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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.

Angela Taylor

Professor of Experimental Astrophysics

Research theme

  • Astronomy and astrophysics
  • Particle astrophysics & cosmology
  • Instrumentation

Sub department

  • Astrophysics

Research groups

  • Experimental radio cosmology
  • C-BASS
  • The Square Kilometre Array (SKA)
Angela.Taylor@physics.ox.ac.uk
Telephone: 01865 (2)73297
Denys Wilkinson Building, room 753
  • About
  • Publications

Optical characterization of OMT-coupled TES bolometers for LiteBIRD

Journal of Low Temperature Physics Springer Nature 209:3-4 (2022) 396-408

Authors:

J Hubmayr, Par Ade, A Adler, E Allys, D Alonso, K Arnold, D Auguste, J Aumont, R Aurlien, Je Austermann, S Azzoni, C Baccigalupi, Aj Banday, R Banerji, Rb Barreiro, N Bartolo, S Basak, E Battistelli, L Bautista, Ja Beall, D Beck, S Beckman, K Benabed, J Bermejo-Ballesteros, M Bersanelli, J Bonis, J Borrill, F Bouchet, F Boulanger, S Bounissou, M Brilenkov, Ml Brown, M Bucher, E Calabrese, M Calvo, P Campeti, A Carones, Fj Casas, A Catalano, A Challinor, V Chan, K Cheung, Y Chinone, C Chiocchetta, Se Clark, L Clermont, S Clesse, J Cliche, F Columbro, Ja Connors

Abstract:

Feedhorn- and orthomode transducer- (OMT) coupled transition edge sensor (TES) bolometers have been designed and micro-fabricated to meet the optical specifications of the LiteBIRD high frequency telescope (HFT) focal plane. We discuss the design and optical characterization of two LiteBIRD HFT detector types: dual-polarization, dual-frequency-band pixels with 195/280 GHz and 235/337 GHz band centers. Results show well-matched passbands between orthogonal polarization channels and frequency centers within 3% of the design values. The optical efficiency of each frequency channel is conservatively reported to be within the range 0.64 - 0.72, determined from the response to a cryogenic, temperature-controlled thermal source. These values are in good agreement with expectations and either exceed or are within 10% of the values used in the LiteBIRD sensitivity forecast. Lastly, we report a measurement of loss in Nb/SiNx/Nb microstrip at 100 mK and over the frequency range 200–350 GHz, which is comparable to values previously reported in the literature.
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A born again 32-meter radio telescope for Mexico

Proceedings of SPIE--the International Society for Optical Engineering SPIE, the international society for optics and photonics 12182 (2022) 121822t-121822t-9

Authors:

Stanley E Kurtz, Angela C Taylor, Michael E Jones, David M Gale, Eduardo Ibarra Medel, Alexander Pollak, Chao Liu
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The C-Band All-Sky Survey (C-BASS): template fitting of diffuse galactic microwave emission in the northern sky

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 513:4 (2022) 5900-5919

Authors:

SE Harper, C Dickinson, A Barr, R Cepeda-Arroita, RDP Grumitt, HM Heilgendorff, L Jew, JL Jonas, ME Jones, JP Leahy, J Leech, TJ Pearson, MW Peel, ACS Readhead, AC Taylor
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The C-Band All-Sky Survey (C-BASS): Template Fitting of Diffuse Galactic Microwave Emission in the Northern Sky

ArXiv 2202.10411 (2022)

Authors:

SE Harper, C Dickinson, A Barr, R Cepeda-Arroita, RDP Grumitt, HM Heilgendorff, L Jew, JL Jonas, ME Jones, JP Leahy, J Leech, TJ Pearson, MW Peel, ACS Readhead, AC Taylor
Details from ArXiV

The LSPE-Strip feed horn array

Journal of Instrumentation IOP Publishing 17:01 (2022) p01029

Authors:

C Franceschet, F Del Torto, F Villa, S Realini, R Bongiolatti, OA Peverini, F Pezzotta, DM Viganó, G Addamo, M Bersanelli, F Cavaliere, F Cuttaia, M Gervasi, A Mennella, G Morgante, AC Taylor, G Virone, M Zannoni
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