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C. Rodriguez

70 papers hereh-index 509k citations111 works total

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

author position
  • sole author1
  • first author16
  • middle author44
  • last author8

Across the 69 of 70 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE37
  • astro-ph.GA20
  • astro-ph.SR5
  • astro-ph.IM3
  • gr-qc3
  • astro-ph.CO2
same name
  • C. Rodriguez — 6 papers, h 3
  • C. Rodriguez — 5 papers, h 5
  • C. Rodriguez — 5 papers, h 2
  • C. Rodriguez — 3 papers, h 3
  • C. Rodriguez — 2 papers, h 2
  • C. Rodriguez — 2 papers, h 2

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
20112023
most citedBinary Black Hole Mergers from Globular Clusters: Masses, Merger Rates, and the Impact of Stellar Evolution

581 citations · 8k across the 70 of their papers we have counts for

collaborators
Showing 2022Show all

3 papers · 1 filter

astro-ph.GA2022★ 9 cited

Evolution of Massive Black Hole Binaries in Collisionally Relaxed Nuclear Star Clusters -- Impact of Mass Segregation

Diptajyoti Mukherjee, Qirong Zhu, Go Ogiya +2

Massive Black Hole (MBH) binaries are considered to be one of the most important sources of Gravitational Waves (GW) that can be detected by GW detectors like LISA. However, there…

astro-ph.GA2022★ 37 cited

Great Balls of FIRE II: The evolution and destruction of star clusters across cosmic time in a Milky Way-mass galaxy

Carl L. Rodriguez, Zachary Hafen, Michael Y. Grudić +4

The current generation of galaxy simulations can resolve individual giant molecular clouds, the progenitors of dense star clusters. But the evolutionary fate of these young massive…

astro-ph.GA2022★ 43 cited

Great Balls of FIRE I: The formation of star clusters across cosmic time in a Milky Way-mass galaxy

Michael Y. Grudić, Zachary Hafen, Carl L. Rodriguez +5

The properties of young star clusters formed within a galaxy are thought to vary in different interstellar medium (ISM) conditions, but the details of this mapping from galactic to…

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