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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.

Dr Micah Bowles

Schmidt AI in Science Fellow

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Zooniverse
  • Galaxy formation and evolution
  • MeerKAT
  • The Square Kilometre Array (SKA)
  • Breakthrough Listen
micah.bowles@physics.ox.ac.uk
Publications
Personal Website
GitHub
ORCID
  • About
  • Research
  • Publications

Scaling Laws for Galaxy Images

(2024)

Authors:

Mike Walmsley, Micah Bowles, Anna MM Scaife, Jason Shingirai Makechemu, Alexander J Gordon, Annette MN Ferguson, Robert G Mann, James Pearson, Jürgen J Popp, Jo Bovy, Josh Speagle, Hugh Dickinson, Lucy Fortson, Tobias Géron, Sandor Kruk, Chris J Lintott, Kameswara Mantha, Devina Mohan, David O'Ryan, Inigo V Slijepevic
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Details from ArXiV

MIGHTEE polarization early science fields: the deep polarized sky

Monthly Notices of the Royal Astronomical Society Oxford University Press 528:2 (2024) 2511-2522

Authors:

Andrew R Taylor, Srikrishna Sekhar, Lennart Heino, Anna MM Scaife, Jeroen Stil, Micah Bowles, Matt Jarvis, Ian Heywood, Jordan D Collier

Abstract:

The MeerKAT International GigaHertz Tiered Extragalactic Exploration (MIGHTEE) is one of the MeerKAT large survey projects, designed to pathfind SKA key science. MIGHTEE is undertaking deep radio imaging of four well-observed fields (COSMOS, XMM-LSS, ELAIS S1, and CDFS) totaling 20 square degrees to μJy sensitivities. Broad-band imaging observations between 880 and1690 MHz yield total intensity continuum, spectro-polarimetry, and atomic hydrogen spectral imaging. Early science data from MIGHTEE are being released from initial observations of COSMOS and XMM–LSS. This paper describes the spectro-polarimetric observations, the polarization data processing of the MIGHTEE early science fields, and presents polarization data images and catalogues. The catalogues include radio spectral index, redshift information, and Faraday rotation measure synthesis results for 13 267 total intensity radio sources down to a polarized intensity detection limit of ∼20 μJy bm−1. Polarized signals were detected from 324 sources. For the polarized detections, we include a catalogue of Faraday Depth from both Faraday Synthesis and Q, U fitting, as well as total intensity and polarization spectral indices. The distribution of redshift of the total radio sources and detected polarized sources are the same, with median redshifts of 0.86 and 0.82, respectively. Depolarization of the emission at longer-wavelengths is seen to increase with decreasing total-intensity spectral index, implying that depolarization is intrinsic to the radio sources. No evidence is seen for a redshift dependence of the variance of Faraday depth.
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Bayesian Imaging for Radio Interferometry with Score-Based Priors

ArXiv 2311.18012 (2023)

Authors:

Noe Dia, MJ Yantovski-Barth, Alexandre Adam, Micah Bowles, Pablo Lemos, Anna MM Scaife, Yashar Hezaveh, Laurence Perreault-Levasseur
Details from ArXiV

Zoobot: Adaptable Deep Learning Models for GalaxyMorphology

The Journal of Open Source Software The Open Journal 8:85 (2023) 5312

Authors:

Mike Walmsley, Campbell Allen, Ben Aussel, Micah Bowles, Kasia Gregorowicz, Inigo Val Slijepcevic, Chris J Lintott, Anna MM Scaife, Maja Jabłońska, Kosio Karchev, Denise Lanzieri, Devina Mohan, David O’Ryan, Bharath Saiguhan, Crisel Suárez, Nicolás Guerra-Varas, Renuka Velu
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Radio galaxy zoo EMU: towards a semantic radio galaxy morphology taxonomy

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 522:2 (2023) 2584-2600

Authors:

Micah Bowles, Hongming Tang, Eleni Vardoulaki, Emma L Alexander, Yan Luo, Lawrence Rudnick, Mike Walmsley, Fiona Porter, Anna MM Scaife, Inigo Val Slijepcevic, Elizabeth AK Adams, Alexander Drabent, Thomas Dugdale, Gülay Gürkan, Andrew M Hopkins, Eric F Jimenez-Andrade, Denis A Leahy, Ray P Norris, Syed Faisal ur Rahman, Xichang Ouyang, Gary Segal, Stanislav S Shabala, O Ivy Wong
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