output
19932026
most citedThe Seventh Data Release of the Sloan Digital Sky Survey

5.4k citations

Showing 2024 · astro-ph.HEShow all

10 papers · 2 filters

astro-ph.HE2024★ 4 cited

Rotation Measure study of FRB 20180916B with the uGMRT

S. Bethapudi, L. G. Spitler, D. Z. Li +4

Context. Fast Radio Burst 20180916B is a repeating FRB whose activity window has a 16.34 day periodicity that also shifts and varies in duration with the observing frequency. Recen…

astro-ph.HE2024★ 19 cited

CHIME/FRB/Pulsar discovery of a nearby long period radio transient with a timing glitch

Fengqiu Adam Dong, Tracy E Clarke, Alice Curtin +22

We present the discovery of a 421 s long period radio transient (LPT) using the CHIME telescope, CHIME J0630+25. The source is localized to RA=06:30:38.4 Dec=25:26:24…

astro-ph.HE2024★ 6 cited

An activity transition in FRB 20201124A: methodological rigor, detection of frequency-dependent cessation, and a geometric magnetar model

A. V. Bilous, J. van Leeuwen, Y. Maan +4

We report detections of fast radio bursts (FRBs) from the repeating source FRB 20201124A with Apertif/WSRT and GMRT, and measurements of basic burst properties, especially the disp…

astro-ph.HE2024

Study of Wolf-Rayet stars using uGMRT

Anindya Saha, Anandmayee Tej, Santiago del Palacio +4

In recent years, systems involving massive stars with large wind kinetic power have been considered as promising sites for investigating relativistic particle acceleration in low r…

astro-ph.HE2024★ 3 cited

Investigating the Role of Pre-supernova Massive Stars in the Acceleration of Galactic Cosmic Rays

Michael De Becker, Santiago del Palacio, Paula Benaglia +5

Galactic cosmic rays (GCRs) constitute a significant part of the energy budget of our Galaxy, and the study of their accelerators is of high importance in modern astrophysics. Thei…

astro-ph.HE2024★ 2 cited

Localisation of the non-thermal X-ray emission of PSR~J2229+6114 from its multi-wavelength pulse profiles

J. Pétri, S. Guillot, L. Guillemot +5

Pulsars are detected over the whole electromagnetic spectrum, from radio wavelengths up to very high energies, in the GeV-TeV range. Whereas the radio emission site for young pulsa…