The Angular Two Point Correlation Function for the FIRST Radio Survey - Initial Results

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dc.creatorCress, C. M.
dc.creatorHelfand, D. J.
dc.creatorBecker, R. H.
dc.creatorWhite, R. L.
dc.creatorGregg, M. D.
dc.date1995-09-07
dc.date1995-09-08
dc.date.accessioned2026-07-07T08:58:20Z
dc.date.available2026-07-07T08:58:20Z
dc.descriptionThe angular two-point correlation function is calculated for the first 300 square degrees of the FIRST radio survey. Results for various subsamples are also obtained. Double-lobed sources are shown to have a higher clustering amplitude than the sample as a whole. Small differences in the correlation function from one region of the sample to another and results of various flux cuts are discussed.
dc.description3 pages latex, 1 page postscript figures, uses paspconf.sty
dc.identifierhttps://arxiv.org/abs/astro-ph/9509043
dc.identifierhttp://arxiv.org/abs/astro-ph/9509043
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147288
dc.subjectAstrophysics
dc.titleThe Angular Two Point Correlation Function for the FIRST Radio Survey - Initial Results
dc.typetext

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