It is not σ8: constraining the non-linear matter power spectrum with the Dark Energy Survey Year-5 supernova sample
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 537:4 (2025) 3814-3825
Contemporaneous optical-radio observations of a fast radio burst in a close galaxy pair
(2025)
Arcminute Microkelvin Imager observations at 15.5 GHz of multiple outbursts of Cygnus X-3 in 2024
ArXiv 2502.20409 (2025)
Arcminute Microkelvin Imager Observations at 15.5 GHz of Multiple Outbursts of Cygnus X-3 in 2024
Research Notes of the American Astronomical Society American Astronomical Society 9:2 (2025) 35
Abstract:
We report radio monitoring of Cygnus X-3 at 15.5 GHz during 2024 with the Arcminute Microkelvin Imager. Observations were made on 296 days throughout the year, and reveal five radio outbursts to multi-jansky levels, peaking in February, April, June, July and August. The brightest peak, with ≈16 Jy, was on June 27th.Calibrating the absolute magnitude of type Ia supernovae in nearby galaxies using [OII] and implications for H0
Monthly Notices of the Royal Astronomical Society (2025) staf266