The host galaxies of tidal disruption events
Abstract Recent studies of Tidal Disruption Events (TDEs) have revealed unexpected
correlations between the TDE rate and the large-scale properties of the host galaxies. In this …
correlations between the TDE rate and the large-scale properties of the host galaxies. In this …
The final season reimagined: 30 tidal disruption events from the ZTF-I Survey
Tidal disruption events (TDEs) offer a unique way to study dormant black holes. While the
number of observed TDEs has grown thanks to the emergence of wide-field surveys in the …
number of observed TDEs has grown thanks to the emergence of wide-field surveys in the …
Seventeen tidal disruption events from the first half of ZTF survey observations: entering a new era of population studies
While tidal disruption events (TDEs) have long been heralded as laboratories for the study of
quiescent black holes, the small number of known TDEs and uncertainties in their emission …
quiescent black holes, the small number of known TDEs and uncertainties in their emission …
First tidal disruption events discovered by SRG/eROSITA: X-ray/optical properties and X-ray luminosity function at z < 0.6
S Sazonov, M Gilfanov, P Medvedev… - Monthly Notices of …, 2021 - academic.oup.com
We present the first sample of tidal disruption events (TDEs) discovered during the SRG all-
sky survey. These 13 events were selected among X-ray transients detected in the 0°< l< …
sky survey. These 13 events were selected among X-ray transients detected in the 0°< l< …
On the quenching of star formation in observed and simulated central galaxies: evidence for the role of integrated AGN feedback
JM Piotrowska, AFL Bluck, R Maiolino… - Monthly Notices of the …, 2022 - academic.oup.com
In this paper, we investigate how massive central galaxies cease their star formation by
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …
comparing theoretical predictions from cosmological simulations: EAGLE, Illustris, and …
How do central and satellite galaxies quench?–Insights from spatially resolved spectroscopy in the MaNGA survey
AFL Bluck, R Maiolino, JM Piotrowska… - Monthly Notices of …, 2020 - academic.oup.com
We investigate how star formation quenching proceeds within central and satellite galaxies
using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a …
using spatially resolved spectroscopy from the SDSS-IV MaNGA DR15. We adopt a …
The quenching of galaxies, bulges, and disks since cosmic noon-A machine learning approach for identifying causality in astronomical data
AFL Bluck, R Maiolino, S Brownson… - Astronomy & …, 2022 - aanda.org
We present an analysis of the quenching of star formation in galaxies, bulges, and disks
throughout the bulk of cosmic history, from z= 2− 0. We utilise observations from the Sloan …
throughout the bulk of cosmic history, from z= 2− 0. We utilise observations from the Sloan …
Six months of multiwavelength follow-up of the tidal disruption candidate ASASSN-14li and implied TDE rates from ASAS-SN
TWS Holoien, CS Kochanek, JL Prieto… - Monthly Notices of …, 2016 - academic.oup.com
We present ground-based and Swift photometric and spectroscopic observations of the
candidate tidal disruption event (TDE) ASASSN-14li, found at the centre of PGC 043234 (d≃ …
candidate tidal disruption event (TDE) ASASSN-14li, found at the centre of PGC 043234 (d≃ …
Weighing black holes using tidal disruption events
B Mockler, J Guillochon… - The Astrophysical …, 2019 - iopscience.iop.org
While once rare, observations of stars being tidally disrupted by supermassive black holes
are quickly becoming commonplace. To continue to learn from these events, it is necessary …
are quickly becoming commonplace. To continue to learn from these events, it is necessary …
Constraining the galaxy–halo connection over the last 13.3 Gyr: star formation histories, galaxy mergers and structural properties
A Rodríguez-Puebla, JR Primack… - Monthly Notices of …, 2017 - academic.oup.com
We present new determinations of the stellar-to-halo mass relation (SHMR) at z= 0–10 that
match the evolution of the galaxy stellar mass function, the star formation rate (SFR)–M …
match the evolution of the galaxy stellar mass function, the star formation rate (SFR)–M …