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N. Nesvadba

115 papers hereh-index 426.5k citations184 works total

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

author position
  • sole author1
  • first author16
  • middle author73
  • last author9

Across the 99 of 115 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA66
  • astro-ph.CO29
  • astro-ph17
  • astro-ph.IM2
  • astro-ph.HE1
same name
  • N. Nesvadba — 8 papers, 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
20042026
most citedSINFONI Integral Field Spectroscopy of z~2 UV-selected Galaxies: Rotation Curves and Dynamical Evolution

482 citations · 6.8k across the 113 of their papers we have counts for

collaborators
Showing 2017Show all

3 papers · 1 filter

astro-ph.GA2017★ 41 cited

Planck's dusty GEMS. IV. Star formation and feedback in a maximum starburst at z=3 seen at 60-pc resolution

R. Canameras, N. Nesvadba, R. Kneissl +7

We present an analysis of high-resolution ALMA interferometry of CO(4-3) line emission and dust continuum in the "Ruby" (PLCK_G244.8+54.9), a bright, gravitationally lensed galaxy…

astro-ph.GA2017★ 23 cited

Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5

R. Canameras, N. P. H. Nesvadba, R. Kneissl +8

We study the properties of the foreground galaxy of the Ruby, the brightest gravitationally lensed high-redshift galaxy on the sub-millimeter sky as probed by the Planck satellite,…

astro-ph.GA2017★ 21 cited

SCUBA-2 follow-up of Herschel-SPIRE observed Planck overdensities

Todd P. MacKenzie, Douglas Scott, Matteo Bianconi +11

We present SCUBA-2 follow-up of 61 candidate high-redshift Planck sources. Of these, 10 are confirmed strong gravitational lenses and comprise some of the brightest such submm sour…

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