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researcher

E. Falco

157 papers hereh-index 5513.3k citations411 works total

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

author position
  • first author5
  • middle author101
  • last author23

Across the 129 of 157 papers where every author was matched, so the position is known.

fields
  • astro-ph86
  • astro-ph.HE17
  • astro-ph.CO16
  • astro-ph.GA15
  • astro-ph.EP14
  • astro-ph.SR6
same name
  • E. Falco — 10 papers, h 3
  • E. Falco — 7 papers
  • E. Falco — 4 papers, h 3
  • E. Falco — 1 paper, h 1
  • E. Falco — 1 paper, h 2
  • E. Falco — 1 paper, 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

activity
19952023
most citedLSST Science Book, Version 2.0

924 citations · 13.9k across the 157 of their papers we have counts for

collaborators
Showing 2001 · astro-phShow all

4 papers · 2 filters

astro-ph2001★ 12 cited

J06587-5558 -- A Very Unusual Polarised Radio Source

H. Liang, R. D. Ekers, R. W. Hunstead +2

We have found a peculiar radio source in the field of one of the hottest known clusters of galaxies 1E0657-56. It is slightly extended, highly polarised (54% at 8.8GHz) and has a v…

astro-ph2001★ 30 cited

Constraining H0 from Chandra Observations of Q0957+561

G. Chartas, V. Gupta, G. Garmire +4

We report the detection of the lens cluster of the gravitational lens (GL) system Q0957+561 from a deep observation with the Advanced CCD Imaging Spectrometer on-board the Chandra…

astro-ph2001★ 50 cited

Rapid UBVRI Follow-up of the Highly Collimated Optical Afterglow of GRB010222

K. Z. Stanek, P. M. Garnavich, S. Jha +6

(Abridged) We present the earliest optical observations of the optical counterpart to the GRB 010222, obtained with the FLWO 1.2-m telescope in UBVRI passbands, starting 3.64 hours…

astro-ph2001★ 121 cited

A Black Hole of > 6 Solar Masses in the X-ray Nova XTE J1118+480

J. E. McClintock, M. R. Garcia, N. Caldwell +3

Observations of the quiescent X-ray nova XTE J1118+480 with the new 6.5-m MMT have revealed that the velocity amplitude of the dwarf secondary is 698 +/- 14 km/s and the orbital pe…

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