Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3553
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dc.contributor.authorMohan, Rekhesh-
dc.contributor.authorDwarakanath, K. S-
dc.contributor.authorSrinivasan, G-
dc.date.accessioned2008-09-11T16:04:41Z-
dc.date.available2008-09-11T16:04:41Z-
dc.date.issued2004-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 25, No. 3 - 4, pp. 143 - 184en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3553-
dc.description.abstractWe have used the Giant Meterwave Radio Telescope (GMRT) to measure the Galactic HI 21-cm line absorption towards 102 extragalactic radio continuum sources, located at high (|b| > 15?) Galactic latitudes. The Declination coverage of the present survey is δ - 45?.With a mean rms optical depth of ? 0.003, this is the most sensitive Galactic HI 21- cm line absorption survey to date. To supplement the absorption data, we have extracted the HI 21-cm line emission profiles towards these 102 lines of sight from the Leiden Dwingeloo Survey of Galactic neutral hydrogen. We have carried out a Gaussian fitting analysis to identify the discrete absorption and emission components in these profiles. In this paper, we present the spectra and the components. A subsequent paper will discuss the interpretation of these results.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://arxiv.org/abs/astro-ph/0410626en
dc.relation.urihttp://dx.doi.org/10.1007/BF02702370en
dc.subjectISM: cloudsen
dc.subjectkinematics and dynamics - radio lines: ISMen
dc.titleA High Galactic Latitude HI 21cm-line Absorption Survey using the GMRT: I. Observations and Spectraen
dc.typeArticleen
Appears in Collections:IIAP Publications



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