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Jupiter's atmosphere

The incredible and intricate details of Jupiter's atmosphere, showing storms and clouds, that we one day hope to image on other worlds beyond our Solar System. Image: Seán Doran Flickr https://www.flickr.com/photos/seandoran

Credit: NASA / SwRI / MSSS / Gerald Eichstädt / Seán Doran

Prof Jayne Birkby

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics
  • Instrumentation
  • Exoplanets and planetary physics

Sub department

  • Astrophysics

Research groups

  • Astronomical instrumentation
  • Exoplanet atmospheres
  • Exoplanets and Stellar Physics
  • Planet formation and dynamics
  • Planetary surfaces
  • Extremely Large Telescope
jayne.birkby@physics.ox.ac.uk
Denys Wilkinson Building, room 761
Personal research page
  • About
  • Books
  • Publications

Origins space telescope: from first light to life

Experimental Astronomy Springer 51:3 (2021) 595-624

Authors:

MC Wiedner, S Aalto, L Armus, E Bergin, J Birkby, CM Bradford, D Burgarella, P Caselli, V Charmandaris, A Cooray, E De Beck, JM Desert, M Gerin, J Goicoechea, M Griffin, P Hartogh, F Helmich, M Hogerheijde, L Hunt, A Karska, Q Kral, D Leisawitz, G Melnick, M Meixner, M Matsuura, D Rigopoulou

Abstract:

Abstract The Origins Space Telescope (Origins) is one of four science and technology definition studies selected by the National Aeronautics and Space Administration (NASA) in preparation of the 2020 Astronomy and Astrophysics Decadal survey in the US. Origins will trace the history of our origins from the time dust and heavy elements permanently altered the cosmic landscape to present-day life. It is designed to answer three major science questions: How do galaxies form stars, make metals, and grow their central supermassive black holes from reionization? How do the conditions for habitability develop during the process of planet formation? Do planets orbiting M-dwarf stars support life? Origins operates at mid- to far-infrared wavelengths from ~ 2.8 μm to 588 μm, and is more than 1000 times more sensitive than prior far-IR missions due to its cold (~ 4.5 K) aperture and state-of-the-art instruments.
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High-contrast observations of brown dwarf companion HR 2562 B with the vector Apodizing Phase Plate coronagraph

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 506:3 (2021) 3224-3238

Authors:

Ben J Sutlieff, Alexander J Bohn, Jayne L Birkby, Matthew A Kenworthy, Katie M Morzinski, David S Doelman, Jared R Males, Frans Snik, Laird M Close, Philip M Hinz, David Charbonneau
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Vector-apodizing phase plate coronagraph: design, current performance, and future development [Invited].

Applied Optics Optica Publishing Group 60:19 (2021) d52-d72

Authors:

DS Doelman, F Snik, EH Por, SP Bos, GPPL Otten, M Kenworthy, SY Haffert, M Wilby, AJ Bohn, BJ Sutlieff, K Miller, M Ouellet, J de Boer, CU Keller, MJ Escuti, S Shi, NZ Warriner, K Hornburg, JL Birkby, J Males, KM Morzinski, LM Close, J Codona, J Long, L Schatz, J Lumbres, A Rodack, K Van Gorkom, A Hedglen, O Guyon, J Lozi, T Groff, J Chilcote, N Jovanovic, S Thibault, C de Jonge, G Allain, C Vallée, D Patel, O Côté, C Marois, P Hinz, J Stone, A Skemer, Z Briesemeister, A Boehle, AM Glauser, W Taylor, P Baudoz, E Huby, O Absil, B Carlomagno, C Delacroix
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High-contrast observations of brown dwarf companion HR 2562 B with the vector Apodizing Phase Plate coronagraph

(2021)

Authors:

Ben J Sutlieff, Alexander J Bohn, Jayne L Birkby, Matthew A Kenworthy, Katie M Morzinski, David S Doelman, Jared R Males, Frans Snik, Laird M Close, Philip M Hinz, David Charbonneau
More details from the publisher

The vector-apodizing phase plate coronagraph: design, current performance, and future development

(2021)

Authors:

DS Doelman, F Snik, EH Por, SP Bos, GPPL Otten, M Kenworthy, SY Haffert, M Wilby, AJ Bohn, BJ Sutlieff, K Miller, M Ouellet, J de Boer, CU Keller, MJ Escuti, S Shi, NZ Warriner, KJ Hornburg, JL Birkby, J Males, KM Morzinski, LM Close, J Codona, J Long, L Schatz, J Lumbres, A Rodack, K Van Gorkom, A Hedglen, O Guyon, J Lozi, T Groff, J Chilcote, N Jovanovic, S Thibault, C de Jonge, G Allain, C Vallée, D Patel, O Côté, C Marois, P Hinz, J Stone, A Skemer, Z Briesemeister, A Boehle, AM Glauser, W Taylor, P Baudoz, E Huby, O Absil, B Carlomagno, C Delacroix
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