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Clustering of High Redshift (Z>2.9) Quasars from the Sloan Digital Sky Survey / Shen, Yue ; Anderson, Scott F ; Bahcall, Neta A ; Berk, Daniel E Vanden ; Fan, Xiaohui ; Hall, Patrick B ; Hennawi, Joseph F ; Oguri, Masamune ; Richards, Gordon T ; Schneider, Donald P et al.
SLAC-PUB-12193. - 2006. - 21 p.
Fulltext from SLAC

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The Second Data Release of the Sloan Digital Sky Survey / SDSS Collaboration
The Sloan Digital Sky Survey has validated and made publicly available its Second Data Release. This data release consists of 3324 square degrees of five-band (u g r i z) imaging data with photometry for over 88 million unique objects, 367,360 spectra of galaxies, quasars, stars and calibrating blank sky patches selected over 2627 degrees of this area, and tables of measured parameters from these data. [...]
astro-ph/0403325; FERMILAB-PUB-04-360-A.- 2004 - 24 p. - Published in : Astron. J. 128 (2004) 502-512 Fulltext: PDF; External link: Fermilab Library Server (fulltext available)

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The First Data Release of the Sloan Digital Sky Survey / SDSS Collaboration
The Sloan Digital Sky Survey has validated and made publicly available its First Data Release. This consists of 2099 square degrees of five-band (u, g, r, i, z) imaging data, 186,240 spectra of galaxies, quasars, stars and calibrating blank sky patches selected over 1360 square degrees of this area, and tables of measured parameters from these data. [...]
astro-ph/0305492; FERMILAB-PUB-03-176-A.- Princeton, NJ : Princeton Univ., 2003 - 16 p. - Published in : Astron. J. 126 (2003) 2081 Access to fulltext document: 0305492.fig1 - PS.GZ; 0305492.fig3 - PS.GZ; 0305492.fig2 - PS.GZ; 0305492.fig5 - PS.GZ; 0305492.fig4 - PS.GZ; 0305492 - PDF; Fulltext: PDF; External link: Fermilab Library Server (fulltext available)

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Se också: liknande författarnamn
36	Hall, P
1	Hall, P A V
130	Hall, P B
11	Hall, P J
1	Hall, Pat
9	Hall, Patrick
1	Hall, Patrick A
2	Hall, Patrick B.
1	Hall, Payson
32	Hall, Peter
1	Hall, Peter Gavin
3	Hall, Peter J
2	Hall, Peter S
1	Hall, Philip
3	Hall, Philip D

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