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A High Galactic Latitude HI 21cm-line Absorption Survey using the GMRT: I. Observations and Spectra

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dc.contributor.author Mohan, Rekhesh
dc.contributor.author Dwarakanath, K. S
dc.contributor.author Srinivasan, G
dc.date.accessioned 2008-09-11T16:04:41Z
dc.date.available 2008-09-11T16:04:41Z
dc.date.issued 2004-12
dc.identifier.citation Journal of Astrophysics and Astronomy, Vol. 25, No. 3 - 4, pp. 143 - 184 en
dc.identifier.issn 0250-6335
dc.identifier.uri http://hdl.handle.net/2248/3553
dc.description.abstract We 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.iso en en
dc.publisher Indian Academy of Sciences en
dc.relation.uri http://arxiv.org/abs/astro-ph/0410626 en
dc.relation.uri http://dx.doi.org/10.1007/BF02702370 en
dc.subject ISM: clouds en
dc.subject kinematics and dynamics - radio lines: ISM en
dc.title A High Galactic Latitude HI 21cm-line Absorption Survey using the GMRT: I. Observations and Spectra en
dc.type Article en


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