J/A+A/451/881       ESIS BVR catalog, ELAIS-S1               (Berta+, 2006)

The ESO-Spitzer Imaging extragalactic Survey (ESIS). I. WFI B, V, R deep observations of ELAIS-S1 and comparison to Spitzer and GALEX data. Berta S., Rubele S., Franceschini A., Held E.V., Rizzi L., Lonsdale C.J., Jarrett T.H., Rodighiero G., Oliver S.J., Dias J.E., Buttery H.J., Fiore F., La Franca F., Puccetti S., Fang F., Shupe D., Surace J., Gruppioni C. <Astron. Astrophys., 451, 881-900 (2006)> =2006A&A...451..881B 2006A&A...451..881B
ADC_Keywords: Surveys ; Galaxies, photometry ; Photometry, Cousins Keywords: surveys - galaxies: evolution - cosmology: observations - infrared: galaxies - ultraviolet: galaxies - galaxies: statistics Abstract: The ESO-Spitzer extragalactic Imaging Survey (ESIS) is the optical follow up of the Spitzer Wide-Area InfraRed Extragalactic (SWIRE) survey in the ELAIS-S1 area. The multiwavelength study of galaxy emission is the key to understand the interplay of the various components of galaxies and to trace their role in cosmic evolution. ESIS provides optical identification and colors of Spitzer IR galaxies and builds the bases for photometric redshift estimates. This paper presents B, V, R Wide Field Imager observations of the first 1.5 square degree of the ESIS survey. Data reduction includes astrometric calibration, illumination and color corrections. Synthetic sources are simulated in scientific and super-sky-flat images, with the purpose of estimating completeness and photometric accuracy for the survey. Number counts and color distributions are compared to literature observational and theoretical data, including non-evolutionary, PLE, evolutionary and semi-analytic Lambda-CDM galaxy models, as well as Milky Way stellar predictions. Object coordinates are defined with an accuracy as good as ∼0.15" rms with respect to GSC 2.2; flux uncertainties are ∼2, 10, 20% at mag. 20, 23, 24 respectively (Vega); we reach 95% completeness at B, V∼25 and R∼24.5. ESIS galaxy number counts are in good agreement with previous works and are best reproduced by evolutionary and hierarchical Lambda-CDM scenarios. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file esisbvr.dat 649 132612 ESIS BVR catalog (magnitudes on the Vega scale) -------------------------------------------------------------------------------- See also: J/A+A/457/501 : XMM-Newton survey of the ELAIS-S1 field (Puccetti+, 2006) J/A+A/476/151 : SWIRE ELAIS-S1 IR-peak galaxy IR fluxes (Berta+, 2007) J/AJ/127/3075 : Mid-infrared population of ELAIS-S1 sample (La Franca+, 2004) Byte-by-byte Description of file: esisbvr.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 A5 --- --- [ESIS:] 6- 25 A20 --- ESIS ESIS designation (JHHMMSS.ss-DDMMSS.ss) 28- 40 F13.9 deg RAdeg Right ascension (J2000) 44- 56 F13.9 deg DEdeg Declination (J2000) 62- 67 F6.3 mag Bmag ?=99.99 Johnson "auto" B magnitude 73- 78 F6.3 mag e_Bmag ?=99.99 rms uncertainty on Bmag 84- 89 F6.3 mag Vmag ?=99.99 Johnson "auto" V magnitude 95-100 F6.3 mag e_Vmag ?=99.99 rms uncertainty on Vmag 106-111 F6.3 mag Rmag ?=99.99 Cousins "auto" R magnitude 117-122 F6.3 mag e_Rmag ?=99.99 rms uncertainty on Rmag 128-133 F6.3 mag BmagIso ?=99.99 Johnson B magnitude 139-144 F6.3 mag e_BmagIso ?=99.99 rms uncertainty on BmagIso 150-155 F6.3 mag VmagIso ?=99.99 Johnson V magnitude 161-166 F6.3 mag e_VmagIso ?=99.99 rms uncertainty on VmagIso 172-177 F6.3 mag RmagIso ?=99.99 Cousins R magnitude 183-188 F6.3 mag e_RmagIso ?=99.99 rms uncertainty on RmagIso 194-199 F6.3 mag BmagIsoc ?=99.99 Corrected Johnson B magnitude 205-210 F6.3 mag e_BmagIsoc ?=99.99 rms uncertainty on BmagIsocor 216-221 F6.3 mag VmagIsoc ?=99.99 Johnson V magnitude 227-232 F6.3 mag e_VmagIsoc ?=99.99 rms uncertainty on VmagIsocor 238-243 F6.3 mag RmagIsoc ?=99.99 Cousins R magnitude 249-254 F6.3 mag e_RmagIsoc ?=99.99 rms uncertainty on RmagIsocor 260-265 F6.3 mag BmagAp1 ?=99.99 Johnson B magnitude 271-276 F6.3 mag e_BmagAp1 ?=99.99 rms uncertainty on BmagAp1 282-287 F6.3 mag VmagAp1 ?=99.99 Johnson V magnitude 293-298 F6.3 mag e_VmagAp1 ?=99.99 rms uncertainty on VmagAp1 304-309 F6.3 mag RmagAp1 ?=99.99 Cousins R magnitude 315-320 F6.3 mag e_RmagAp1 ?=99.99 rms uncertainty on RmagAp1 326-331 F6.3 mag BmagAp2 ?=99.99 Johnson B magnitude 337-342 F6.3 mag e_BmagAp2 ?=99.99 rms uncertainty on BmagAp2 348-353 F6.3 mag VmagAp2 ?=99.99 Johnson V magnitude 359-364 F6.3 mag e_VmagAp2 ?=99.99 rms uncertainty on VmagAp2 370-375 F6.3 mag RmagAp2 ?=99.99 Cousins R magnitude 381-386 F6.3 mag e_RmagAp2 ?=99.99 rms uncertainty on RmagAp2 392-397 F6.3 mag BmagAp3 ?=99.99 Johnson B magnitude 403-408 F6.3 mag e_BmagAp3 ?=99.99 rms uncertainty on BmagAp3 414-419 F6.3 mag VmagAp3 ?=99.99 Johnson V magnitude 425-430 F6.3 mag e_VmagAp3 ?=99.99 rms uncertainty on VmagAp3 436-441 F6.3 mag RmagAp3 ?=99.99 Cousins R magnitude 447-452 F6.3 mag e_RmagAp3 ?=99.99 rms uncertainty on RmagAp3 458-463 F6.3 mag BmagAp4 ?=99.99 Johnson B magnitude 469-474 F6.3 mag e_BmagAp4 ?=99.99 rms uncertainty on BmagAp4 480-485 F6.3 mag VmagAp4 ?=99.99 Johnson V magnitude 491-496 F6.3 mag e_VmagAp4 ?=99.99 rms uncertainty on VmagAp4 502-507 F6.3 mag RmagAp4 ?=99.99 Cousins R magnitude 513-518 F6.3 mag e_RmagAp4 ?=99.99 rms uncertainty on RmagAp4 524-529 F6.3 mag BmagAp5 ?=99.99 Johnson B magnitude 535-540 F6.3 mag e_BmagAp5 ?=99.99 rms uncertainty on BmagAp5 546-551 F6.3 mag VmagAp5 ?=99.99 Johnson V magnitude 557-562 F6.3 mag e_VmagAp5 ?=99.99 rms uncertainty on VmagAp5 568-573 F6.3 mag RmagAp5 ?=99.99 Cousins R magnitude 579-584 F6.3 mag e_RmagAp5 ?=99.99 rms uncertainty on RmagAp5 589-594 F6.2 pix BFWHM ?=99.99 B band FWHM assuming a gaussian core 601-605 F5.2 --- S/GB ?=99.99 B band star/galaxy classifier output (0 for galaxy) 611-616 F6.2 pix VFWHM ?=99.99 V band FWHM assuming a gaussian core 623-627 F5.2 --- S/GV ?=99.99 V band star/galaxy classifier output (0 for galaxy) 634-639 F6.3 pix RFWHM ?=99.99 R band FWHM assuming a gaussian core 645-649 F5.2 --- S/GR ?=99.99 R band star/galaxy classifier output (0 for galaxy) -------------------------------------------------------------------------------- Acknowledgements: Stefano Berta, berta(at)mpe.mpg.de
(End) Patricia Vannier [CDS] 30-Jul-2008
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