collaborators

25 papers

astro-ph.IM2026

The Cross-Survey Decade: A Call to Action

Gioia Rau, Robert Benjamin, Federica Bianco +24

By 2027, three flagship wide-field surveys will be operating simultaneously from ground and space, observing overlapping sky and representing more than $6 billion in US and Europea…

astro-ph.HE2026

Tidal disruption event rates across cosmic time: forecasts for LSST, Roman, and JWST and their constraints on the supermassive black hole mass function

Mitchell Karmen, Suvi Gezari, Colin Norman +1

The paper builds a semi‑empirical model for how tidal disruption event (TDE) rates evolve with redshift under different supermassive black hole mass‑function scenarios, and uses fo…

astro-ph.IM2026

The Lazuli Space Observatory: Opportunities for time-domain and multi-messenger astronomy

T. Wevers, T. J. Maccarone, A. Palmese +14

Advancing time-domain and multi-messenger astronomy requires a multi-wavelength network of observatories capable of rapidly discovering, classifying, and characterizing transient p…

astro-ph.HE2026

TDE 2025abcr: A Tidal Disruption Event in the Outskirts of a Massive Galaxy

Robert Stein, Jonathan Carney, Charlotte Ward +27

Tidal disruption events (TDEs) have traditionally been discovered in optical sky surveys through targeted searches of nuclear transients. However, it is expected that some TDEs wil…

astro-ph.HE2026

The Wandering Supermassive Black Hole Powering the off-nuclear TDE AT2024tvd

M. Guolo, A. Mummery, S. van Velzen +11

We present an analysis of the spectral energy distribution (SED) of the off-nuclear tidal disruption event (TDE) AT2024tvd during its late-time plateau phase, combining X-ray spect…

astro-ph.HE2026

AT2019cmw: A highly luminous, cooling featureless TDE candidate from the disruption of a high mass star in an early-type galaxy

Jacob L. Wise, Daniel A. Perley, Nikhil Sarin +23

We present optical/UV photometric and spectroscopic observations, as well as X-ray and radio follow-up, of the extraordinary event AT2019cmw. With a peak bolometric luminosity of ~…