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researcher

H. Dannerbauer

100 papers hereh-index 6916.2k citations357 works total

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

author position
  • first author5
  • middle author52
  • last author5

Across the 62 of 100 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA85
  • astro-ph6
  • astro-ph.CO6
  • astro-ph.IM3
same name
  • H. Dannerbauer — 40 papers
  • H. Dannerbauer — 5 papers, h 5
  • H. Dannerbauer — 1 paper, h 2
  • H. Dannerbauer — 1 paper
  • H. Dannerbauer — 1 paper

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
20042024
most citedAn ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling

485 citations · 4k across the 73 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.GA2015★ 485 cited

An ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling

Elisabete da Cunha, Fabian Walter, Ian Smail +15

[abridged] The ALESS survey has followed-up a sample of 122 sub-millimeter sources in the Extended Chandra Deep Field South at 870um with ALMA, allowing to pinpoint the positions o…

astro-ph.GA2015★ 31 cited

A multi-wavelength exploration of the [CII]/IR ratio in H-ATLAS/GAMA galaxies out to z=0.2

E. Ibar, M. A. Lara-López, R. Herrera-Camus +23

We explore the behaviour of [CII]-157.74um forbidden fine-structure line observed in a sample of 28 galaxies selected from ~50deg^2 of the H-ATLAS survey. The sample is restricted…

astro-ph.GA2015★ 60 cited

A direct constraint on the gas content of a massive, passively evolving elliptical galaxy at z = 1.43

Mark T. Sargent, E. Daddi, F. Bournaud +6

Gas and dust in star-forming galaxies at the peak epoch of galaxy assembly are presently the topic of intense study, but little is known about the interstellar medium (ISM) of dist…

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