activity
20012023
most citedMethods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs

1.8k citations · 16.8k across the 193 of their papers we have counts for

collaborators

196 papers

astro-ph.HE2023

Swift/UVOT discovery of Swift J221951-484240: a UV luminous ambiguous nuclear transient

S. R. Oates, N. P. M. Kuin, M. Nicholl +57

We report the discovery of Swift J221951-484240 (hereafter: J221951), a luminous slow-evolving blue transient that was detected by the Neil Gehrels Swift Observatory Ultra-violet/O…

astro-ph.SR2023★ 11 cited

Infrared spectroscopy of the 2022 eruption of the recurrent nova U Sco

A. Evans, D. P. K. Banerjee, C. E. Woodward +5

We present near-infrared spectroscopy of the 2022 eruption of the recurrent nova U Sco, over the period from 5.2 to 45.4 days after outburst. This is the most intensive infrared st…

astro-ph.HE2023★ 25 cited

The multi-wavelength view of shocks in the fastest nova V1674 Her

K. V. Sokolovsky, T. J. Johnson, S. Buson +41

Classical novae are shock-powered multi-wavelength transients triggered by a thermonuclear runaway on an accreting white dwarf. V1674 Her is the fastest nova ever recorded (time to…

astro-ph.HE2023★ 112 cited

GRB 221009A: Discovery of an Exceptionally Rare Nearby and Energetic Gamma-Ray Burst

Maia A. Williams, Jamie A. Kennea, S. Dichiara +53

We report the discovery of the unusually bright long-duration gamma-ray burst (GRB), GRB 221009A, as observed by the Neil Gehrels Swift Observatory (Swift), Monitor of All-sky X-ra…

astro-ph.HE2022★ 16 cited

High Resolution X-ray Spectra of RS Ophiuchi (2006 and 2021): Revealing the cause of SSS variability

J. -U. Ness, A. P. Beardmore, M. F. Bode +9

Swift observed the SSS phase in RS Oph much fainter in 2021 than in 2006, and we compare an XMM-Newton grating spectrum on day 55.6 in 2021 (2021d55.6) to SSS Chandra and XMM-Newto…

astro-ph.HE2022

Ultraviolet and X-ray light-curves of novae observed by the Neil Gehrels Swift Observatory

K. L. Page, N. P. M. Kuin, J. P. Osborne

With rapid response capabilities, and a daily planning of its observing schedule, the Neil Gehrels Swift Observatory is ideal for monitoring transient and variable sources. Here we…