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J. Miller

27 papers hereh-index 416k citations194 works total

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

author position
  • sole author2
  • first author1
  • middle author5
  • last author1

Across the 9 of 27 papers where every author was matched, so the position is known.

fields
  • astro-ph22
  • astro-ph.HE5
same name
  • J. Miller — 11 papers, h 10
  • J. Miller — 8 papers, h 35
  • J. Miller — 7 papers, h 47
  • J. Miller — 5 papers, h 36
  • J. Miller — 5 papers, h 34
  • J. Miller — 3 papers

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
20012009
most citedRelativistic X-ray Lines from the Inner Accretion Disks Around Black Holes

409 citations · 1.2k across the 14 of their papers we have counts for

collaborators
Showing 2005Show all

3 papers · 1 filter

astro-ph2005

On the Robustness of Cool Disc Components in Bright ULXs

J. M. Miller, A. C. Fabian, M. C. Miller

In this letter, we comment on the robustness of putative cool (kT ~ 0.2 keV) accretion disc components in the X-ray spectra of the most luminous (L ~ 10^40 erg/s) ultra-luminous X-…

astro-ph2005

The evolution of the timing properties of the black-hole transient GX 339-4 during its 2002/2003 outburst

T. Belloni, J. Homan, P. Casella +5

We present the results of the timing and color analysis of more than two hundred RXTE/PCA observations of the bright black-hole transient GX 339-4 obtained during its 2002/2003 out…

astro-ph2005

Evidence for a Link Between Fe K-alpha Emission Line Strength and QPO Phase in a Black Hole

J. M. Miller, J. Homan

In X-ray binaries, the frequencies revealed in X-ray quasi-periodic oscillations (QPOs) are often interpreted as characteristic frequencies in the inner accretion disk, though the…

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