activity
20192026
most citedAstro2020 Science White Paper: The Next Decade of Astroinformatics and Astrostatistics

1 citations · 2 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.IM2026

The statistical properties of the cross spectrum

Edward J. R. Nathan, Adam Ingram, Daniela Huppenkothen +2

The cross spectrum encodes the correlated variability between two time signals. In recent years, the cross spectrum has been used to study astronomical sources, particularly in the…

astro-ph.HE2026

A NICER View of PSR J0030+0451: Updated Constraints from Six Years of NICER Observations

Yves Kini, Lucien Mauviard, Tuomo Salmi +13

Pulse-profile modeling of rotation-powered millisecond pulsars targeted by NICER has enabled mass--radius constraints of several neutron star sources, with implications for the den…

astro-ph.HE2025

Modeling X-ray photon pile-up with a normalizing flow

Ole König, Daniela Huppenkothen, Douglas Finkbeiner +5

The dynamic range of imaging detectors flown on-board X-ray observatories often only covers a limited flux range of extrasolar X-ray sources. The analysis of bright X-ray sources i…

astro-ph.HE2024

Representation learning for fast radio burst dynamic spectra

Dirk Kuiper, Gabriella Contardo, Daniela Huppenkothen +1

Fast radio bursts (FRBs) are millisecond-duration radio transients of extragalactic origin, with diverse time-frequency patterns and emission properties that require explanation. W…

astro-ph.HE20241 cited

RTFAST-Spectra: Emulation of X-ray reverberation mapping for active galactic nuclei

Benjamin Ricketts, Daniela Huppenkothen, Matteo Lucchini +4

Bayesian analysis has begun to be more widely adopted in X-ray spectroscopy, but it has largely been constrained to relatively simple physical models due to limitations in X-ray mo…

astro-ph.HE2024

A probe of the maximum energetics of fast radio bursts through a prolific repeating source

O. S. Ould-Boukattine, P. Chawla, J. W. T. Hessels +12

Fast radio bursts (FRBs) are sufficiently energetic to be detectable from luminosity distances up to at least seven billion parsecs (redshift ). Probing the maximum energies…