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T. Marsh

4 papers hereh-index 4178 citations7 works total

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

author position
  • middle author3
  • last author1

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

fields
  • astro-ph3
  • astro-ph.SR1
same name
  • T. Marsh — 304 papers, h 59
  • T. Marsh — 40 papers, h 20
  • T. Marsh — 29 papers, h 20
  • T. Marsh — 16 papers, h 6
  • T. Marsh — 3 papers, h 3
  • T. Marsh — 2 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
20012019
most citedSearch for progenitors of supnernovae type Ia with SPY

122 citations · 346 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR2019★ 91 cited

The ESO supernovae type Ia progenitor survey (SPY)

R. Napiwotzki, C. A. Karl, T. Lisker +13

Close double degenerate binaries are one of the favoured progenitor channels for type Ia supernovae, but it is unclear how many suitable systems there are in the Galaxy. We report…

astro-ph2005★ 104 cited

Binaries discovered by the SPY project. IV. Five single-lined DA double white dwarfs

G. Nelemans, R. Napiwotzki, C. Karl +8

We present results from our ongoing follow-up observations of double white dwarf binaries detected in the ESO SN Ia Progenitor SurveY (SPY). We discuss our observing strategy and d…

astro-ph2002★ 122 cited

Search for progenitors of supnernovae type Ia with SPY

R. Napiwotzki, N. Christlieb, H. Drechsel +13

We have started a large survey for double degenerate (DD) binaries as potential progenitors of type Ia supernovae with the UVES spectrograph at the ESO VLT (ESO SN Ia Progenitor su…

astro-ph2001★ 29 cited

The Quiescent Spectrum of the AM CVn star CP Eri

Paul J. Groot, Gijs Nelemans, Danny Steeghs +1

We used the 6.5m MMT to obtain a spectrum of the AM CVn star CP Eri in quiescence. The spectrum is dominated by He I emission lines, which are clearly double peaked with a peak-to-…

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