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researcher

S. Kraemer

83 papers hereh-index 456k citations230 works total

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

author position
  • first author8
  • middle author46
  • last author8

Across the 62 of 83 papers where every author was matched, so the position is known.

fields
  • astro-ph43
  • astro-ph.GA22
  • astro-ph.HE10
  • astro-ph.CO4
  • astro-ph.IM2
  • astro-ph.SR2
same name
  • S. Kraemer — 62 papers, h 34
  • S. Kraemer — 24 papers, h 5
  • S. Kraemer — 4 papers, h 2
  • S. Kraemer — 3 papers, h 4
  • S. Kraemer — 2 papers, h 12
  • S. Kraemer — 2 papers, h 6

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
19972023
most citedThe Ionized Gas and Nuclear Environment in NGC 3783. I. Time-Averaged 900 ks Chandra Grating Spectroscopy

328 citations · 3.7k across the 83 of their papers we have counts for

collaborators
Showing 2010Show all

3 papers · 1 filter

astro-ph.SR2010★ 3 cited

Stellar Imager (SI): developing and testing a predictive dynamo model for the Sun by imaging other stars

Kenneth G. Carpenter, Carolus J. Schrijver, Margarita Karovska +39

The Stellar Imager mission concept is a space-based UV/Optical interferometer designed to resolve surface magnetic activity and subsurface structure and flows of a population of Su…

astro-ph.CO2010★ 50 cited

Modeling the Outflow in the Narrow-Line Region of Markarian 573:Biconical Illumination of a Gaseous Disk

T. C. Fischer, D. M. Crenshaw, S. B. Kraemer +2

We present a study of the outflowing ionized gas in the resolved narrow-line region (NLR) of the Seyfert 2 galaxy Mrk 573, and its interaction with an in- ner dust/gas disk, based…

astro-ph.CO2010★ 10 cited

Significant X-ray Line Emission in the 5-6 keV band of NGC 4051

T. J. Turner, L. Miller, J. N. Reeves +4

A Suzaku X-ray observation of NGC 4051 taken during 2005 Nov reveals line emission at 5.44 keV in the rest-frame of the galaxy which does not have an obvious origin in known rest-f…

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