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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Prof. Matt Jarvis

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Cosmology
  • Galaxy formation and evolution
  • Hintze Centre for Astrophysical Surveys
  • MeerKAT
  • Rubin-LSST
  • The Square Kilometre Array (SKA)
Matt.Jarvis@physics.ox.ac.uk
Telephone: 01865 (2)83654
Denys Wilkinson Building, room 703
  • About
  • Publications

A spatially resolved spectral analysis of giant radio galaxies with MeerKAT

Monthly Notices of the Royal Astronomical Society 537:1 (2024) 272-284

Authors:

KKL Charlton, J Delhaize, K Thorat, I Heywood, MJ Jarvis, MJ Hardcastle, F An, I Delvecchio, CL Hale, IH Whittam, M Brüggen, L Marchetti, L Morabito, Z Randriamanakoto, SV White, AR Taylor
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MeerKAT discovery of a MIGHTEE Odd Radio Circle

Monthly Notices of the Royal Astronomical Society: Letters Oxford University Press (OUP) 537:1 (2024) l42-l48

Authors:

Ray P Norris, Bärbel S Koribalski, Catherine L Hale, Matt J Jarvis, Peter J Macgregor, A Russell Taylor
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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.
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Deep extragalactic H i survey of the COSMOS field with FAST

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 534:1 (2024) 202-214

Authors:

Hengxing Pan, Matt J Jarvis, Ming Zhu, Yin-Zhe Ma, Mario G Santos, Anastasia A Ponomareva, Ian Heywood, Yingjie Jing, Chen Xu, Ziming Liu, Yogesh Chandola, Yipeng Jing
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MIGHTEE-H i: deep spectral line observations of the COSMOS field

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 534:1 (2024) 76-96

Authors:

I Heywood, AA Ponomareva, N Maddox, MJ Jarvis, BS Frank, EAK Adams, M Baes, A Bianchetti, JD Collier, RP Deane, M Glowacki, SL Jung, H Pan, SHA Rajohnson, G Rodighiero, I Ruffa, MG Santos, F Sinigaglia, M Vaccari
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