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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 1996Show all

4 papers · 1 filter

astro-ph1996★ 1 cited

The X-ray lightcurve of SN 1987A

G. Hasinger, B. Aschenbach, J. Trümper

X-ray observations of SN 1987A in the Magellanic Clouds have been performed throughout the ROSAT mission, using the PSPC and the HRI detectors. We present the X-ray light curve bas…

astro-ph1996

The Long-Term X-Ray Lightcurve of RX J0527.8-6954

J. Greiner, R. Schwarz, G. Hasinger +1

We present further observational data of the supersoft X-ray source RX J0527.8-6954 exhibiting a continuous decline over the past 5 yrs. With no clear trend of a concordant tempera…

astro-ph1996★ 31 cited

Optical and X-ray properties of the RIXOS AGN: I - The continua

E. M. Puchnarewicz, K. O. Mason, E. Romero-Colmenero +6

We present measurements of the optical and X-ray continua of 108 AGN (Seyfert 1s and quasars) from the Rosat International X-ray/Optical Survey (RIXOS). The sample covers a wide ra…

astro-ph1996★ 4 cited

The long-term X-ray lightcurve of RX J0527.8--6954

J. Greiner, R. Schwarz, G. Hasinger +1

Supersoft X-ray sources are commonly believed to be stably burning white dwarfs. However, the observations of some supersoft sources show dramatic variability of their X-ray flux o…

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