 83 F6.3 mag Kmag ?Magnitude in K band from PSF fit 85- 89 F5.2 mag e_Kmag ?Magnitude error in K band from PSF fit 91- 96 F6.3 mag Imag5.5 ?Magnitude in I band from 5.5'' aperture 98-102 F5.2 mag e_Imag5.5 ?Error in I band mag from 5.5'' aperture 104-109 F6.3 mag Jmag5.5 ?Magnitude in J band from 5.5'' aperture 111-115 F5.2 mag e_Jmag5.5 ?Error in J band mag from 5.5'' aperture 117-122 F6.3 mag Kmag5.5 ?Magnitude in K band from 5.5'' aperture 124-128 F5.2 mag e_Kmag5.5 ?Error in K band mag from 5.5'' aperture 130-135 F6.3 mag Imag4.5 ?Magnitude in I band from 4.5'' aperture 137-141 F5.2 mag e_Imag4.5 ?Error in I band mag from 4.5'' aperture 143-148 F6.3 mag Jmag4.5 ?Magnitude in J band from 4.5'' aperture 150-154 F5.2 mag e_Jmag4.5 ?Error in J band mag from 4.5'' aperture 156-161 F6.3 mag Kmag4.5 ?Magnitude in K band from 4.5'' aperture 163-167 F5.2 mag e_Kmag4.5 ?Error in K band mag from 4.5'' aperture 169-174 F6.3 mag Imag3.5 ?Magnitude in I band from 3.5'' aperture 176-179 F4.2 mag e_Imag3.5 ?Error in I band mag from 3.5'' aperture 181-186 F6.3 mag Jmag3.5 ?Magnitude in J band from 3.5'' aperture 188-192 F5.2 mag e_Jmag3.5 ?Error in J band mag from 3.5'' aperture 194-199 F6.3 mag Kmag3.5 ?Magnitude in K band from 3.5'' aperture 201-205 F5.2 mag e_Kmag3.5 ?Error in K band mag from 3.5'' aperture 207-212 F6.3 mag Imag3.5c ?I band Magnitude in 3.5'' corrected aperture 214-217 F4.2 mag e_Imag3.5c ?I band mag error in 3.5'' corrected aperture 219-224 F6.3 mag Jmag3.5c ?J band Magnitude in 3.5'' corrected aperture 226-230 F5.2 mag e_Jmag3.5c ?J band mag error in 3.5'' corrected aperture 232-237 F6.3 mag Kmag3.5c ?K band Magnitude in 3.5'' corrected aperture 239-243 F5.2 mag e_Kmag3.5c ?K band mag error in 3.5'' corrected aperture 245-250 F6.3 mag Imag2.5c ?I band Magnitude in 2.5'' corrected aperture 252-255 F4.2 mag e_Imag2.5c ?I band mag error in 2.5'' corrected aperture 257-262 F6.3 mag Jmag2.5c ?J band Magnitude in 2.5'' corrected aperture 264-268 F5.2 mag e_Jmag2.5c ?J band mag error in 2.5'' corrected aperture 270-275 F6.3 mag Kmag2.5c ?K band Magnitude in 2.5'' corrected aperture 277-281 F5.2 mag e_Kmag2.5c ?K band mag error in 2.5'' corrected aperture 283-288 F6.3 mag Imag1.5c ?I band Magnitude in 1.5'' corrected aperture 290-293 F4.2 mag e_Imag1.5c ?I band mag error in 1.5'' corrected aperture 295-300 F6.3 mag Jmag1.5c ?J band Magnitude in 1.5'' corrected aperture 302-306 F5.2 mag e_Jmag1.5c ?J band mag error in 1.5'' corrected aperture 308-313 F6.3 mag Kmag1.5c ?K band Magnitude in 1.5'' corrected aperture 315-319 F5.2 mag e_Kmag1.5c ?K band mag error in 1.5'' corrected aperture 321-324 F4.1 mag Rmag ?R magnitude of USNOA2.0 nearest match 326-329 F4.1 mag Bmag ?B magnitude of USNOA2.0 nearest match 331-333 I3 --- q_Imag [0,100]?Quality flag for I band (100=top) 335-337 I3 --- q_Jmag [0,100]?Quality flag for J band (100=top) 339-341 I3 --- q_Kmag [0,100]?Quality flag for K band (100=top) 343-344 I2 % Ipsf [0,100]?Correlation to PSF for I band (4) 346-347 I2 % Jpsf [0,100]?Correlation to PSF for J band (4) 349-350 I2 % Kpsf [0,100]?Correlation to PSF for K band (4) 352-355 F4.2 --- IMpsf [0,1]?Mean correlation to PSF in I band (4) 357-360 F4.2 --- JMpsf [0,1]?Mean correlation to PSF in J band (4) 362-365 F4.2 --- KMpsf [0,1]?Mean correlation to PSF in K band (4) 367-371 F5.1 pix Ix ?Pixel x position in I band 373-377 F5.1 pix Iy ?Pixel y position in I band 379-383 F5.1 pix Jx ?Pixel x position in J band 385-389 F5.1 pix Jy ?Pixel y position in J band 391-395 F5.1 pix Kx ?Pixel x position in K band 397-401 F5.1 pix Ky ?Pixel y position in K band 403-412 F10.6 deg A2RAdeg ?Right Ascension of USNOA2.0 nearest match 414-423 F10.6 deg A2DEdeg ?Declination of USNOA2.0 nearest match 425-432 F8.3 yr A2Ep ?Epoch of USNOA2.0 nearest match 434-437 I4 mas Dist ?Distance to USNOA2.0 nearest match 439-452 F14.6 d ObsJD Julian day for DENIS observation 454-457 A4 --- Iflg ?Image and source flag in I band (2) 459-462 A4 --- Jflg ?Image and source flag in J band (2) 464-467 A4 --- Kflg ?Image and source flag in K band (2) 469-469 I1 --- mult ?Multiplicity flag (3) -------------------------------------------------------------------------------- Note (1): the image number is incremented at each image taken during the survey. In case a source results from the merging of two consecutive overlapping images (N and N+1) in the same strip (Flag_mult set to 1, see Note 3), the image number corresponds to the first image N. Note (2): This flag is the concatenation of image and source flags, in hexadecimal format. For the image flag, the first two digits contain: Bit 0 (0100) clouds during observation Bit 1 (0200) electronic Read-Out problem Bit 2 (0400) internal temperature problem Bit 3 (0800) very bright star Bit 4 (1000) bright star Bit 5 (2000) stray light Bit 6 (4000) unknown problem For the source flag, the last two digits contain: Bit 0 (0001) source might be a dust on mirror Bit 1 (0002) source is a ghost detection of a bright star Bit 2 (0004) source is saturated Bit 3 (0008) source is multiple detect Bit 4 (0010) reserved Note (3): if set to 1, this flag indicates that the source was detected in two consecutive images, and that the 2 measurements have been combined Note (4): the correlation with the PSF is higher for the point sources, whereas cosmics have a very low correlation. The mean correlation values xMpsf are a function of the magnitude only, and do not depend on individual sources. -------------------------------------------------------------------------------- Acknowledgements: DENIS is the result of a joint effort involving human and financial contributions of several Institutes mostly located in Europe. It has been supported financially mainly by the French Institut National des Sciences de l'Univers, CNRS, and French Education Ministry, the European Southern Observatory, the State of Baden-Wuerttemberg, and the European Commission under networks of the SCIENCE and Human Capital and Mobility programs, the Landessternwarte, Heidelberg, l'Institut d'Astrophysique de Paris, the Institut fur Astrophysik der Universitat Innsbruck and Instituto de Astrofisica de Canarias. History: * 07-Apr-2003: Installation at CDS, as catalog "B/denis" * 22-Sep-2005: Becomes catalog "II/252" * 28-Jan-2025: format migration (CDS) References: The DENIS Consortium (April 2003)
(End) Nicolas Epchtein [OCA], Sebastien Derriere [CDS] 07-Apr-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