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M. Eckart

38 papers hereh-index 385.2k citations322 works total

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

author position
  • middle author20

Across the 20 of 38 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE22
  • astro-ph.IM9
  • astro-ph.GA4
  • astro-ph.SR2
  • astro-ph.CO1
same name
  • M. Eckart — 2 papers, h 1

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

works on
active galactic nuclei 1coronal flares 1magnetic reconnection 1ultra-fast outflows 1xrism observations 1

From the 1 of 38 linked papers with an AI index.

activity
20242026
most citedDelving into the depths of NGC 3783 with XRISM IV. Mapping of the accretion flow with Fe KI^± emission lines

10 citations · 37 across the 15 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.HE2024

Overionized plasma in the supernova remnant Sagittarius A East anchored by XRISM observations

XRISM Collaboration

Sagittarius A East is a supernova remnant with a unique surrounding environment, as it is located in the immediate vicinity of the supermassive black hole at the Galactic center, S…

astro-ph.HE2024

The XRISM/Resolve view of the Fe K region of Cyg X-3

XRISM Collaboration

The X-ray binary system Cygnus X-3 (4U 2030+40, V1521 Cyg) is luminous but enigmatic owing to the high intervening absorption. High-resolution X-ray spectroscopy uniquely probes th…

astro-ph.SR2024

High-Resolution Laboratory Measurements of M-shell Fe EUV Line Emission using EBIT-I

Alexander J. Fairchild, Natalie Hell, Peter Beiersdorfer +4

Solar physicists routinely utilize observations of Ar-like Fe IX and Cl-like Fe X emission to study a variety of solar structures. However, unidentified lines exist in the Fe IX an…

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