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researcher

E. Nagel

33 papers hereh-index 9508 citations35 works total

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

author position
  • first author2
  • middle author25

Across the 27 of 33 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP21
  • astro-ph.SR11
  • astro-ph.IM1
same name
  • E. Nagel — 57 papers, h 22
  • E. Nagel — 13 papers, h 9
  • E. Nagel — 2 papers, h 4
  • E. Nagel — 2 papers, h 84
  • E. Nagel — 1 paper, h 0
  • E. Nagel — 1 paper, h 3

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
20172026
most citedThe CARMENES search for exoplanets around M dwarfs: High-resolution optical and near-infrared spectroscopy of 324 survey stars

253 citations · 911 across the 33 of their papers we have counts for

collaborators
Showing 2023Show all

3 papers · 1 filter

astro-ph.SR2023★ 23 cited

The CARMENES search for exoplanets around M dwarfs. Telluric absorption corrected high S/N optical and near-infrared template spectra of 382 M dwarf stars

E. Nagel, S. Czesla, A. Kaminski +22

Light from celestial objects interacts with the molecules of the Earth's atmosphere, resulting in the production of telluric absorption lines in ground-based spectral data. Correct…

astro-ph.SR2023★ 10 cited

The CARMENES search for exoplanets around M dwarfs. Behaviour of the Paschen lines during flares and quiescence

B. Fuhrmeister, S. Czesla, J. H. M. M. Schmitt +17

The hydrogen Paschen lines are known activity indicators, but studies of them in M~dwarfs during quiescence are as rare as their reports in flare studies. This situation is mostly…

astro-ph.EP2023★ 32 cited

The CARMENES search for exoplanets around M dwarfs, Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star

D. Kossakowski, M. Kürster, T. Trifonov +47

We present the discovery of an Earth-mass planet (Mb​sini=1.26±0.21M⊕​) on a 15.6d orbit of a relatively nearby (d∼9.6pc) and low-mass (0.167±0.011M⊙​) M…

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