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researcher

C. Rauch

8 papers hereh-index 468 citations14 works total

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

author position
  • first author1
  • middle author4

Across the 5 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA6
  • astro-ph.IM2
same name
  • C. Rauch — 9 papers, h 8
  • C. Rauch — 4 papers, h 7
  • C. Rauch — 3 papers, h 22
  • C. Rauch — 3 papers, h 13
  • C. Rauch — 2 papers, h 2
  • C. Rauch — 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
20122017
most citedNear-infrared proper motions and spectroscopy of infrared excess sources at the Galactic Center

97 citations · 186 across the 8 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.IM2012★ 2 cited

Beating the confusion limit: The necessity of high angular resolution for probing the physics of Sagittarius A* and its environment: Opportunities for LINC-NIRVANA (LBT), GRAVITY (VLTI) and and METIS (E-ELT)

A. Eckart, N. Sabha, G. Witzel +16

The super-massive 4 million solar mass black hole (SMBH) SgrA* shows variable emission from the millimeter to the X-ray domain. A detailed analysis of the infrared light curves all…

astro-ph.IM2012★ 97 cited

Near-infrared proper motions and spectroscopy of infrared excess sources at the Galactic Center

A. Eckart, K. Muzic, S. Yazici +11

There are a number of faint compact infrared excess sources in the central stellar cluster of the Milky Way. Their nature and origin is unclear. In addition to several isolated obj…

astro-ph.GA2012★ 52 cited

The S-Star Cluster at the Center of the Milky Way: On the nature of diffuse NIR emission in the inner tenth of a parsec

Nadeen Sabha, Andreas Eckart, David Merritt +9

Sagittarius A*, the super-massive black hole at the center of the Milky Way, is surrounded by a small cluster of high velocity stars, known as the S-stars. We aim to constrain the…

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