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J/AJ/133/2222     Clustering of high-redshift QSOs from SDSS       (Shen+, 2007)

Clustering of high-redshift (z≥2.9) quasars from the Sloan Digital Sky Survey. Shen Y., Strauss M.A., Oguri M., Hennawi J.F., Fan X., Richards G.T., Hall P.B., Gunn J.E., Schneider D.P., Szalay A.S., Thakar A.R., Vanden Berk D.E., Anderson S.F., Bahcall N.A., Connolly A.J., Knapp G.R. <Astron. J., 133, 2222-2241 (2007)> =2007AJ....133.2222S
ADC_Keywords: Surveys ; QSOs ; Redshifts ; Photometry Keywords: cosmology: observations - large-scale structure of universe - quasars: general - surveys Abstract: We study the two-point correlation function of a uniformly selected sample of 4426 luminous optical quasars with redshift 2.9≤z≤5.4 selected over 4041deg2 from the Fifth Data Release of the Sloan Digital Sky Survey. We fit a power-law to the projected correlation function wp(rp) to marginalize over redshift-space distortions and redshift errors. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 58 5884 High Redshift Quasar Sample; with duplicate objects removed and a Redshift cut of z≥2.9
See also: II/276 : The SDSS Photometric Catalog, Release 5 (Adelman-McCarthy+, 2007) : SDSS Home Page Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 4 I4 --- Plate Plate number 6- 8 I3 --- Fiber Fiber identification number 10- 14 I5 --- MJD Modified Julian Date 16- 25 F10.6 deg RAdeg Right Ascension in decimal degrees (J2000) (1) 27- 36 F10.6 deg DEdeg Declination in decimal degrees (J2000) (1) 38- 42 F5.3 --- z Redshift (2) 44- 48 F5.3 --- e_z Error in z 50- 54 F5.2 mag imag Dereddened i band PSF (asinh) magnitude (3) 56 I1 --- Sfl [0/1] 1 indicates that the object is in the clustering subsample (4) 58 I1 --- Gfl [0/1] 1 indicates that the object is in the good imaging field
Note (1): Objects identified as [SSO2007] DDD.dddddd+DD.dddddd in Simbad. Note (2): Re-measured using line fitting procedures. Note (3): Corrected for Galactic extinction (Schlegel et al., 1998ApJ...500..525S); they use the ubercalibration described by Padmanabhan et al. (2007MNRAS.378..852P), which differs slightly from that used in the official DR5 quasar catalog (Schneider et al., 2007AJ....134..102S). Note (4): The subsample clustering analysis is 1) Selected from the Main SDSS survey with main target selection criteria 2) With target version v310 or later.
History: From electronic version of the journal
(End) Greg Schwarz [AAS], Patricia Vannier [CDS] 01-Apr-2009
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

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