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From the 1 of 5 linked papers with an AI index.

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20242026
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5 papers

astro-ph.HE2026

Swift gives a new BAT-GLIMPSE: Gamma-ray Localization using Imaging and Mosaic techniques for Pointing and Slew Epochs

S. Ronchini, T. Parsotan, J. DeLaunay +1

The paper presents BAT-GLIMPSE, an open‑source, low‑latency pipeline that automatically localizes transient gamma‑ray sources in Swift‑BAT data during both pointing observations an…

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.HE2025

SVOM GRB 250314A at z 7.3: an exploding star in the era of reionization

B. Cordier, J. Y. Wei, N. R. Tanvir +103

Most long Gamma-ray bursts originate from a rare type of massive stellar explosion. Their afterglows, while rapidly fading, can be initially extremely luminous at optical/near-infr…

astro-ph.GA2025

The ultraviolet luminosity function of star-forming galaxies between redshifts of 0.4 and 0.6

M. J. Page, T. Dwelly, I. McHardy +7

We combine ultraviolet imaging of the 13H survey field, taken with the XMM-Newton Optical Monitor telescope (XMM-OM) and the Neil Gehrels Swift Observatory Ultraviolet and Optical…

astro-ph.HE2024

Panning for gold with the Neil Gehrels Swift Observatory: an optimal strategy for finding the counterparts to gravitational wave events

R. A. J. Eyles-Ferris, P. A. Evans, A. A. Breeveld +17

The LIGO, Virgo and KAGRA gravitational wave observatories are currently undertaking their O4 observing run offering the opportunity to discover new electromagnetic counterparts to…