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Jayant Murthy

Researcher at Indian Institute of Astrophysics

Publications -  156
Citations -  2054

Jayant Murthy is an academic researcher from Indian Institute of Astrophysics. The author has contributed to research in topics: Interstellar medium & Stars. The author has an hindex of 24, co-authored 150 publications receiving 1837 citations. Previous affiliations of Jayant Murthy include Johns Hopkins University Applied Physics Laboratory & Johns Hopkins University.

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A compilation of interstellar column densities

TL;DR: In this paper, the absorption line data toward 3008 stars was collated in order to create a unified database of interstellar column densities, and the preliminary results from their analysis show a tight relation [N(H)/E(B - V) = 6.12 Multiplication-Sign 10{sup 21}] between N(H) and E(B-V).
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Science with a Wide-field UV Transient Explorer

TL;DR: In this paper, the potential scientific impact of a wide-field UV survey on the study of explosive and other transient events, as well as known classes of variable objects, such as active galactic nuclei and variable stars, is reviewed.
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Science with a wide-field UV transient explorer

TL;DR: In this article, the potential scientific impact of a wide-field UV survey on the study of explosive and other transient events, as well as known classes of variable objects, such as active galactic nuclei and variable stars, was reviewed.
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Probing the role of carbon in ultraviolet extinction along galactic sight lines

TL;DR: This paper reported previously undetermined interstellar gas and dust-phase carbon abundances along 15 Galactic sight lines based on archival data of the strong 1334.5323 A transition observed with the Space Telescope Imaging Spectrograph.
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Lyman-Alpha Absorption and the D/H Ratio in the Local Interstellar Medium*

TL;DR: Using the Goddard High Resolution Spectrograph onboard the Hubble Space Telescope, this article observed Lyα absorption against stellar chromospheres along six lines of sight, with additional observations of the Mg II H and K lines along five of the lines of view and Fe II absorption along four of the line of sight.