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dc.contributorVirginia Tech
dc.contributor.authorSalgado, J. F.
dc.contributor.authorAltschuler, D. R.
dc.contributor.authorGhosh, T.
dc.contributor.authorDennison, B. K.
dc.contributor.authorMitchell, K. J.
dc.contributor.authorPayne, H. E.
dc.date.accessioned2014-03-10T13:18:52Z
dc.date.available2014-03-10T13:18:52Z
dc.date.issued1999-01
dc.identifier.citationJosé Francisco Salgado et al. 1999 ApJS 120 77 doi:10.1086/313169
dc.identifier.issn0067-0049
dc.identifier.urihttp://hdl.handle.net/10919/25860
dc.description.abstractWe present the results of a low-frequency flux density monitoring program of 33 extragalactic radio sources. The light curves at 318 and 430 MHz over a 14 yr period are presented. The measurements were made with the NAIC Arecibo 305 m radio telescope at approximately bimonthly intervals between 1980 January and 1989 February and at less regular intervals between 1989 October and 1993 October, for a total of 64 observing sessions. In addition, we provide a first discussion of the results, pointing out several source properties and interesting objects.
dc.description.sponsorshipNSF AST 81-17864, AST 87-15532
dc.language.isoen_US
dc.publisherIOP PUBLISHING LTD
dc.subjectISM, general
dc.subjectquasars, general
dc.subjectradio continuum, galaxies
dc.subjectvariability
dc.subjectspectrum
dc.subjectjets
dc.title14-year program monitoring the flux densities of 33 radio sources at low frequencies
dc.typeArticle - Refereed
dc.identifier.urlhttp://iopscience.iop.org/0067-0049/120/1/77
dc.date.accessed2014-02-28
dc.title.serialAstrophysical Journal Supplement Series
dc.identifier.doihttps://doi.org/10.1086/313169


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