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J. C. Kasper

21 papers hereh-index 15653 citations18 works total

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

author position
  • middle author19

Across the 19 of 21 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM12
  • astro-ph.CO3
  • astro-ph.GA2
  • astro-ph1
  • astro-ph.EP1
  • astro-ph.HE1
same name
  • J. C. Kasper — 3 papers

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
20062015
most citedGLEAM: The GaLactic and Extragalactic All-sky MWA survey

304 citations · 1.3k across the 20 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.CO2013★ 165 cited

A study of fundamental limitations to statistical detection of redshifted HI from the epoch of reionization

Nithyanandan Thyagarajan, N. Udaya Shankar, Ravi Subrahmanyan +46

In this paper we explore for the first time the relative magnitudes of three fundamental sources of uncertainty, namely, foreground contamination, thermal noise and sample variance…

astro-ph.IM2013★ 52 cited

On the detection and tracking of space debris using the Murchison Widefield Array. I. Simulations and test observations demonstrate feasibility

S. J. Tingay, D. L. Kaplan, B. McKinley +60

The Murchison Widefield Array (MWA) is a new low frequency interferomeric radio telescope. The MWA is the low frequency precursor to the Square Kilometre Array (SKA) and is the fir…

astro-ph.CO2013★ 102 cited

A 189 MHz, 2400 square degree polarization survey with the Murchison Widefield Array 32-element prototype

G. Bernardi, L. J. Greenhill, D. A. Mitchell +50

We present a Stokes I, Q and U survey at 189 MHz with the Murchison Widefield Array 32-element prototype covering 2400 square degrees. The survey has a 15.6 arcmin angular resoluti…

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