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researcher

N. F. Förster Schreiber

101 papers hereh-index 13596 citations26 works total

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

author position
  • sole author1
  • first author6
  • middle author80
  • last author2

Across the 89 of 101 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO46
  • astro-ph.GA46
  • astro-ph5
  • astro-ph.IM3
  • astro-ph.EP1
same name
  • N. F. Förster Schreiber — 28 papers, h 0
  • N. F. Förster Schreiber — 17 papers, h 34

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
20002026
most citedThe SINS survey: SINFONI Integral Field Spectroscopy of z ~ 2 Star-forming Galaxies

1.1k citations · 19.3k across the 99 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.GA2019★ 53 cited

Plateau de Bure High-z Blue-Sequence Survey 2 (PHIBSS2): Search for Secondary Sources, CO Luminosity Functions in the Field, and the Evolution of Molecular Gas Density through Cosmic Time

Laura Lenkić, Alberto D. Bolatto, Natascha M. Förster Schreiber +8

We report on the results of a search for serendipitous sources in CO emission in 110 cubes targeting CO(2-1), CO(3-2), and CO(6-5) at z ~ 1-2 from the second Plateau de Bure High-z…

astro-ph.GA2019★ 826 cited

A geometric distance measurement to the Galactic Center black hole with 0.3% uncertainty

R. Abuter, A. Amorim, M. Bauboeck +51

We present a 0.16% precise and 0.27% accurate determination of R0, the distance to the Galactic Center. Our measurement uses the star S2 on its 16-year orbit around the massive bla…

astro-ph.GA2019★ 59 cited

The MOSDEF Survey: Kinematic and Structural Evolution of Star-Forming Galaxies at 1.4≤z≤3.8

Sedona H. Price, Mariska Kriek, Guillermo Barro +15

We present ionized gas kinematics for 681 galaxies at z∼1.4−3.8 from the MOSFIRE Deep Evolution Field survey, measured using models which account for random galaxy-slit misal…

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