J/A+A/568/A46   High redshift cosmic web with quasar systems   (Einasto+, 2014)

Tracing a high redshift cosmic web with quasar systems. Einasto M., Tago E., Lietzen H., Park C., Heinamaki P., Saar E., Song H., Liivamaki L.J., Einasto J. <Astron. Astrophys. 568, A46 (2014)> =2014A&A...568A..46E 2014A&A...568A..46E
ADC_Keywords: QSOs ; Redshifts ; Photometry, SDSS Keywords: cosmology: large-scale structure of the Universe - quasars: general Abstract: To understand the formation, evolution, and present-day properties of the cosmic web we need to study it at low and high redshifts. We trace the cosmic web at redshifts 1.0<z<1.8 using the quasar (QSO) data from in the SDSS DR7 QSO catalogue. We apply a friend-of-friend (FoF) algorithm to the quasar and random catalogues to determine systems at a series of linking length, and analyse richness and sizes of these systems. At the linking lengths l≤30Mpc/h, the number of quasar systems is larger than the number of systems detected in random catalogues, and the systems themselves have smaller diameters than random systems. The diameters of quasar systems are comparable to the sizes of poor galaxy superclusters in the local Universe. The richest quasar systems have four members. The mean space density of quasar systems is close to the mean space density of local rich superclusters. At intermediate linking lengths (40≤l≤70Mpc/h), the richness and length of quasar systems are similar to those derived from random catalogues. Quasar system diameters are similar to the sizes of rich superclusters and supercluster chains in the local Universe. The percolating system, which penetrate the whole sample volume appears in a quasar sample at a smaller linking length than in random samples (85Mpc/h). At the linking length 70Mpc/h, the richest systems of quasars have diameters exceeding 500Mpc. Quasar luminosities in systems are not correlated with the system richness. Quasar system catalogues in our web pages and at the Strasbourg Astronomical Data Center (CDS) serve as a database for searching for superclusters of galaxies and for tracing the cosmic web at high redshifts. Description: We present quasar system catalogues based on SDSS DR7 QSO catalogue (Schneider et al., 2010AJ....139.2360S 2010AJ....139.2360S, Cat. VII/260) File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file qso20all.dat 136 1207 Quasar table in systems at linking length 20Mpc qso30all.dat 136 3348 Quasar table in systems at linking length 30Mpc qso40all.dat 136 6516 Quasar table in systems at linking length 40Mpc qso50all.dat 136 10543 Quasar table in systems at linking length 50Mpc qso60all.dat 136 14450 Quasar table in systems at linking length 60Mpc qso70all.dat 136 17864 Quasar table in systems at linking length 70Mpc qso80all.dat 136 22381 Quasar table in systems at linking length 80Mpc qso20fof.dat 80 593 Quasar system table at linking length 20Mpc qso30fof.dat 80 1590 Quasar system table at linking length 30Mpc qso40fof.dat 80 2852 Quasar system table at linking length 40Mpc qso50fof.dat 80 4064 Quasar system table at linking length 50Mpc qso60fof.dat 80 4536 Quasar system table at linking length 60Mpc qso70fof.dat 80 3885 Quasar system table at linking length 70Mpc qso80fof.dat 80 2222 Quasar system table at linking length 80Mpc -------------------------------------------------------------------------------- See also: VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010) J/A+AS/123/119 : The supercluster-void network. I. (Einasto+ 1997) J/A+A/540/A123 : Galaxy clusters from SDSS DR8 (Einasto+, 2012) J/A+A/542/A36 : Rich clusters from SDSS DR8 (Einasto+, 2012) J/A+A/566/A1 : Flux- & volume-limited groups for SDSS galaxies (Tempel+ 2014) Byte-by-byte Description of file: qso??all.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 5 I5 --- IDqso [61/25011] ID of quasar (our list number) 7- 10 I4 --- IDsys [0/4536] ID of quasar system 12- 14 I3 --- Nqso [1/920] Number of quasars in the system 16- 25 F10.6 deg RAdeg Right ascension of a quasar (J2000) 27- 42 F16.12 deg DEdeg Declination of a quasar (J2000) 44- 60 F17.13 deg lambda [-55/55] SDSS Survey coordinate of a quasar 62- 76 F15.11 deg eta [-33/35] SDSS Survey coordinate of a quasar 78- 87 F10.8 --- zqso [1/1.8] Redshift of a quasar 89- 98 F10.7 mag imag i-magnitude of quasar 100-117 I18 --- Best SDSS-DR7 BestObjID 119-136 I18 --- Spec SDSS-DR7 SpecObjID ------------------------------------------------------------------------------- Byte-by-byte Description of file: qso??fof.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 I7 --- IDsys [1/4536] ID of quasar system 8- 14 I7 --- Nqso [2/920] Number of quasars in the system 15- 26 F12.6 deg RAdeg Right ascension of the system centre (J2000) 27- 38 F12.6 deg DEdeg Declination of the system centre (J2000) 39- 50 F12.6 deg lambda SDSS Survey coordinate of the system centre 51- 62 F12.6 deg eta SDSS Survey coordinate of the system centre 63- 71 F9.1 Mpc Dist Co-moving distance of a system centre (1) 72- 80 F9.1 Mpc Diam [1/2067] Diameter of a system (1) ------------------------------------------------------------------------------- Note (1): Distances in Mpc/h, where the cosmological parameters are: h=H0/100, Ωm=0.27, ΩΛ=0.73. ------------------------------------------------------------------------------- Acknowledgements: Maret Einasto, maret.einasto(at)to.ee History: * 12-Aug-2014: on-line version * 13-Oct-2014: corrected qso*all.dat files (from author)
(End) Maret Einasto [Tartu Obs., Estonia], Patricia Vannier [CDS] 03-Jul-2014
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