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researcher

G. Khullar

4 papers here

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO2
  • astro-ph.GA1
  • astro-ph.HE1
same name
  • G. Khullar — 1 paper

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

most citedAn X-ray Detection of Star Formation In a Highly Magnified Giant Arc

11 citations · 11 across the 1 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2019

Strong Lensing Model of SPT-CLJ0356-5337, a Major Merger Candidate at Redshift 1.0359

Guillaume Mahler, Keren Sharon, Michael D. Gladders +10

We present an analysis of the mass distribution inferred from strong lensing by SPT-CL J0356-5337, a cluster of galaxies at redshift z = 1.0359 revealed in the follow-up of the SPT…

astro-ph.HE2019★ 11 cited

An X-ray Detection of Star Formation In a Highly Magnified Giant Arc

M. B. Bayliss, M. McDonald, K. Sharon +19

In the past decade, our understanding of how stars and galaxies formed during the first 5 billion years after the Big Bang has been revolutionized by observations that leverage gra…

astro-ph.CO2019

The SPTpol Extended Cluster Survey

L. E. Bleem, S. Bocquet, B. Stalder +135

We describe the observations and resultant galaxy cluster catalog from the 2770 deg2 SPTpol Extended Cluster Survey (SPT-ECS). Clusters are identified via the Sunyaev-Zel'dovich…

astro-ph.CO2019

Galaxy Clusters Selected via the Sunyaev-Zel'dovich Effect in the SPTpol 100-Square-Degree Survey

N. Huang, L. E. Bleem, B. Stalder +74

We present a catalog of galaxy cluster candidates detected in 100 square degrees surveyed with the SPTpol receiver on the South Pole Telescope. The catalog contains 89 candidates d…

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