J/ApJS/119/189           Deep Multicolor Survey. IV.  (Osmer+ 1998)

A Deep Multicolor Survey. IV. The Electronic Stellar Catalog Osmer P.S., Kennefick, J.D., Hall P.B., Green R.F. <Astrophys. J. Suppl. Ser. 119, 189 (1998)> =1998ApJS..119..189O 1998ApJS..119..189O
ADC_Keywords: QSOs ; Galaxies, photometry ; Surveys Keywords: catalogs - galaxies: compact - quasars: general - stars: general - surveys Description: This stellar catalog contains 19,494 objects from the Deep Multicolor Survey (DMS) and results from follow-up spectroscopic observations of 234 objects in the catalog. The DMS is based on CCD imaging with the Mayall 4 m telescope in U, B, V, R', I75, and I86 and covers 0.83 deg^2 in six fields at high Galactic latitude. The survey reached 5 sigma limiting magnitudes of 22.1 in I86 to 23.8 in B. The catalog gives positions, magnitudes and error estimates, and classification codes in the six filter bands for all the objects. In addition, the survey is useful for the study of faint field galaxies and of faint stars at high Galactic latitude. Presented are tables that summarize the spectroscopic results for the 55 quasars, 44 compact narrow emission-line galaxies, and 135 stars in the DMS that we have confirmed to date. Also included are illustrations of all the spectra. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file field01h.dat 190 2299 Field 01h of the Deep Multicolor Survey field10h.dat 190 1441 Field 10h of the Deep Multicolor Survey field14h.dat 190 3528 Field 14h of the Deep Multicolor Survey field17h.dat 190 4417 Field 17h of the Deep Multicolor Survey field21h.dat 190 4462 Field 21h of the Deep Multicolor Survey field22h.dat 190 3347 Field 22h of the Deep Multicolor Survey table1.dat 113 55 Spectroscopically Identified Quasars table1.ps 72 732 Postscript version of table1 table2.dat 113 44 Spectroscopically Identified Compact Narrow Emission-Line Galaxies table2.ps 72 641 Postscript version of table2 table3.dat 137 135 Spectroscopically Identified Stars table3.ps 72 1051 Postscript version of table3 fig1.ps 88 1895 *Observed differential source counts fig2.ps 80 2007 *Log of the cumulative source counts fig3.ps 80 19963 V vs. B-V color-magnitude diagram for the stellar objects on the DMS -------------------------------------------------------------------------------- Note on fig1.ps and fig2.ps: Counts for the stellar objects in three different filters: B, V, R' See also: J/ApJS/104/185 : A deep multicolor survey. I. (Hall+ 1996) J/ApJ/462/614 : A deep multicolor survey. II (Hall+ 1996) J/AJ/114/2269 : A deep multicolor survey. III (Kennefick+ 1997) Byte-by-byte Description of file: field*.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 I4 --- No Sequential number 6- 8 A3 --- Field Field designation 10- 11 I2 h RAh Right ascension (1950.0) 13- 14 I2 min RAm Right ascension (1950.0) 16- 20 F5.2 s RAs Right ascension (1950.0) 22 A1 --- DE- Declination sign 23- 24 I2 deg DEd Declination (1950.0) 26- 27 I2 arcmin DEm Declination (1950.0) 29- 33 F5.2 arcsec DEs Declination (1950.0) 35- 41 F7.2 pix x x coordinates on the image 43- 49 F7.2 pix y y coordinates on the image 51- 56 F6.3 mag Umag U magnitude 58- 63 F6.3 mag e_Umag *[-.333,.333] error estimate for U magnitude 65- 70 F6.3 mag Bmag B magnitude 72- 77 F6.3 mag e_Bmag *[-.333,.333] error estimate for B magnitude 79- 84 F6.3 mag Vmag V magnitude 86- 91 F6.3 mag e_Vmag *[-.333,.333] error estimate for V magnitude 93- 98 F6.3 mag Rmag R magnitude 100-105 F6.3 mag e_Rmag *[-.333,.333] error estimate for R magnitude 107-112 F6.3 mag I75mag I75 magnitude 114-119 F6.3 mag e_I75mag *[-.333,.333] error estimate for I75 magnitude 121-126 F6.3 mag I86mag I86 magnitude 128-133 F6.3 mag e_I86mag *[-.333,.333] error estimate for I86 magnitude 135-136 A2 --- u1 *U magnitude filter classification code 138-139 A2 --- u2 *U magnitude image classification code 141-142 A2 --- b1 *B magnitude filter classification code 144-145 A2 --- b2 *B magnitude image classification code 147-148 A2 --- v1 *V magnitude filter classification code 150-151 A2 --- v2 *V magnitude image classification code 153-154 A2 --- r1 *R magnitude filter classification code 156-157 A2 --- r2 *R magnitude image classification code 159-160 A2 --- i1 *I75 magnitude filter classification code 162-163 A2 --- i2 *I75 magnitude image classification code 165-166 A2 --- I1 *I86 magnitude filter classification code 168-169 A2 --- I2 *I86 magnitude image classification code 171-190 A20 --- Comments *Comments on individual objects ------------------------------------------------------------------------------- Note on e_Umag, e_Bmag, e_Vmag, e_Rmag, e_I75mag, e_I86mag: Error of 0.333 mag means that the magnitude value corresponds to the 3 sigma limit for that object. Also, an error value of -0.333 indicates that the object should have been detected in one of the frames but was not. Thus the measurement is being flagged as possibly subject to a non-statistical error. Note on u1, u2, b1, b2, v1, v2, r1, r2, i1, i2, I1, I2: Refer to object classification codes from FOCAS for each filter and image. The codes are: s = star sf = fuzzy star Fs = forced star g = galaxy n = noise d = diffuse object l = long object u = unknown (not detected by FOCAS in both images of that field) x = no image available When an object was classified as a star in either or both images of a field, its classification was forced to star in each image - thus the Fs classification. No information was retained on the original classification in each image. An exception is objects used as PSF templates; these objects already had a "forced" flag present in FOCAS, and so the original classification was not overwritten. Most cases of "s" or "sf" in the catalog are objects of this sort. The other exceptions are all filters in the 01e and the B filter in the 10e field, for which only one image was available. In these cases, the classifications given are the original FOCAS classifications. Note on Comments: Contains comments on individual objects. The codes are: q = quasar c = CNELG (compact narrow emission-line galaxy) s = star u = unknown (spectrum has too low S/N ratio to classify) The number following "q" or "c" is the redshift, with a "?" indicating an uncertain or unknown redshift. Other codes include "cr" for cosmic ray and "bp" for bad pixel followed by a filter and/or offset image code; i.e., "cr,u1" means a cosmic ray contaminates the object in the first U image. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat, table2.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 14 A14 --- Name Quasars (table1.dat) and CNELG (table2.dat) 16- 23 A8 --- ID Running number for the object and field identifier 25- 29 F5.3 --- z ? Redshift 30 A1 --- u_z [?] Uncertainty flag on z 31- 36 F6.3 mag Umag U magnitude 38- 43 F6.3 mag e_Umag *[-.333,.333] error estimate for U magnitude 45- 50 F6.3 mag Bmag B magnitude 52- 57 F6.3 mag e_Bmag *[-.333,.333] error estimate for B magnitude 59- 64 F6.3 mag Vmag V magnitude 66- 71 F6.3 mag e_Vmag *[-.333,.333] error estimate for V magnitude 73- 78 F6.3 mag Rmag R magnitude 80- 85 F6.3 mag e_Rmag *[-.333,.333] error estimate for R magnitude 87- 92 F6.3 mag I75mag I75 magnitude 94- 99 F6.3 mag e_I75mag *[-.333,.333] error estimate for I75 magnitude 101-106 F6.3 mag I86mag I86 magnitude 108-113 F6.3 mag e_I86mag *[-.333,.333] error estimate for I86 magnitude -------------------------------------------------------------------------------- Note on e_Umag, e_Bmag, e_Vmag, e_Rmag, e_I75mag, e_I86mag: Error of 0.333 mag means that the magnitude value corresponds to the 3 sigma limit for that object. Also, an error value of -0.333 indicates that the object should have been detected in one of the frames but was not. Thus the measurement is being flagged as possibly subject to a non-statistical error. -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- ID Catalog Identification number 10- 15 F6.3 mag Umag U magnitude 17- 22 F6.3 mag e_Umag *[-.333,.333] error estimate for U magnitude 24- 29 F6.3 mag Bmag B magnitude 31- 36 F6.3 mag e_Bmag *[-.333,.333] error estimate for B magnitude 38- 43 F6.3 mag Vmag V magnitude 45- 50 F6.3 mag e_Vmag *[-.333,.333] error estimate for V magnitude 52- 57 F6.3 mag Rmag R magnitude 59- 64 F6.3 mag e_Rmag *[-.333,.333] error estimate for R magnitude 66- 71 F6.3 mag I75mag I75 magnitude 73- 78 F6.3 mag e_I75mag *[-.333,.333] error estimate for I75 magnitude 80- 85 F6.3 mag I86mag I86 magnitude 87- 92 F6.3 mag e_I86mag *[-.333,.333] error estimate for I86 magnitude 94-137 A44 --- Comments Comments on the spectral features or type of the star ------------------------------------------------------------------------------- Note on e_Umag, e_Bmag, e_Vmag, e_Rmag, e_I75mag, e_I86mag: Error of 0.333 mag means that the magnitude value corresponds to the 3 sigma limit for that object. Also, an error value of -0.333 indicates that the object should have been detected in one of the frames but was not. Thus the measurement is being flagged as possibly subject to a non-statistical error. -------------------------------------------------------------------------------- Acknowledgements: Copied in May 1999 from ftp://ftp.astronomy.ohio-state.edu/pub/posmer/DMS4/ Patrick S. Osmer
(End) Gail L. Schneider [ADC/SSDOO] 11-Jun-1999
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