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researcher

L. C. Ho

42 papers hereh-index 243.3k citations37 works total

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

author position
  • sole author5
  • first author5
  • middle author16
  • last author16

Across the 42 of 42 papers where every author was matched, so the position is known.

fields
  • astro-ph31
  • astro-ph.GA9
  • astro-ph.HE1
  • astro-ph.IM1
same name
  • L. C. Ho — 21 papers, h 6
  • L. C. Ho — 19 papers, h 5
  • L. C. Ho — 15 papers, h 5
  • L. C. Ho — 12 papers, h 10
  • L. C. Ho — 10 papers, h 2
  • L. C. Ho — 7 papers, h 8

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
19972025
most citedEstimating Black Hole Masses in Active Galaxies Using the Halpha Emission Line

840 citations · 6.1k across the 42 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

astro-ph2006★ 24 cited

The Host Galaxy of the Quasar HE 0450-2958

Minjin Kim, Luis C. Ho, Chien Y. Peng +1

A recent study suggests that the quasar HE 0450-2958 is hosted by a galaxy substantially fainter than that inferred from the correlation between black hole mass and bulge luminosit…

astro-ph2006★ 64 cited

Radio Emission on Sub-Parsec Scales from the Intermediate-Mass Black Hole in NGC 4395

J. M. Wrobel, L. C. Ho

The Seyfert 1 nucleus of NGC 4395 is energized by a black hole of 360,000 Solar masses (Peterson et al.), making it one of only two nuclear black holes of intermediate mass, one th…

astro-ph2006★ 218 cited

Stellar populations in the nuclei of late-type spiral galaxies

Carl-Jakob Walcher, Torsten Boeker, Stephane Charlot +5

(Abridged) As part of an ongoing effort to study the stellar nuclei of very late-type, bulge-less spirals, we present results from a high-resolution spectroscopic survey of nine su…

astro-ph2006★ 92 cited

Constraints on the Star Formation Rate in Active Galaxies

Minjin Kim, Luis C. Ho, Myungshin Im

The [O II] 3727 emission line is often used as an indicator of star formation rate in extragalactic surveys, and it can be an equally effective tracer of star formation in systems…

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