Anomaly Detection and RFI Classification with Unsupervised Learning in Narrowband Radio Technosignature Searches

ArXiv 2411.16556 (2024)

Authors:

Ben Jacobson-Bell, Steve Croft, Carmen Choza, Alex Andersson, Daniel Bautista, Vishal Gajjar, Matthew Lebofsky, David HE MacMahon, Caleb Painter, Andrew PV Siemion

A spatially-resolved spectral analysis of giant radio galaxies with MeerKAT

ArXiv 2411.06813 (2024)

Authors:

KKL Charlton, J Delhaize, K Thorat, I Heywood, MJ Jarvis, MJ Hardcastle, Fangxia An, I Delvecchio, CL Hale, IH Whittam, M Brüggen, L Marchetti, L Morabito, Z Randriamanakoto, SV White, AR Taylor

MIGHTEE: the continuum survey Data Release 1

Monthly Notices of the Royal Astronomical Society Oxford University Press 536:3 (2024) 2187-2211

Authors:

Catherine Hale, Ian Heywood, Matthew Jarvis, Imogen Whittam, Philip Best, Fangxia An, Rebecca Bowler, Ian Harrison, Allison Matthews, Dan Smith, Russ Taylor, Mattia Vaccari

Abstract:

The MeerKAT International GHz Tiered Extragalactic Exploration Survey (MIGHTEE) is one of the large survey projects using the MeerKAT telescope, covering four fields that have a wealth of ancillary data available. We present Data Release 1 of the MIGHTEE continuum survey, releasing total intensity images and catalogues over ∼20 deg2, across three fields at ∼1.2-1.3 GHz. This includes 4.2 deg2 over the Cosmic Evolution Survey (COSMOS) field, 14.4 deg2 over the XMM Large-Scale Structure (XMM-LSS) field and deeper imaging over 1.5 deg2 of the Extended Chandra Deep Field South (CDFS). We release images at both a lower resolution (7–9 arcsec) and higher resolution (∼5 arcsec). These images have central rms sensitivities of ∼1.3 −2.7 μJy beam−1 (∼1.2 −3.6 μJy beam−1) in the lower (higher) resolution images respectively. We also release catalogues comprised of ∼144 000 (∼114 000) sources using the lower (higher) resolution images. We compare the astrometry and flux-density calibration with the Early Science data in the COSMOS and XMM-LSS fields and previous radio observations in the CDFS field, finding broad agreement. Furthermore, we extend the source counts at the ∼10 μJy level to these larger areas (∼20 deg2) and, using the areal coverage of MIGHTEE we measure the sample variance for differing areas of sky. We find a typical sample variance of 10-20percnt for 0.3 and 0.5 sq. deg. sub-regions at S1.4 ≤ 200 μJy, which increases at brighter flux densities, given the lower source density and expected higher galaxy bias for these sources.

Simultaneous optical and X-ray detection of a Thermonuclear Burst in the 2024 outburst of EXO 0748–676

Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) (2024) slae103

Authors:

Amy H Knight, Lauren Rhodes, Douglas JK Buisson, James H Matthews, Noel Castro Segura, Adam Ingram, Matthew Middleton, Timothy P Roberts

MIGHTEE: The Continuum Survey Data Release 1

(2024)

Authors:

CL Hale, I Heywood, MJ Jarvis, IH Whittam, PN Best, Fangxia An, RAA Bowler, I Harrison, A Matthews, DJB Smith, AR Taylor, M Vaccari