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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.

Professor Stephen Smartt CBE FRS MRIA

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Hintze Centre for Astrophysical Surveys
  • Pulsars, transients and relativistic astrophysics
  • Rubin-LSST
stephen.smartt@physics.ox.ac.uk
Telephone: 01865273405
Denys Wilkinson Building, room 714
  • About
  • Publications

Type Ia supernovae with and without blueshifted narrow Na I D lines - how different is their structure?

(2017)

Authors:

Stephan Hachinger, Friedrich K Roepke, Paolo A Mazzali, Avishay Gal-Yam, Kate Maguire, Mark Sullivan, Stefan Taubenberger, Chris Ashall, Heather Campbell, Nancy Elias-Rosa, Ulrich Feindt, Laura Greggio, Cosimo Inserra, Matteo Miluzio, Stephen J Smartt, David Young
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A transient search using combined human and machine classifications

Monthly Notices of the Royal Astronomical Society Oxford University Press 472:2 (2017) 1315-1323

Authors:

DE Wright, Christopher J Lintott, SJ Smartt, KW Smith, L Fortson, L Trouille, Campbell R Allen, M Beck, MC Bouslog, A Boyer, KC Chambers, H Flewelling, W Granger, EA Magnier, A McMaster, Grant RM Miller, James E O'Donnell, B Simmons, Helen R Spiers, JL Tonry, Marten Veldthuis, RJ Wainscoat, C Waters, M Willman, Z Wolfenbarger

Abstract:

Large modern surveys require efficient review of data in order to find transient sources such as supernovae, and to distinguish such sources from artefacts and noise. Much effort has been put into the development of automatic algorithms, but surveys still rely on human review of targets. This paper presents an integrated system for the identification of supernovae in data from Pan-STARRS1, combining classifications from volunteers participating in a citizen science project with those from a convolutional neural network. The unique aspect of this work is the deployment, in combination, of both human and machine classifications for near real-time discovery in an astronomical project. We show that the combination of the two methods outperforms either one used individually. This result has important implications for the future development of transient searches, especially in the era of LSST and other large-throughput surveys.
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Observations of the GRB afterglow ATLAS17aeu and its possible association with GW170104

(2017)

Authors:

B Stalder, J Tonry, SJ Smartt, M Coughlin, KC Chambers, CW Stubbs, T-W Chen, E Kankare, KW Smith, L Denneau, A Sherstyuk, A Heinze, H Weiland, A Rest, DR Young, ME Huber, H Flewelling, T Lowe, EA Magnier, ASB Schultz, C Waters, R Wainscoat, M Willman, DE Wright, JK Chu, D Sanders, C Inserra, K Maguire, R Kotak
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OGLE-2014-SN-131: A long-rising Type Ibn supernova from a massive progenitor ⋆

Astronomy & Astrophysics EDP Sciences 602 (2017) a93

Authors:

E Karamehmetoglu, F Taddia, J Sollerman, Ł Wyrzykowski, S Schmidl, M Fraser, C Fremling, J Greiner, C Inserra, Z Kostrzewa-Rutkowska, K Maguire, S Smartt, M Sullivan, DR Young
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The evolution of superluminous supernova LSQ14mo and its interacting host galaxy system ⋆

Astronomy & Astrophysics EDP Sciences 602 (2017) a9

Authors:

T-W Chen, M Nicholl, SJ Smartt, PA Mazzali, RM Yates, TJ Moriya, C Inserra, N Langer, T Krühler, Y-C Pan, R Kotak, L Galbany, P Schady, P Wiseman, J Greiner, S Schulze, AWS Man, A Jerkstrand, KW Smith, M Dennefeld, C Baltay, J Bolmer, E Kankare, F Knust, K Maguire, D Rabinowitz, S Rostami, M Sullivan, DR Young
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