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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

JWST PRIMER: a lack of outshining in four normal z = 4 − 6 galaxies from the ALMA-CRISTAL Survey

Monthly Notices of the Royal Astronomical Society Oxford University Press 539:3 (2025) 2685-2706

Authors:

NEP Lines, RAA Bowler, NJ Adams, R Fisher, RG Varadaraj, Y Nakazato, M Aravena, RJ Assef, JE Birkin, D Ceverino, E da Cunha, F Cullen, I De Looze, CT Donnan, JS Dunlop, A Ferrara, NA Grogin, R Herrera-Camus, R Ikeda, AM Koekemoer, M Killi, J Li, DJ McLeod, RJ McLure

Abstract:

We present a spatially resolved analysis of four star-forming galaxies at using data from the JWST Public Release Imaging for Extragalactic Research (PRIMER) and ALMA-[C II] Resolved ISm in STar-forming galaxies with ALma (CRISTAL) surveys to probe the stellar and interstellar medium properties on the sub- scale. In the JWST NIRCam imaging we find that the galaxies are composed of multiple clumps (between 2 and ∼8) separated by , with comparable morphologies and sizes in the rest-frame ultraviolet (UV) and optical. Using BAGPIPES to perform pixel-by-pixel spectral energy distribution (SED) fitting to the JWST data, we show that the star formation rate (SFR) () and stellar mass ( ) derived from the resolved analysis are in close () agreement with those obtained by fitting the integrated photometry. In contrast to studies of lower mass sources, we thus find a reduced impact of outshining of the older (more massive) stellar populations in these normal galaxies. Our JWST analysis recovers bluer rest-frame UV slopes () and younger ages () than archival values. We find that the dust continuum from ALMA-CRISTAL seen in two of these galaxies correlates, as expected, with regions of redder rest-frame UV slopes and the SED-derived , as well as the peak in the stellar mass map. We compute the resolved –relation, showing that the IRX is consistent with the local starburst attenuation curve and further demonstrating the presence of an inhomogeneous dust distribution within the galaxies. A comparison of the CRISTAL sources to those from the FirstLight zoom-in simulation of galaxies with the same and SFR reveals similar age and colour gradients, suggesting that major mergers may be important in the formation of clumpy galaxies at this epoch.
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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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