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E. Perlman

46 papers hereh-index 384.3k citations306 works total

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

author position
  • first author9
  • middle author25
  • last author5

Across the 39 of 46 papers where every author was matched, so the position is known.

fields
  • astro-ph44
  • astro-ph.CO2
same name
  • E. Perlman — 9 papers, h 18
  • E. Perlman — 2 papers, h 2
  • E. Perlman — 1 paper, h 5
  • E. Perlman — 1 paper, h 12

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
19972009
most citedA multi-zone model for simulating the high energy variability of TeV blazars

67 citations · 466 across the 19 of their papers we have counts for

collaborators
Showing 2004Show all

4 papers · 1 filter

astro-ph2004

A Chandra Survey of Quasar Jets: First Results

H. L. Marshall, D. A. Schwartz, J. E. J. Lovell +6

We present results from Chandra X-ray imaging and spectroscopy of a flux-limited sample of flat spectrum radio-emitting quasars with jet-like extended structure. Twelve of twenty q…

astro-ph2004

A Physical Classification Scheme for Blazars

H. Landt, P. Padovani, E. S. Perlman +1

Blazars are currently separated into BL Lacertae objects (BL Lacs) and flat spectrum radio quasars (FSRQ) based on the strength of their emission lines. This is done rather arbitra…

astro-ph2004

Observations of Abell 4059 with Chandra, HST and VLA: unraveling a complex cluster/radio-galaxy interaction

Yun Young Choi, Christopher S. Reynolds, Sebastian Heinz +3

(abridged) We present a detailed reanalysis of the Chandra data for the galaxy cluster Abell 4059 and its central radio galaxy, PKS2354-35. We also present new 1.4GHz and 4.7GHz Cn…

astro-ph2004

XMM-Newton observations of the BL Lac MS0205.7+3509: a dense, low-metallicity absorber

D. Watson, B. McBreen, L. Hanlon +5

The high-frequency-peaked BL Lac, MS0205.7+3509 was observed twice with XMM-Newton. Both X-ray spectra are synchrotron-dominated, with mean 0.2--10keV fluxes of 2.80+/-0.01 and 3.3…

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