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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.

Christopher Duncan

Visitor

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
  • Euclid
christopher.duncan@physics.ox.ac.uk
Telephone: 01865(2)83016
Denys Wilkinson Building, room 555A
  • About
  • Publications

Euclid preparation

Astronomy & Astrophysics EDP Sciences 631 (2019) a85

Authors:

R Barnett, SJ Warren, DJ Mortlock, J-G Cuby, C Conselice, PC Hewett, CJ Willott, N Auricchio, A Balaguera-Antolínez, M Baldi, S Bardelli, F Bellagamba, R Bender, A Biviano, D Bonino, E Bozzo, E Branchini, M Brescia, J Brinchmann, C Burigana, S Camera, V Capobianco, C Carbone, J Carretero, CS Carvalho, FJ Castander, M Castellano, S Cavuoti, A Cimatti, R Clédassou, G Congedo, L Conversi, Y Copin, L Corcione, J Coupon, HM Courtois, M Cropper, A Da Silva, CAJ Duncan, S Dusini, A Ealet, S Farrens, P Fosalba, S Fotopoulou, N Fourmanoit, M Frailis, M Fumana, S Galeotta, B Garilli, W Gillard, BR Gillis, J Graciá-Carpio, F Grupp, H Hoekstra, F Hormuth, H Israel, K Jahnke, S Kermiche, M Kilbinger, CC Kirkpatrick, T Kitching, R Kohley, B Kubik, M Kunz, H Kurki-Suonio, R Laureijs, S Ligori, PB Lilje, I Lloro, E Maiorano, O Mansutti, O Marggraf, N Martinet, F Marulli, R Massey, N Mauri, E Medinaceli, S Mei, Y Mellier, RB Metcalf, JJ Metge, G Meylan, M Moresco, L Moscardini, E Munari, C Neissner, SM Niemi, T Nutma, C Padilla, S Paltani, F Pasian, P Paykari, WJ Percival, V Pettorino, G Polenta, M Poncet, L Pozzetti, F Raison, A Renzi, J Rhodes, H-W Rix, E Romelli, M Roncarelli, E Rossetti, R Saglia, D Sapone, R Scaramella, P Schneider, V Scottez, A Secroun, S Serrano, G Sirri, L Stanco, F Sureau, P Tallada-Crespí, D Tavagnacco, AN Taylor, M Tenti, I Tereno, R Toledo-Moreo, F Torradeflot, L Valenziano, T Vassallo, Y Wang, A Zacchei, G Zamorani, J Zoubian, E Zucca
More details from the publisher
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CFHTLenS and RCSLenS: testing photometric redshift distributions using angular cross-correlations with spectroscopic galaxy surveys

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 463:4 (2016) 3737-3754

Authors:

A Choi, C Heymans, C Blake, H Hildebrandt, CAJ Duncan, T Erben, R Nakajima, L Van Waerbeke, M Viola
More details from the publisher

Cluster mass profile reconstruction with size and flux magnification on the HST STAGES survey

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 457:1 (2016) 764-785

Authors:

Christopher AJ Duncan, Catherine Heymans, Alan F Heavens, Benjamin Joachimi
More details from the publisher
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On the complementarity of galaxy clustering with cosmic shear and flux magnification

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 437:3 (2014) 2471-2487

Authors:

Christopher AJ Duncan, Benjamin Joachimi, Alan F Heavens, Catherine Heymans, Hendrik Hildebrandt
More details from the publisher

Cosmic magnification as a probe of cosmology

Proceedings of the 47th Rencontres de Moriond on Cosmology 2012 (2012) 173-176

Authors:

C Duncan, A Heavens, B Joachimi, C Heymans

Abstract:

With the wealth of upcoming data from wide-field surveys such as KiDS, Pan-STARRS, DES and Euclid, it is more important than ever to understand the full range of independent probes of cosmology at our disposal. With this in mind, we motivate the use of cosmic magnification as a probe of cosmology, presenting forecasts for the improvements to cosmic shear cosmological parameter constraints when cosmic magnification is included for a KiDS-like survey. We find that when uncertainty in the galaxy bias is factored into the forecasts, cosmic magnification is less powerful that previously reported, but as it is less likely to be prone to measurement error we conclude it is a useful tool for cosmological analyses.

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