activity
20232026
most citedLimits on the Ejecta Mass During the Search for Kilonovae Associated with Neutron Star-Black Hole Mergers: A case study of S230518h, GW230529, S230627c and the Low-Significance Candidate S240422ed

11 citations · 28 across the 11 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2026

Radiation-hydrodynamics of star-disc collisions: From system parameters to outflows and lightcurves

Taj Jankovič, Sergey Karpov, Michal Zajaček +2

Quasi-periodic eruptions (QPEs) are nuclear transients producing bright, repeating soft X-ray flares superimposed on quiescent emission. A promising interpretation is that they are…

astro-ph.HE2026★ 1 cited

Radiation-hydrodynamics of star-disc collisions for quasi-periodic eruptions

Taj Jankovič, Clément Bonnerot, Sergey Karpov +1

Quasi-periodic eruptions (QPEs) are recently discovered transients of unknown nature occurring near supermassive black holes, which feature bright X-ray bursts separated by hours t…

astro-ph.HE2025

Lost and Found - A gallery of overlooked optical nuclear transients from the ZTF archive

E. Quintin, E. Russeil, M. Llamas Lanza +12

Tidal disruption events (TDEs) correspond to the destruction of a star by the tidal forces around a black hole, leading to outbursts which can last from months to years. These tran…

astro-ph.HE2025★ 5 cited

Early Identification of Optical Tidal Disruption Events: A science module for the Fink broker

Miguel Llamas Lanza, Sergey Karpov, Etienne Russeil +5

The detection of tidal disruption events (TDEs) is one of the key science goals of large optical time-domain surveys such as the Zwicky Transient Facility (ZTF) and the upcoming Ve…

astro-ph.HE2025★ 11 cited

Limits on the Ejecta Mass During the Search for Kilonovae Associated with Neutron Star-Black Hole Mergers: A case study of S230518h, GW230529, S230627c and the Low-Significance Candidate S240422ed

M. Pillas, S. Antier, K. Ackley +78

Neutron star-black hole (NSBH) mergers, detectable via their gravitational-wave (GW) emission, are expected to produce kilonovae (KNe). Four NSBH candidates have been identified an…

astro-ph.HE2023★ 1 cited

Ready for O4 II: GRANDMA Observations of Swift GRBs during eight-weeks of Spring 2022

I. Tosta e Melo, J. -G. Ducoin, Z. Vidadi +106

We present a campaign designed to train the GRANDMA network and its infrastructure to follow up on transient alerts and detect their early afterglows. In preparation for O4 II camp…