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V. Gupta

4 papers hereh-index 7252 citations17 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author1
  • last author1

Across the 2 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.IM2
same name
  • V. Gupta — 12 papers, h 40
  • V. Gupta — 6 papers, h 8
  • V. Gupta — 4 papers, h 6
  • V. Gupta — 3 papers
  • V. Gupta — 2 papers, h 3
  • V. Gupta — 2 papers, h 42

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20182020
most citedFive new real-time detections of Fast Radio Bursts with UTMOST

65 citations · 110 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.IM2020★ 29 cited

A magnetar parallax

H. Ding, A. T. Deller, M. E. Lower +7

XTE J1810-197 (J1810) was the first magnetar identified to emit radio pulses, and has been extensively studied during a radio-bright phase in 2003−2008. It is estimated to be rel…

astro-ph.IM2019

The UTMOST Survey for Magnetars, Intermittent pulsars, RRATs and FRBs I: System description and overview

V. Venkatraman Krishnan, C. Flynn, W. Farah +22

We describe the ongoing `Survey for Magnetars, Intermittent pulsars, Rotating radio transients and Fast radio bursts' (SMIRF), performed using the newly refurbished UTMOST telescop…

astro-ph.HE2019★ 65 cited

Five new real-time detections of Fast Radio Bursts with UTMOST

W. Farah, C. Flynn, M. Bailes +25

We detail a new fast radio burst (FRB) survey with the Molonglo Radio Telescope, in which six FRBs were detected between June 2017 and December 2018. By using a real-time FRB detec…

astro-ph.HE2018★ 16 cited

Hunting for radio emission from the intermittent pulsar J1107-5907 at low frequencies

B. W. Meyers, S. E. Tremblay, N. D. R. Bhat +30

The rare intermittent pulsars pose some of the most challenging questions surrounding the pulsar emission mechanism, but typically have relatively minimal low-frequency (≲…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.