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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.

Aprajita Verma

Associate Professor

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Zooniverse
  • Astronomical instrumentation
  • Galaxy formation and evolution
  • Hintze Centre for Astrophysical Surveys
  • MeerKAT
  • Rubin-LSST
  • Extremely Large Telescope
aprajita.verma@physics.ox.ac.uk
Telephone: 01865 (2)73374
Denys Wilkinson Building, room 760
  • About
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  • Teaching
  • Publications

Space Warps: I. Crowd-sourcing the discovery of gravitational lenses

Monthly Notices of the Royal Astronomical Society Oxford University Press 455:2 (2015) 1171-1190

Authors:

Philip J Marshall, Aprajita Verma, Anupreeta More, Christopher P Davis, Surhud More, Amit Kapadia, Michael Parrish, Chris Snyder, Julianne Wilcox, Christine Macmillan, Elisabeth Baeten, Michael Baumer, Claude Cornen, Edwin Simpson, Chris J Lintott, David Miller, Edward Paget, Robert Simpson, Arfon M Smith, Rafael K眉ng, Thomas E Collett, Prasenjit Saha

Abstract:

We describe SpaceWarps, a novel gravitational lens discovery service that yields samples of high purity and completeness through crowd-sourced visual inspection. Carefully produced colour composite images are displayed to volunteers via a webbased classification interface, which records their estimates of the positions of candidate lensed features. Images of simulated lenses, as well as real images which lack lenses, are inserted into the image stream at random intervals; this training set is used to give the volunteers instantaneous feedback on their performance, as well as to calibrate a model of the system that provides dynamical updates to the probability that a classified image contains a lens. Low probability systems are retired from the site periodically, concentrating the sample towards a set of lens candidates. Having divided 160 square degrees of Canada-France-Hawaii Telescope Legacy Survey (CFHTLS) imaging into some 430,000 overlapping 82 by 82 arcsecond tiles and displaying them on the site, we were joined by around 37,000 volunteers who contributed 11 million image classifications over the course of 8 months. This Stage 1 search reduced the sample to 3381 images containing candidates; these were then refined in Stage 2 to yield a sample that we expect to be over 90% complete and 30% pure, based on our analysis of the volunteers performance on training images. We comment on the scalability of the SpaceWarps system to the wide field survey era, based on our projection that searches of 105 images could be performed by a crowd of 105 volunteers in 6 days.

A DEEP HERSCHEL/PACS OBSERVATION OF CO(40-39) IN NGC 1068: A SEARCH FOR THE MOLECULAR TORUS

The Astrophysical Journal American Astronomical Society 811:2 (2015) 74

Authors:

AW Janssen, S Bruderer, E Sturm, A Contursi, R Davies, S Hailey-Dunsheath, A Poglitsch, R Genzel, J Graci谩-Carpio, D Lutz, L Tacconi, J Fischer, E Gonz谩lez-Alfonso, A Sternberg, S Veilleux, A Verma, L Burtscher

The Red Radio Ring: a gravitationally lensed hyperluminous infrared radio galaxy at z = 2.553 discovered through the citizen science project Space Warps

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 452:1 (2015) 502-510

Authors:

JE Geach, A More, A Verma, PJ Marshall, N Jackson, P-E Belles, R Beswick, E Baeten, M Chavez, C Cornen, BE Cox, T Erben, NJ Erickson, S Garrington, PA Harrison, K Harrington, DH Hughes, RJ Ivison, C Jordan, Y-T Lin, A Leauthaud, C Lintott, S Lynn, A Kapadia, J-P Kneib, C Macmillan, M Makler, G Miller, A Monta帽a, R Mujica, T Muxlow, G Narayanan, D脫 Briain, T O'Brien, M Oguri, E Paget, M Parrish, NP Ross, E Rozo, CE Rusu, ES Rykoff, D Sanchez-Arg眉elles, R Simpson, C Snyder, FP Schloerb, M Tecza, W-H Wang, L Van Waerbeke, J Wilcox, M Viero, GW Wilson, MS Yun, M Zeballos

A multiwavelength exploration of the [C ii]/IR ratio in H-ATLAS/GAMA galaxies out to z = 0.2

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 449:3 (2015) 2498-2513

Authors:

E Ibar, MA Lara-L贸pez, R Herrera-Camus, R Hopwood, A Bauer, RJ Ivison, MJ Micha艂owski, H Dannerbauer, P van der Werf, D Riechers, N Bourne, M Baes, I Valtchanov, L Dunne, A Verma, S Brough, A Cooray, G De Zotti, S Dye, S Eales, C Furlanetto, S Maddox, M Smith, O Steele, D Thomas, E Valiante

HIGH-J CO SLEDs IN NEARBY INFRARED BRIGHT GALAXIES OBSERVED BY HERSCHEL/PACS* * Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA.

The Astrophysical Journal American Astronomical Society 802:2 (2015) 81

Authors:

N Mashian, E Sturm, A Sternberg, A Janssen, S Hailey-Dunsheath, J Fischer, A Contursi, E Gonz谩lez-Alfonso, J Graci谩-Carpio, A Poglitsch, S Veilleux, R Davies, R Genzel, D Lutz, L Tacconi, A Verma, A Wei脽, E Polisensky, T Nikola

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