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Soma Mukherjee

Researcher at University of Texas at Austin

Publications -  280
Citations -  72580

Soma Mukherjee is an academic researcher from University of Texas at Austin. The author has contributed to research in topics: LIGO & Gravitational wave. The author has an hindex of 95, co-authored 266 publications receiving 59549 citations. Previous affiliations of Soma Mukherjee include The University of Texas Rio Grande Valley & Saha Institute of Nuclear Physics.

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Median-based noise floor tracker (MNFT): robust estimation of noise floor drifts in interferometric data

TL;DR: In this paper, the median-based noise floor tracker (MNFT) was developed to track the slow drifts in the noise floor, which smoothes the data to eliminate transients in contrast to methods such as running mean, where transient interference cannot be removed.
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Upper limits on gravitational wave emission from 78 radio pulsars (Physical Review D - Particles, Fields, Gravitation and Cosmology (2007) 76, (042001))

B. P. Abbott, +455 more
- 10 Mar 2008 - 
TL;DR: In this paper, a formatting error in the fifty-first affiliation in the author list has been identified; the affiliation should read as ‘‘University of Western Australia, Crawley, WA 6009, Australia.
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A report on the status of the GEO 600 gravitational wave detector

TL;DR: GEO 600 as discussed by the authors is an interferometric gravitational wave detector with 600 m arms, which employs a dual-recycled optical scheme allowing its optical response to be tuned over a range of frequencies (from ~100 Hz to a few kHz).
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Towards a data and detector characterization robot for gravitational wave detectors

TL;DR: The first design steps towards building this detector characterization robot are presented along with some preliminary results and some possibilities for the future are outlined.
Journal Article

Search of the Orion spur for continuous gravitational waves using a loosely coherent algorithm on data from LIGO interferometers

J. Aasi, +945 more
TL;DR: In this article, the authors reported results of a wideband search for periodic gravitational waves from isolated neutron stars within the Orion spur towards both the inner and outer regions of our Galaxy, where the search is unimpeded by dust and concentrations of stars.