Prompt gravitational-wave mergers aided by gas in active galactic nuclei: the hydrodynamics of binary-single black hole scatterings

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 539:2 (2025) 1501-1515

Authors:

Connar Rowan, Henry Whitehead, Gaia Fabj, Pankaj Saini, Bence Kocsis, Martin Pessah, Johan Samsing

The Luminosity Function and Clustering of H$\alpha$ Emitting Galaxies at $z\approx4-6$ from a Complete NIRCam Grism Redshift Survey

(2025)

Authors:

Xiaojing Lin, Eiichi Egami, Fengwu Sun, Haowen Zhang, Xiaohui Fan, Jakob M Helton, Feige Wang, Andrew J Bunker, Zheng Cai, Daniel J Eisenstein, Daniel T Jaffe, Zhiyuan Ji, Xiangyu Jin, Maria Anne Pudoka, Sandro Tacchella, Wei Leong Tee, Pierluigi Rinaldi, Brant Robertson, Yang Sun, Christopher NA Willmer, Chris Willott, Junyu Zhang, Yongda Zhu

Cosmic ray transport and acceleration with magnetic mirroring

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) (2025) staf562

Authors:

AR Bell, JH Matthews, AM Taylor, G Giacinti

REBELS-IFU: dust attenuation curves of 12 massive galaxies at z ≃ 7

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 539:1 (2025) 109-126

Authors:

R Fisher, RAA Bowler, M Stefanon, LE Rowland, HSB Algera, M Aravena, R Bouwens, P Dayal, A Ferrara, Y Fudamoto, C Gulis, JA Hodge, H Inami, K Ormerod, A Pallottini, SG Phillips, NS Sartorio, S Schouws, R Smit, L Sommovigo, DP Stark, PP van der Werf

A MeerKAT survey of nearby dwarf novae: I. New detections

Monthly Notices of the Royal Astronomical Society Oxford University Press 539:3 (2025) 1894-1907

Authors:

J Kersten, E Körding, PA Woudt, PJ Groot, DRA Williams, I Heywood, DL Coppejans, C Knigge, JCA Miller-Jones, GR Sivakoff, R Fender

Abstract:

A programme to search for radio emission from dwarf-novae-type cataclysmic variables was conducted with the South African MeerKAT radio telescope. The dwarf novae RU Pegasi, V426 Ophiuchi, and IP Pegasi were detected during outburst at L band (1284 MHz central frequency). Previously, only one cataclysmic variable was radio-detected at a frequency this low. We now bring the number to four. With these three newly found radio-emitters, the population of dwarf novae confirmed to be radio-emitting at any frequency reaches 10 systems. We found that the radio luminosity is correlated with the optical luminosity. For V426 Ophiuchi and RU Pegasi we found a radio decline contemporary with the outburst’s optical decline. The peak radio luminosity of dwarf novae in outburst is very similar to that of novalike Cataclysmic Variables and no correlation with orbital period is seen.