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E. Miller

12 papers hereh-index 7791 citations30 works total

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

author position
  • middle author9

Across the 9 of 12 papers where every author was matched, so the position is known.

fields
  • astro-ph.IM7
  • astro-ph.HE4
  • astro-ph.GA1
same name
  • E. Miller — 84 papers, h 34
  • E. Miller — 49 papers, h 24
  • E. Miller — 29 papers, h 9
  • E. Miller — 25 papers, h 42
  • E. Miller — 20 papers, h 3
  • E. Miller — 13 papers, h 5

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
20142026
most citedDevelopment of the Timing System for the X-Ray Imaging and Spectroscopy Mission

3 citations · 3 across the 12 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

4 papers · 1 filter

astro-ph.HE2025

Evidence for Charge Exchange Emission in Supernova Remnant N132D from XRISM/Resolve Observations

Liyi Gu, Hiroya Yamaguchi, Adam Foster +24

XRISM has delivered one of its first light observations on N132D, the X-ray brightest supernova remnant in the Large Magellanic Cloud. Utilizing 193 ks of high-resolution X-ray spe…

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.HE2014

ASTRO-H White Paper - New Spectral Features

R. K. Smith, H. Odaka, M. Audard +27

This white paper addresses selected new (to X-ray astronomy) physics and data analysis issues that will impact ASTRO-H SWG observations as a result of its high-spectral-resolution…

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