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dc.contributor.authorBlundell, K.M.
dc.contributor.authorSchechter, P.L.
dc.contributor.authorMorgan, N.D.
dc.contributor.authorJarvis, M.J.
dc.contributor.authorRawlings, S.
dc.contributor.authorTonry, J.L.
dc.date.accessioned2010-12-06T14:03:52Z
dc.date.available2010-12-06T14:03:52Z
dc.date.issued2010
dc.identifier.citationBlundell , K M , Schechter , P L , Morgan , N D , Jarvis , M J , Rawlings , S & Tonry , J L 2010 , ' A doubled double hot spot in J0816+5003 and the logarithmic slope of the lensing potential ' , The Astrophysical Journal , vol. 723 , no. 2 , pp. 1319-1324 . https://doi.org/10.1088/0004-637X/723/2/1319
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 158792
dc.identifier.otherPURE UUID: a570d12f-82f1-4944-938d-7f97b390dd46
dc.identifier.otherdspace: 2299/5059
dc.identifier.otherScopus: 78650124416
dc.identifier.urihttp://hdl.handle.net/2299/5059
dc.descriptionOriginal article can be found at: http://iopscience.iop.org/0004-637X/ Copyright American Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractWe present an analysis of observations of the doubly lensed double hot spot in the giant radio galaxy J0816+5003 from MERLIN, MDM, WIYN, WHT, UKIRT, and the VLA. The images of the two hot spot components span a factor of 2 in radius on one side of the lensing galaxy at impact parameters of less than 500 pc. Hence, we measure the slope of the lensing potential over a large range in radius, made possible by significant improvement in the accuracy of registration of the radio and optical frame and higher resolution imaging data than previously available. We also infer the lens and source redshifts to be 0.332 and ~1, respectively. Purely on the basis of lens modeling, and independently of stellar velocity dispersion measurements, we find the potential to be very close to isothermalen
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.titleA doubled double hot spot in J0816+5003 and the logarithmic slope of the lensing potentialen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1088/0004-637X/723/2/1319
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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