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researcher

G. Hasinger

57 papers hereh-index 398.8k citations331 works total

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

author position
  • first author2
  • middle author39
  • last author8

Across the 49 of 57 papers where every author was matched, so the position is known.

fields
  • astro-ph35
  • astro-ph.CO15
  • astro-ph.GA6
  • astro-ph.IM1
same name
  • G. Hasinger — 66 papers, h 32
  • G. Hasinger — 51 papers, h 44
  • G. Hasinger — 43 papers, h 36
  • G. Hasinger — 31 papers, h 28
  • G. Hasinger — 29 papers, h 6
  • G. Hasinger — 5 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
19952021
most citedMass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

2k citations · 5.9k across the 56 of their papers we have counts for

collaborators
Showing 2005Show all

4 papers · 1 filter

astro-ph2005★ 1 cited

Extending the X-ray luminosity function of AGN to high redshift

J. Silverman, P. Green, W. Barkhouse +6

X-ray surveys of the extragalactic universe are now able to detect significant numbers of AGN out to high redshift (z~5). We highlight some results from the Chandra Multiwavelength…

astro-ph2005

X-RED: A Satellite Mission Concept To Detect Early Universe Gamma Ray Bursts

Mirko Krumpe, Deirdre Coffey, Georg Egger +14

Gamma ray bursts (GRBs) are the most energetic eruptions known in the Universe. Instruments such as Compton-GRO/BATSE and the GRB monitor on BeppoSAX have detected more than 2700 G…

astro-ph2005★ 22 cited

SIMBOL-X, a formation flying-mission for hard X-ray astrophysics

P. Ferrando, A. Goldwurm, P. Laurent +13

SIMBOL-X is a hard X-ray mission, operating in the ~ 0.5-70 keV range, which is proposed by a consortium of European laboratories in response to the 2004 call for ideas of CNES for…

astro-ph2005

Signs of WHIM in the soft X-ray background

A. M. Soltan, M. J. Freyberg, G. Hasinger

Small angular scale structure of the soft X-ray background correlated with the galaxy distribution is investigated. An extensive data sample from the ROSAT and XMM-Newton archives…

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