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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

Supernova simulations and strategies for the dark energy survey

Astrophysical Journal 753:2 (2012)

Authors:

JP Bernstein, R Kessler, S Kuhlmann, R Biswas, E Kovacs, G Aldering, I Crane, CB D'Andrea, DA Finley, JA Frieman, T Hufford, MJ Jarvis, AG Kim, J Marriner, P Mukherjee, RC Nichol, P Nugent, D Parkinson, RRR Reis, M Sako, H Spinka, M Sullivan

Abstract:

We present an analysis of supernova light curves simulated for the upcoming Dark Energy Survey (DES) supernova search. The simulations employ a code suite that generates and fits realistic light curves in order to obtain distance modulus/redshift pairs that are passed to a cosmology fitter. We investigated several different survey strategies including field selection, supernova selection biases, and photometric redshift measurements. Using the results of this study, we chose a 30deg2 search area in the griz filter set. We forecast (1) that this survey will provide a homogeneous sample of up to 4000 TypeIa supernovae in the redshift range 0.05

Herschel-ATLAS: VISTA VIKING near-infrared counterparts in the Phase 1 GAMA 9-h data

\mnras 423 (2012) 2407-2424-2407-2424

Authors:

S Fleuren, W Sutherland, L Dunne, DJB Smith, SJ Maddox, J Gonz谩lez-Nuevo, J Findlay, R Auld, M Baes, NA Bond, DG Bonfield, N Bourne, A Cooray, S Buttiglione, A Cava, A Dariush, G De Zotti, SP Driver, S Dye, S Eales, J Fritz, MLP Gunawardhana, R Hopwood, E Ibar, RJ Ivison, MJ Jarvis, L Kelvin, A Lapi, J Liske, MJ Micha lowski, M Negrello, E Pascale, M Pohlen, M Prescott, EE Rigby, A Robotham, D Scott, P Temi, MA Thompson, E Valiante, PVD Werf

The Spitzer Extragalactic Representative Volume Survey (SERVS): survey definition and goals

ArXiv 1206.406 (2012)

Authors:

J-C Mauduit, M Lacy, D Farrah, JA Surace, M Jarvis, S Oliver, C Maraston, M Vaccari, L Marchetti, G Zeimann, EA Gonzalez-Solares, J Pforr, AO Petric, B Henriques, PA Thomas, J Afonso, A Rettura, G Wilson, JT Falder, JE Geach, M Huynh, RP Norris, N Seymour, GT Richards, SA Stanford, DM Alexander, RH Becker, PN Best, L Bizzocchi, D Bonfield, N Castro, A Cava, S Chapman, N Christopher, DL Clements, G Covone, N Dubois, JS Dunlop, E Dyke, A Edge, HC Ferguson, S Foucaud, A Franceschini, RR Gal, JK Grant, M Grossi, E Hatziminaoglou, S Hickey, JA Hodge, J-S Huang, RJ Ivison, M Kim, O LeFevre, M Lehnert, CJ Lonsdale, LM Lubin, RJ McLure, H Messias, A Martinez-Sansigre, AMJ Mortier, DM Nielsen, M Ouchi, G Parish, I Perez-Fournon, M Pierre, S Rawlings, A Readhead, SE Ridgway, D Rigopoulou, AK Romer, IG Rosebloom, HJA Rottgering, M Rowan-Robinson, A Sajina, CJ Simpson, I Smail, GK Squires, JA Stevens, R Taylor, M Trichas, T Urrutia, E van Kampen, A Verma, CK Xu

Abstract:

We present the Spitzer Extragalactic Representative Volume Survey (SERVS), an 18 square degrees medium-deep survey at 3.6 and 4.5 microns with the post-cryogenic Spitzer Space Telescope to ~2 microJy (AB=23.1) depth of five highly observed astronomical fields (ELAIS-N1, ELAIS-S1, Lockman Hole, Chandra Deep Field South and XMM-LSS). SERVS is designed to enable the study of galaxy evolution as a function of environment from z~5 to the present day, and is the first extragalactic survey both large enough and deep enough to put rare objects such as luminous quasars and galaxy clusters at z>1 into their cosmological context. SERVS is designed to overlap with several key surveys at optical, near- through far-infrared, submillimeter and radio wavelengths to provide an unprecedented view of the formation and evolution of massive galaxies. In this paper, we discuss the SERVS survey design, the data processing flow from image reduction and mosaicing to catalogs, as well as coverage of ancillary data from other surveys in the SERVS fields. We also highlight a variety of early science results from the survey.

Blind Detections of CO J = 1-0 in 11 H-ATLAS Galaxies at z = 2.1-3.5 with the GBT/Zpectrometer

\apj 752 (2012) 152-152

Authors:

AI Harris, AJ Baker, DT Frayer, I Smail, AM Swinbank, DA Riechers, PP van der Werf, R Auld, M Baes, RS Bussmann, S Buttiglione, A Cava, DL Clements, A Cooray, H Dannerbauer, A Dariush, G De Zotti, L Dunne, S Dye, S Eales, J Fritz, J Gonz谩lez-Nuevo, R Hopwood, E Ibar, RJ Ivison, MJ Jarvis, S Maddox, M Negrello, E Rigby, DJB Smith, P Temi, J Wardlow

The evolutionary connection between QSOs and SMGs: molecular gas in far-infrared luminous QSOs at z 2.5

ArXiv e-prints (2012)

Authors:

JM Simpson, I Smail, AM Swinbank, DM Alexander, R Auld, M Baes, DG Bonfield, DL Clements, A Cooray, KEK Coppin, ALR Danielson, A Dariush, L Dunne, G de Zotti, CM Harrison, R Hopwood, C Hoyos, E Ibar, RJ Ivison, MJ Jarvis, A Lapi, SJ Maddox, MJ Page, DA Riechers, E Valiante, PP van der Werf

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