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researcher

C. Kramer

160 papers hereh-index 6117.7k citations329 works total

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

author position
  • first author6
  • middle author110
  • last author9

Across the 125 of 160 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA80
  • astro-ph.CO42
  • astro-ph17
  • astro-ph.IM9
  • astro-ph.HE5
  • gr-qc4
same name
  • C. Kramer — 45 papers, h 27
  • C. Kramer — 43 papers, h 7
  • C. Kramer — 14 papers, h 7
  • C. Kramer — 3 papers, h 5
  • C. Kramer — 3 papers, h 9
  • C. Kramer — 3 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
19982023
most citedFirst M87 Event Horizon Telescope Results. II. Array and Instrumentation

1.1k citations · 13k across the 160 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

astro-ph2006

A complete 12CO 2-1 map of M51 with HERA

C. Kramer, M. Hitschfeld, K. F. Schuster +2

The nearby, almost face-on, and interacting galaxy M51 offers an excellent opportunity to study the distribution of molecular gas and the mechanisms governing the star formation ra…

astro-ph2006★ 143 cited

A complete 12CO 2-1 map of M51 with HERA: I. Radial averages of CO, HI, and radio continuum

K. F. Schuster, C. Kramer, M. Hitschfeld +2

The mechanisms governing the star formation rate in spiral galaxies are not yet clear. The nearby, almost face-on, and interacting galaxy M51 offers an excellent opportunity to stu…

astro-ph2006★ 23 cited

Study of Photon Dominated Regions in Cepheus B

B. Mookerjea, C. Kramer, M. Roellig +1

Aim: The aim of the paper is to understand the emission from the photon dominated regions in Cepheus B, estimate the column densities of neutral carbon in bulk of the gas in Cepheu…

astro-ph2006

A KOSMA 7 deg^2 13CO 2--1 & 12CO 3--2 survey of the Perseus cloud

K. Sun, C. Kramer, V. Ossenkopf +3

Characterizing the spatial and velocity structure of molecular clouds is a first step towards a better understanding of interstellar turbulence and its link to star formation. We p…

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