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researcher

H. Sung

24 papers hereh-index 161.3k citations89 works total

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

author position
  • middle author17
  • last author5

Across the 22 of 24 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA14
  • astro-ph.SR6
  • astro-ph.HE3
  • astro-ph1
same name
  • H. Sung — 36 papers, h 21
  • H. Sung — 4 papers, h 63
  • H. Sung — 1 paper, h 6
  • H. Sung — 1 paper, h 1
  • H. Sung — 1 paper, h 3
  • H. Sung — 1 paper, h 23

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
20062023
most citedSpace Telescope and Optical Reverberation Mapping Project. III. Optical Continuum Emission and Broad-Band Time Delays in NGC 5548

314 citations · 962 across the 22 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

3 papers · 1 filter

astro-ph.HE2023★ 7 cited

Unusual Hard X-ray Flares Caught in NICER Monitoring of the Binary Supermassive Black Hole Candidate AT2019cuk/Tick Tock/SDSS J1430+2303

Megan Masterson, Erin Kara, Dheeraj R. Pasham +17

The nuclear transient AT2019cuk/Tick Tock/SDSS J1430+2303 has been suggested to harbor a supermassive black hole (SMBH) binary near coalescence. We report results from high-cadence…

astro-ph.HE2021★ 13 cited

GECKO Optical Follow-up Observation of Three Binary Black Hole Merger Events: GW190408_181802, GW190412, and GW190503_185404

Joonho Kim, Myungshin Im, Gregory S. H. Paek +12

We present optical follow-up observation results of three binary black hole merger (BBH) events, GW190408_181802, GW190412, and GW190503_185404, which were detected by the Advanced…

astro-ph.HE2015★ 1 cited

The Very Early Light Curve of SN 2015F in NGC 2442: A Possible Detection of Shock-Heated Cooling Emission and Constraints on SN Ia Progenitor System

Myungshin Im, Changsu Choi, Sung-Chul Yoon +4

The main progenitor candidate of Type Ia supernovae (SNe Ia) is white dwarfs in binary systems where the companion star is another white dwarf (double degenerate system) or a less…

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