Clustering in the quasar distribution

Details Clustering in the quasar distribution Clustering in the quasar distribution

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986acasn..27..144h&link_type=abstract

(Acta Astronomica Sinica, vol. 27, 1986, p. 144-150) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 10, Sept. 1986, p

Astronomy and Astrophysics

Astrophysics

3

Mass Distribution, Quasars, Data Sampling, Power Spectra, Red Shift

Scientific paper

Three objective-prism plates and one direct plate centred at 01h44mand -40°00arcmin were taken. 1092 quasar candidates were picked up in the 40 square degree field. The two-dimensional power spectrum analysis method is adopted to test the clustering of quasar candidates in the field. The intervals of reciprocal wavelength are Δ(1/λ) = 0.2. The clustering scale is about 0.5 degree. If one takes the average redshift Z = 2, the diameter of the supercluster is about 35 Mpc.

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