Chestnut Hill College

output

20182026

most citedInferring CSM Properties of Type II SNe Using a Magnitude-Limited ZTF Sample

13 citations

researchers with a paper here

Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.

T. Starkenburg2 · h 15
V. Kalogera2 · h 29
A. B. Pace1 · h 3
Adam A. Miller1 · h 9
A. Dorozsmai1 · h 4
A. Drlica-Wagner1 · h 95
A. Lapi1 · h 4
Aleksandra Ćiprijanović1 · h 3
Alexander T. Gagliano1 · h 3
Alex Ji1 · h 5
A. Mahabal1 · h 61
A. Malz1 · h 20

collaborating institutions

Northwestern UniversityUS10 papers
Massachusetts Institute of TechnologyUS5 papers
University of ChicagoUS5 papers
California Institute of TechnologyUS4 papers
Institute of AstronomyRU4 papers
Canadian Institute for Theoretical AstrophysicsCA3 papers
Monash UniversityAU3 papers
Simons FoundationUS3 papers
The NSF AI Institute for Artificial Intelligence and Fundamental InteractionsUS3 papers
University of CambridgeGB3 papers
University of TorontoCA3 papers
AlbaNovaSE2 papers

Showing astro-ph.SRShow all

1 paper · 1 filter

astro-ph.SR2025★ 2 cited

Modelling the Future of Gaia Neutron Star-Main Sequence Binaries: From Eccentric Orbits to Millisecond Pulsar-White Dwarfs

Debatri Chattopadhyay, Kyle A. Rocha, Seth Gossage +3

We model the evolution of 21 Gaia neutron star (NS)-main-sequence binaries (orbital period $P_{orb} \sim 200$ -- $1000$ days, eccentricity $e ≳ 0.2$ ) using binary evolutio…