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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 Rebecca Bowler

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Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Galaxy formation and evolution
rebecca.bowler@physics.ox.ac.uk
  • About
  • Brief CV
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  • Publications

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
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The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam

The Astrophysical Journal American Astronomical Society 979:2 (2025) 140

Authors:

Christina C Williams, Pascal A Oesch, Andrea Weibel, Gabriel Brammer, Aidan P Cloonan, Katherine E Whitaker, Laia Barrufet, Rachel Bezanson, Rebecca AA Bowler, Pratika Dayal, Marijn Franx, Jenny E Greene, Anne Hutter, Zhiyuan Ji, Ivo Labbé, Sinclaire M Manning, Michael V Maseda, Mengyuan Xiao
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Euclid preparation. LVII. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys

Astronomy & Astrophysics EDP Sciences (2024)

Authors:

M Selwood, S Fotopoulou, MN Bremer, L Bisigello, H Landt, E Banados, G Zamorani, F Shankar, D Stern, E Lusso, L Spinoglio, V Allevato, F Ricci, A Feltre, F Mannucci, M Salvato, RA Bowler, M Mignoli, D Vergani, F La Franca, A Amara, S Andreon, N Auricchio, M Baldi, S Bardelli, R Bender, C Bodendorf, D Bonino, E Branchini, M Brescia, J Brinchmann, S Camera, V Capobianco, C Carbone, J Carretero, S Casas, M Castellano, S Cavuoti, A Cimatti, G Congedo, CJ Conselice, L Conversi, Y Copin, F Courbin, HM Courtois, M Cropper, A Da Silva, H Degaudenzi, AM Di Giorgio, J Dinis, F Dubath, X Dupac, S Dusini, M Farina, S Farrens, S Ferriol, M Frailis, E Franceschi, S Galeotta, B Gillis, C Giocoli, A Grazian, F Grupp, L Guzzo, SVH Haugan, H Hoekstra, MS Holliman, W Holmes, I Hook, F Hormuth, A Hornstrup, P Hudelot, K Jahnke, E Keihänen, S Kermiche, A Kiessling, B Kubik, M Kummel, M Kunz, H Kurki-Suonio, R Laureijs, S Ligori, PB Lilje, V Lindholm, I Lloro, D Maino, E Maiorano, O Mansutti, O Marggraf, K Markovic, N Martinet, F Marulli, R Massey, E Medinaceli, S Mei, M Melchior, Y Mellier, M Meneghetti, E Merlin, G Meylan, M Moresco, L Moscardini, E Munari, S-M Niemi, JW Nightingale, C Padilla, S Paltani, F Pasian, K Pedersen, WJ Percival, V Pettorino, G Polenta, M Poncet, LA Popa, L Pozzetti, F Raison, R Rebolo, A Renzi, J Rhodes, G Riccio, Hans-Walter Rix, E Romelli, M Roncarelli, E Rossetti, R Saglia, D Sapone, B Sartoris, R Scaramella, M Schirmer, P Schneider, T Schrabback, A Secroun, G Seidel, S Serrano, C Sirignano, G Sirri, L Stanco, C Surace, P Tallada-Crespi, D Tavagnacco, AN Taylor, HI Teplitz, I Tereno, R Toledo-Moreo, F Torradeflot, I Tutusaus, L Valenziano, T Vassallo, A Veropalumbo, Y Wang, J Weller, E Zucca, A Biviano, M Bolzonella, E Bozzo, C Burigana, C Colodro-Conde, G De Lucia, D Di Ferdinando, JA Escartin Vigo, R Farinelli, K George, J Gracia-Carpio, M Martinelli, N Mauri, C Neissner, Z Sakr, V Scottez, M Tenti, M Viel, M Wiesmann, Y Akrami, S Anselmi, C Baccigalupi, M Ballardini, M Bethermin, A Blanchard, L Blot, S Borgani, S Bruton, R Cabanac, A Calabro, G Canas-Herrera, A Cappi, CS Carvalho, G Castignani, T Castro, KC Chambers, S Contarini, T Contini, AR Cooray, O Cucciati, S Davini, B De Caro, G Desprez, A Diaz-Sanchez, S Di Domizio, H Dole, S Escoffier, AG Ferrari, I Ferrero, F Finelli, A Fontana, F Fornari, L Gabarra, K Ganga, J Garcia-Bellido, V Gautard, E Gaztanaga, F Giacomini, G Gozaliasl, A Hall, H Hildebrandt, J Hjorth, JE Kajava, V Kansal, D Karagiannis, C Kirkpatrick, L Legrand, G Libet, A Loureiro, J Macias-Perez, G Maggio, M Magliocchetti, R Maoli, CJAP Martins, S Matthew, L Maurin, RB Metcalf, P Monaco, C Moretti, G Morgante, S Nadathur, L Nicastro, Nicholas A Walton, L Patrizii, A Pezzotta, M Pontinen, V Popa, C Porciani, D Potter, I Risso, P-F Rocci, M Sahlen, AG Sanchez, A Schneider, E Sefusatti, M Sereno, P Simon, A Spurio Mancini, J Steinwagner, G Testera, R Teyssier, S Toft, S Tosi, A Troja, M Tucci, C Valieri, J Valiviita, G Verza, JR Weaver, IA Zinchenko
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REBELS-25: discovery of a dynamically cold disc galaxy at z = 7.31

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 535:3 (2024) 2068-2091

Authors:

Lucie E Rowland, Jacqueline Hodge, Rychard Bouwens, Pavel E Mancera Piña, Alexander Hygate, Hiddo Algera, Manuel Aravena, Rebecca Bowler, Elisabete da Cunha, Pratika Dayal, Andrea Ferrara, Thomas Herard-Demanche, Hanae Inami, Ivana van Leeuwen, Ilse de Looze, Pascal Oesch, Andrea Pallottini, Siân Phillips, Matus Rybak, Sander Schouws, Renske Smit, Laura Sommovigo, Mauro Stefanon, Paul van der Werf
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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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