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S. Schulze

28 papers hereh-index 271.8k citations36 works total

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

author position
  • first author1
  • middle author18

Across the 19 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE13
  • astro-ph.GA8
  • astro-ph.SR7
same name
  • S. Schulze — 124 papers, h 54
  • S. Schulze — 49 papers, h 7
  • S. Schulze — 25 papers, h 15
  • S. Schulze — 25 papers, h 4
  • S. Schulze — 14 papers, h 16
  • S. Schulze — 7 papers, h 7

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
20142026
most citedPESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects

361 citations · 2.1k across the 27 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.GA2014

A young stellar environment for the superluminous supernova PTF12dam

C. C. Thöne, A. de Ugarte Postigo, R. García-Benito +3

The progenitors of super luminous supernovae (SLSNe) are still a mystery. Hydrogen-poor SLSN hosts are often highly star-forming dwarf galaxies and the majority belongs to the clas…

astro-ph.SR2014★ 361 cited

PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects

S. J. Smartt, S. Valenti, M. Fraser +99

The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction str…

astro-ph.GA2014★ 225 cited

Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies

G. Leloudas, S. Schulze, T. Kruehler +16

Superluminous supernovae (SLSNe) are very bright explosions that were only discovered recently and that show a preference for occurring in faint dwarf galaxies. Understanding why s…

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