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1
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Ahrer EM, Stevenson KB, Mansfield M, Moran SE, Brande J, Morello G, Murray CA, Nikolov NK, Petit Dit de la Roche DJM, Schlawin E, Wheatley PJ, Zieba S, Batalha NE, Damiano M, Goyal JM, Lendl M, Lothringer JD, Mukherjee S, Ohno K, Batalha NM, Battley MP, Bean JL, Beatty TG, Benneke B, Berta-Thompson ZK, Carter AL, Cubillos PE, Daylan T, Espinoza N, Gao P, Gibson NP, Gill S, Harrington J, Hu R, Kreidberg L, Lewis NK, Line MR, López-Morales M, Parmentier V, Powell DK, Sing DK, Tsai SM, Wakeford HR, Welbanks L, Alam MK, Alderson L, Allen NH, Anderson DR, Barstow JK, Bayliss D, Bell TJ, Blecic J, Bryant EM, Burleigh MR, Carone L, Casewell SL, Changeat Q, Chubb KL, Crossfield IJM, Crouzet N, Decin L, Désert JM, Feinstein AD, Flagg L, Fortney JJ, Gizis JE, Heng K, Iro N, Kempton EMR, Kendrew S, Kirk J, Knutson HA, Komacek TD, Lagage PO, Leconte J, Lustig-Yaeger J, MacDonald RJ, Mancini L, May EM, Mayne NJ, Miguel Y, Mikal-Evans T, Molaverdikhani K, Palle E, Piaulet C, Rackham BV, Redfield S, Rogers LK, Roy PA, Rustamkulov Z, Shkolnik EL, Sotzen KS, Taylor J, Tremblin P, Tucker GS, Turner JD, de Val-Borro M, Venot O, Zhang X. Early Release Science of the exoplanet WASP-39b with JWST NIRCam. Nature 2023; 614:653-658. [PMID: 36623551 PMCID: PMC9946836 DOI: 10.1038/s41586-022-05590-4] [Citation(s) in RCA: 2] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/16/2022] [Accepted: 11/24/2022] [Indexed: 01/11/2023]
Abstract
Measuring the metallicity and carbon-to-oxygen (C/O) ratio in exoplanet atmospheres is a fundamental step towards constraining the dominant chemical processes at work and, if in equilibrium, revealing planet formation histories. Transmission spectroscopy (for example, refs. 1,2) provides the necessary means by constraining the abundances of oxygen- and carbon-bearing species; however, this requires broad wavelength coverage, moderate spectral resolution and high precision, which, together, are not achievable with previous observatories. Now that JWST has commenced science operations, we are able to observe exoplanets at previously uncharted wavelengths and spectral resolutions. Here we report time-series observations of the transiting exoplanet WASP-39b using JWST's Near InfraRed Camera (NIRCam). The long-wavelength spectroscopic and short-wavelength photometric light curves span 2.0-4.0 micrometres, exhibit minimal systematics and reveal well defined molecular absorption features in the planet's spectrum. Specifically, we detect gaseous water in the atmosphere and place an upper limit on the abundance of methane. The otherwise prominent carbon dioxide feature at 2.8 micrometres is largely masked by water. The best-fit chemical equilibrium models favour an atmospheric metallicity of 1-100-times solar (that is, an enrichment of elements heavier than helium relative to the Sun) and a substellar C/O ratio. The inferred high metallicity and low C/O ratio may indicate significant accretion of solid materials during planet formation (for example, refs. 3,4,) or disequilibrium processes in the upper atmosphere (for example, refs. 5,6).
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Affiliation(s)
- Eva-Maria Ahrer
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK.
- Department of Physics, University of Warwick, Coventry, UK.
| | | | | | - Sarah E Moran
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
| | - Jonathan Brande
- Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | - Giuseppe Morello
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Departamento de Astrofísica, Universidad de La Laguna (ULL), Tenerife, Spain
- INAF- Palermo Astronomical Observatory, Piazza del Parlamento, Palermo, Italy
| | - Catriona A Murray
- Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO, USA
| | | | | | | | - Peter J Wheatley
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - Sebastian Zieba
- Max Planck Institute for Astronomy, Heidelberg, Germany
- Leiden Observatory, University of Leiden, Leiden, The Netherlands
| | | | | | - Jayesh M Goyal
- School of Earth and Planetary Sciences (SEPS), National Institute of Science Education and Research (NISER), HBNI, Jatani, India
| | - Monika Lendl
- Département d'Astronomie, Université de Genève, Sauverny, Switzerland
| | | | - Sagnick Mukherjee
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Kazumasa Ohno
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Natalie M Batalha
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
- Astrobiology Program, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Matthew P Battley
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - Jacob L Bean
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - Thomas G Beatty
- Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA
| | - Björn Benneke
- Department of Physics and Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | | | - Aarynn L Carter
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Patricio E Cubillos
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
- INAF - Osservatorio Astrofisico di Torino, Pino Torinese, Italy
| | - Tansu Daylan
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | - Néstor Espinoza
- Space Telescope Science Institute, Baltimore, MD, USA
- Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | - Peter Gao
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington DC, USA
| | - Neale P Gibson
- School of Physics, Trinity College Dublin, Dublin, Ireland
| | - Samuel Gill
- Department of Physics, University of Warwick, Coventry, UK
| | - Joseph Harrington
- Planetary Sciences Group, Department of Physics and Florida Space Institute, University of Central Florida, Orlando, FL, USA
| | - Renyu Hu
- Astrophysics Section, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | | | - Nikole K Lewis
- Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | - Michael R Line
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | | | - Vivien Parmentier
- Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
- Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France
| | - Diana K Powell
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA
| | - David K Sing
- Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
| | - Shang-Min Tsai
- Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
| | | | - Luis Welbanks
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Munazza K Alam
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington DC, USA
| | - Lili Alderson
- School of Physics, University of Bristol, Bristol, UK
| | - Natalie H Allen
- Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | - David R Anderson
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - Joanna K Barstow
- School of Physical Sciences, The Open University, Milton Keynes, UK
| | - Daniel Bayliss
- Department of Physics, University of Warwick, Coventry, UK
| | - Taylor J Bell
- BAER Institute, NASA Ames Research Center, Moffet Field, CA, USA
| | - Jasmina Blecic
- Department of Physics, New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
- Center for Astro, Particle and Planetary Physics (CAP3), New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
| | - Edward M Bryant
- Mullard Space Science Laboratory, University College London, Dorking, UK
| | | | - Ludmila Carone
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - S L Casewell
- School of Physics and Astronomy, University of Leicester, Leicester, UK
| | - Quentin Changeat
- Space Telescope Science Institute, Baltimore, MD, USA
- European Space Agency, Space Telescope Science Institute, Baltimore, MD, USA
- Department of Physics and Astronomy, University College London, London, UK
| | - Katy L Chubb
- Centre for Exoplanet Science, University of St Andrews, St Andrews, UK
| | - Ian J M Crossfield
- Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | - Nicolas Crouzet
- Leiden Observatory, Leiden University, Leiden, The Netherlands
| | - Leen Decin
- Institute of Astronomy, Department of Physics and Astronomy, KU Leuven, Leuven, Belgium
| | - Jean-Michel Désert
- Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, The Netherlands
| | - Adina D Feinstein
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - Laura Flagg
- Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | - Jonathan J Fortney
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - John E Gizis
- Department of Physics and Astronomy, University of Delaware, Newark, DE, USA
| | - Kevin Heng
- Department of Physics, University of Warwick, Coventry, UK
- University Observatory Munich, Ludwig Maximilian University, Munich, Germany
- ARTORG Center for Biomedical Engineering, University of Bern, Bern, Switzerland
| | - Nicolas Iro
- Institute for Astrophysics, University of Vienna, Vienna, Austria
| | - Eliza M-R Kempton
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Sarah Kendrew
- European Space Agency, Space Telescope Science Institute, Baltimore, MD, USA
| | - James Kirk
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA
- Department of Physics, Imperial College London, London, UK
| | - Heather A Knutson
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | | | - Pierre-Olivier Lagage
- Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France
| | - Jérémy Leconte
- Laboratoire d'Astrophysique de Bordeaux, Université de Bordeaux, Pessac, France
| | | | - Ryan J MacDonald
- Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | - Luigi Mancini
- Max Planck Institute for Astronomy, Heidelberg, Germany
- Department of Physics, University of Rome "Tor Vergata", Rome, Italy
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | - E M May
- Johns Hopkins APL, Laurel, MD, USA
| | - N J Mayne
- Department of Physics and Astronomy, University of Exeter, Exeter, UK
| | - Yamila Miguel
- Leiden Observatory, University of Leiden, Leiden, The Netherlands
- SRON Netherlands Institute for Space Research, Leiden, The Netherlands
| | | | - Karan Molaverdikhani
- Max Planck Institute for Astronomy, Heidelberg, Germany
- University Observatory Munich, Ludwig Maximilian University, Munich, Germany
- Exzellenzcluster Origins, Garching, Germany
| | - Enric Palle
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
| | - Caroline Piaulet
- Department of Physics and Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | - Benjamin V Rackham
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Seth Redfield
- Astronomy Department and Van Vleck Observatory, Wesleyan University, Middletown, CT, USA
| | - Laura K Rogers
- Institute of Astronomy, University of Cambridge, Cambridge, UK
| | - Pierre-Alexis Roy
- Department of Physics and Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | - Zafar Rustamkulov
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
| | - Evgenya L Shkolnik
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Kristin S Sotzen
- Johns Hopkins APL, Laurel, MD, USA
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
| | - Jake Taylor
- Department of Physics and Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
- Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
| | - P Tremblin
- Maison de la Simulation, CEA, CNRS, Univ. Paris-Sud, UVSQ, Université Paris-Saclay, Gif-sur-Yvette, France
| | | | - Jake D Turner
- Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | | | - Olivia Venot
- Université de Paris Cité and Univ Paris Est Creteil, CNRS, LISA, Paris, France
| | - Xi Zhang
- Department of Earth and Planetary Sciences, University of California, Santa Cruz, Santa Cruz, CA, USA
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2
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Rustamkulov Z, Sing DK, Mukherjee S, May EM, Kirk J, Schlawin E, Line MR, Piaulet C, Carter AL, Batalha NE, Goyal JM, López-Morales M, Lothringer JD, MacDonald RJ, Moran SE, Stevenson KB, Wakeford HR, Espinoza N, Bean JL, Batalha NM, Benneke B, Berta-Thompson ZK, Crossfield IJM, Gao P, Kreidberg L, Powell DK, Cubillos PE, Gibson NP, Leconte J, Molaverdikhani K, Nikolov NK, Parmentier V, Roy P, Taylor J, Turner JD, Wheatley PJ, Aggarwal K, Ahrer E, Alam MK, Alderson L, Allen NH, Banerjee A, Barat S, Barrado D, Barstow JK, Bell TJ, Blecic J, Brande J, Casewell S, Changeat Q, Chubb KL, Crouzet N, Daylan T, Decin L, Désert J, Mikal-Evans T, Feinstein AD, Flagg L, Fortney JJ, Harrington J, Heng K, Hong Y, Hu R, Iro N, Kataria T, Kempton EMR, Krick J, Lendl M, Lillo-Box J, Louca A, Lustig-Yaeger J, Mancini L, Mansfield M, Mayne NJ, Miguel Y, Morello G, Ohno K, Palle E, Petit Dit de la Roche DJM, Rackham BV, Radica M, Ramos-Rosado L, Redfield S, Rogers LK, Shkolnik EL, Southworth J, Teske J, Tremblin P, Tucker GS, Venot O, Waalkes WC, Welbanks L, Zhang X, Zieba S. Early Release Science of the exoplanet WASP-39b with JWST NIRSpec PRISM. Nature 2023; 614:659-663. [PMID: 36623548 PMCID: PMC9946832 DOI: 10.1038/s41586-022-05677-y] [Citation(s) in RCA: 7] [Impact Index Per Article: 7.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Key Words] [Grants] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/22/2022] [Accepted: 12/21/2022] [Indexed: 01/11/2023]
Abstract
Transmission spectroscopy1-3 of exoplanets has revealed signatures of water vapour, aerosols and alkali metals in a few dozen exoplanet atmospheres4,5. However, these previous inferences with the Hubble and Spitzer Space Telescopes were hindered by the observations' relatively narrow wavelength range and spectral resolving power, which precluded the unambiguous identification of other chemical species-in particular the primary carbon-bearing molecules6,7. Here we report a broad-wavelength 0.5-5.5 µm atmospheric transmission spectrum of WASP-39b8, a 1,200 K, roughly Saturn-mass, Jupiter-radius exoplanet, measured with the JWST NIRSpec's PRISM mode9 as part of the JWST Transiting Exoplanet Community Early Release Science Team Program10-12. We robustly detect several chemical species at high significance, including Na (19σ), H2O (33σ), CO2 (28σ) and CO (7σ). The non-detection of CH4, combined with a strong CO2 feature, favours atmospheric models with a super-solar atmospheric metallicity. An unanticipated absorption feature at 4 µm is best explained by SO2 (2.7σ), which could be a tracer of atmospheric photochemistry. These observations demonstrate JWST's sensitivity to a rich diversity of exoplanet compositions and chemical processes.
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Affiliation(s)
- Z Rustamkulov
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA.
| | - D K Sing
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
- Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | - S Mukherjee
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - E M May
- Johns Hopkins APL, Laurel, MD, USA
| | - J Kirk
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
- Department of Physics, Imperial College London, London, UK
| | - E Schlawin
- Steward Observatory, University of Arizona, Tucson, AZ, USA
| | - M R Line
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - C Piaulet
- Institute of Research on Exoplanets, Department of Physics, University of Montreal, Montreal, Québec, Canada
| | - A L Carter
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - N E Batalha
- NASA Ames Research Center, Moffett Field, CA, USA
| | - J M Goyal
- School of Earth and Planetary Sciences, National Institute of Science Education and Research (NISER), HBNI, Jatani, India
| | - M López-Morales
- Center for Astrophysics, Harvard and Smithsonian, Cambridge, MA, USA
| | - J D Lothringer
- Department of Physics, Utah Valley University, Orem, UT, USA
| | - R J MacDonald
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
- Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | - S E Moran
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
| | | | - H R Wakeford
- School of Physics, University of Bristol, HH Wills Physics Laboratory, Bristol, UK
| | - N Espinoza
- Space Telescope Science Institute, Baltimore, MD, USA
| | - J L Bean
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - N M Batalha
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - B Benneke
- Institute of Research on Exoplanets, Department of Physics, University of Montreal, Montreal, Québec, Canada
| | - Z K Berta-Thompson
- Department of Astrophysical and Planetary Sciences, University of Colorado, Boulder, CO, USA
| | - I J M Crossfield
- Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | - P Gao
- Earth and Planets Laboratory, Carnegie Institution of Washington, Washington, DC, USA
| | - L Kreidberg
- Max Planck Institute for Astronomy, Heidelberg, Germany
| | - D K Powell
- Harvard and Smithsonian, Center for Astrophysics, Cambridge, MA, USA
| | - P E Cubillos
- INAF - Astrophysics Observatory at Turin, Turin, Italy
| | - N P Gibson
- School of Physics, Trinity College Dublin, Dublin, Ireland
| | - J Leconte
- Laboratoire d'Astrophysique de Bordeaux, CNRS, Université de Bordeaux, Pessac, France
| | - K Molaverdikhani
- University Observatory Munich, Ludwig Maximilian University, Munich, Germany
- Exzellenzcluster Origins, Garching, Germany
| | - N K Nikolov
- Space Telescope Science Institute, Baltimore, MD, USA
| | - V Parmentier
- Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France
- Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
| | - P Roy
- Institute of Research on Exoplanets, Department of Physics, University of Montreal, Montreal, Québec, Canada
| | - J Taylor
- Department of Physics, University of Oxford, Oxford, UK
| | - J D Turner
- Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | - P J Wheatley
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - K Aggarwal
- Indian Institute of Technology, Indore, Indore, India
| | - E Ahrer
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - M K Alam
- Earth and Planets Laboratory, Carnegie Institution of Washington, Washington, DC, USA
| | - L Alderson
- School of Physics, University of Bristol, HH Wills Physics Laboratory, Bristol, UK
| | - N H Allen
- Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | - A Banerjee
- School of Physical Sciences, The Open University, Milton Keynes, UK
| | - S Barat
- Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, the Netherlands
| | - D Barrado
- Centre for Astrobiology (CSIC-INTA), European Space Astronomy Centre Campus, University of Maria de Maeztu, Madrid, Spain
| | - J K Barstow
- School of Physical Sciences, The Open University, Milton Keynes, UK
| | - T J Bell
- BAER Institute, NASA Ames Research Center, Moffet Field, Mountain View, CA, USA
| | - J Blecic
- New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
- Center for Astro, Particle and Planetary Physics (CAP3), New York University Abu Dhabi, Abu Dhabi, UAE
| | - J Brande
- Department of Physics and Astronomy, University of Kansas, Lawrence, KS, USA
| | - S Casewell
- School of Physics and Astronomy, University of Leicester, Leicester, UK
| | - Q Changeat
- Space Telescope Science Institute, Baltimore, MD, USA
- European Space Agency (ESA), ESA Baltimore Office, Baltimore, MD, USA
- Department of Physics and Astronomy, University College London, London, UK
| | - K L Chubb
- Centre for Exoplanet Science, University of St Andrews, St Andrews, UK
| | - N Crouzet
- Leiden Observatory, Leiden University, Leiden, the Netherlands
| | - T Daylan
- Department of Astrophysical Sciences, Princeton University, Princeton, NJ, USA
| | - L Decin
- Department of Physics and Astronomy, KU Leuven, Leuven, Belgium
| | - J Désert
- Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, the Netherlands
| | - T Mikal-Evans
- Max Planck Institute for Astronomy, Heidelberg, Germany
| | - A D Feinstein
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
- School of Physical Sciences, The Open University, Milton Keynes, UK
| | - L Flagg
- Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | - J J Fortney
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - J Harrington
- Planetary Science Group, Department of Physics and Florida Space Institute, University of Central Florida, Orlando, FL, USA
| | - K Heng
- University Observatory Munich, Ludwig Maximilian University, Munich, Germany
| | - Y Hong
- Department of Astronomy and Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | - R Hu
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - N Iro
- Institute for Astrophysics, University of Vienna, Vienna, Austria
| | - T Kataria
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - E M-R Kempton
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - J Krick
- California Institute of Technology, IPAC, Pasadena, CA, USA
| | - M Lendl
- Department of Astronomy, University of Geneva, Geneva, Switzerland
| | - J Lillo-Box
- Centre for Astrobiology (CSIC-INTA), European Space Astronomy Centre Campus, University of Maria de Maeztu, Madrid, Spain
| | - A Louca
- Leiden Observatory, Leiden University, Leiden, the Netherlands
| | | | - L Mancini
- Max Planck Institute for Astronomy, Heidelberg, Germany
- INAF - Astrophysics Observatory at Turin, Turin, Italy
- Department of Physics, University of Rome 'Tor Vergata', Rome, Italy
| | - M Mansfield
- Steward Observatory, University of Arizona, Tucson, AZ, USA
| | - N J Mayne
- Department of Physics and Astronomy, Faculty of Environment, Science and Economy, University of Exeter, Exeter, UK
| | - Y Miguel
- Leiden Observatory, Leiden University, Leiden, the Netherlands
- SRON Netherlands Institute for Space Research, Leiden, the Netherlands
| | - G Morello
- Institute for Astrophysics of Canarias (IAC), La Laguna, Tenerife, Spain
- Department of Astrophysics, University of La Laguna, La Laguna, Tenerife, Spain
- INAF Äì Palermo Astronomical Observatory, Palermo, Italy
| | - K Ohno
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - E Palle
- Institute for Astrophysics of Canarias (IAC), La Laguna, Tenerife, Spain
| | | | - B V Rackham
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - M Radica
- Institute of Research on Exoplanets, Department of Physics, University of Montreal, Montreal, Québec, Canada
| | - L Ramos-Rosado
- Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | - S Redfield
- Astronomy Department and Van Vleck Observatory, Wesleyan University, Middletown, CT, USA
| | - L K Rogers
- Institute of Astronomy, University of Cambridge, Cambridgeshire, UK
| | - E L Shkolnik
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - J Southworth
- Astrophysics Group, Keele University, Staffordshire, UK
| | - J Teske
- Earth and Planets Laboratory, Carnegie Institution of Washington, Washington, DC, USA
| | - P Tremblin
- UVSQ, CNRS, CEA, Maison de la Simulation, Université Paris-Saclay, Gif-sur-Yvette, France
| | - G S Tucker
- Department of Physics, Brown University, Providence, RI, USA
| | - O Venot
- Université de Paris Cité and Univ Paris Est Creteil, CNRS, LISA, Paris, France
| | - W C Waalkes
- Astrophysics and Planetary Sciences, University of Colorado Boulder, Boulder, CO, USA
| | - L Welbanks
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - X Zhang
- Department of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz, CA, USA
| | - S Zieba
- Max Planck Institute for Astronomy, Heidelberg, Germany
- Leiden Observatory, Leiden University, Leiden, the Netherlands
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Raslau FD, Lin LY, Andersen AH, Powell DK, Smith CD, Escott EJ. Peeking into the Black Box of Coregistration in Clinical fMRI: Which Registration Methods Are Used and How Well Do They Perform? AJNR Am J Neuroradiol 2018; 39:2332-2339. [PMID: 30361428 DOI: 10.3174/ajnr.a5846] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/09/2018] [Accepted: 08/25/2018] [Indexed: 11/07/2022]
Abstract
BACKGROUND AND PURPOSE Interpretation of fMRI depends on accurate functional-to-structural alignment. This study explores registration methods used by FDA-approved software for clinical fMRI and aims to answer the following question: What is the degree of misalignment when registration is not performed, and how well do current registration methods perform? MATERIALS AND METHODS This retrospective study of presurgical fMRI for brain tumors compares nonregistered images and 5 registration cost functions: Hellinger, mutual information, normalized mutual information, correlation ratio, and local Pearson correlation. To adjudicate the accuracy of coregistration, we edge-enhanced echo-planar maps and rated them for alignment with structural anatomy. Lesion-to-activation distances were measured to evaluate the effects of different cost functions. RESULTS Transformation parameters were congruent among Hellinger, mutual information, normalized mutual information, and the correlation ratio but divergent from the local Pearson correlation. Edge-enhanced images validated the local Pearson correlation as the most accurate. Hellinger worsened misalignment in 59% of cases, primarily exaggerating the inferior translation; no cases were worsened by the local Pearson correlation. Three hundred twenty lesion-to-activation distances from 25 patients were analyzed among nonregistered images, Hellinger, and the local Pearson correlation. ANOVA analysis revealed significant differences in the coronal (P < .001) and sagittal (P = .04) planes. If registration is not performed, 8% of cases may have a >3-mm discrepancy and up to a 5.6-mm lesion-to-activation distance difference. If a poor registration method is used, 23% of cases may have a >3-mm discrepancy and up to a 6.9-mm difference. CONCLUSIONS The local Pearson correlation is a special-purpose cost function specifically designed for T2*-T1 coregistration and should be more widely incorporated into software tools as a better method for coregistration in clinical fMRI.
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Affiliation(s)
- F D Raslau
- From the Departments of Radiology (F.D.R., L.Y.L., E.J.E., C.D.S.)
| | - L Y Lin
- From the Departments of Radiology (F.D.R., L.Y.L., E.J.E., C.D.S.)
| | | | | | - C D Smith
- From the Departments of Radiology (F.D.R., L.Y.L., E.J.E., C.D.S.)
- Neurology (C.D.S.)
- Neuroscience (A.H.A., D.K.P., C.D.S.)
| | - E J Escott
- From the Departments of Radiology (F.D.R., L.Y.L., E.J.E., C.D.S.)
- Otolaryngology-Head & Neck Surgery (E.J.E.), University of Kentucky, Lexington, Kentucky
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Whang JS, Kolber M, Powell DK, Libfeld E. Diffusion-weighted signal patterns of intracranial haemorrhage. Clin Radiol 2015; 70:909-16. [PMID: 26050534 DOI: 10.1016/j.crad.2015.04.006] [Citation(s) in RCA: 18] [Impact Index Per Article: 2.0] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/02/2014] [Revised: 03/26/2015] [Accepted: 04/15/2015] [Indexed: 01/08/2023]
Abstract
The signal pattern of intracranial haemorrhage on diffusion-weighted imaging (DWI) as it evolves over time is rarely discussed due to the sensitivity of T2*-weighted sequences and the specificity of classic signal patterns on T1 and T2-weighted sequences. The DWI signal is strongly affected by the magnetic susceptibility of paramagnetic blood products and, therefore, is markedly hypointense in the same phases that demonstrate hypointensity on T2*-weighted sequences; however, hyperacute haemorrhage (oxyhaemoglobin-predominant clot) and late subacute haemorrhage (extracellular methaemoglobin) do not demonstrate T2* hypointensity. Moreover, T2*-weighted sequences are less sensitive to the presence of extra-axial haemorrhage than to intraparenchymal haemorrhage. At these stages of evolution, haemorrhage demonstrates high DWI signal in association with low ADC values, which may be more pronounced than even its corresponding fluid-attenuated inversion recovery (FLAIR) signal. DWI is useful for identifying hyperacute subarachnoid haemorrhage and as a problem-solving tool in challenging cases.
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Affiliation(s)
- J S Whang
- Department of Radiology Mount Sinai Beth Israel Medical Center, New York, NY, USA.
| | - M Kolber
- Department of Radiology Mount Sinai Beth Israel Medical Center, New York, NY, USA
| | - D K Powell
- Department of Radiology New York Presbyterian, Columbia Campus, New York, NY, USA
| | - E Libfeld
- Department of Radiology Mount Sinai Beth Israel Medical Center, New York, NY, USA
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Powell DK, Nwoke F, Urken ML, Buchbinder D, Jacobson AS, Silberzweig JE, Khorsandi AS. Scapular free flap harvest site: recognising the spectrum of radiographic post-operative appearance. Br J Radiol 2013; 86:20120574. [PMID: 23392191 DOI: 10.1259/bjr.20120574] [Citation(s) in RCA: 6] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [What about the content of this article? (0)] [Affiliation(s)] [Abstract] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/05/2022] Open
Abstract
OBJECTIVE Scapular free flap harvesting for oral cavity cancer reconstruction is an increasingly used and versatile option. We aim to describe the appearance of the scapula harvest site on chest radiograph and CT. METHODS We retrospectively reviewed a surgical database of 82 patients who underwent scapular osteocutaneous flap harvesting for oral cavity cancer reconstruction and had imaging performed at our institution. We searched the picture archiving and communications system for all associated imaging. RESULTS Characteristic radiographic appearance in the immediate post-operative period as well as in the remote post-operative period is described, including an upside-down V-shaped paraglenoid notch, rectangular (or triangular) lateral border defects and a sharply pointed inferior scapular body. Additionally, common CT appearances are discussed, including an abrupt gleno-scapular interval, an absent axillary rim bulge and a Z-shaped scapula. CONCLUSION The altered appearance of the scapular defect following surgical harvest is easily recognised. Although the description of this defect may not alter management and may reasonably be omitted, a radiologist's comfort with these appearances may potentially enhance the understanding of patient management and recognition of superimposed complications, such as infection. ADVANCES IN KNOWLEDGE Scapular osteocutaneous free flap reconstruction is an increasingly used technique after oral cavity surgery. Very few radiologists reported in our review the surgical scapular defects, and there is apparent ignorance of their appearance. We described characteristic radiographic and CT signs of scapular free flap harvesting to increase radiologists' familiarity with these defects, which may provide clinical information and possibly contribute to detection of complications.
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Affiliation(s)
- D K Powell
- Department of Radiology, Beth Israel Medical Center, New York, NY, USA.
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Espinosa GA, Wilbur AC, Warner DL, James CF, Michael A, Powell DK, Otto RJ. Carpal bone malignancies. Mil Med 1987; 152:93-5. [PMID: 3103027] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 01/04/2023] Open
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Abstract
Platelet antibodies were looked for in 47 patients with autoimmune thrombocytopenia using a modification of the enzyme-linked assay previously described. Surface-bound antibodies measured as increased platelet-associated IgG were found in 32 (68%) of the patients. After incubation in test sera, the platelet-associated IgG of normal donor platelets was significantly increased in 27 of the 47 patients (57%), thus demonstrating the presence of platelet antibodies free in their sera. 6 patients had antibodies only in the serum without any elevation of their platelet-associated IgG. When both tests are evaluated together no antibody was detected by either the direct or the indirect test in 9 of the 47 patients (29%) studied. The technique used is described and the interpretation of our results discussed.
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Abstract
An enzyme linked immunoassay incorporating antihuman globulin coupled with alkaline phosphatase has been developed to measure platelet associated IgG (PAIgG). Using a method in which platelet IgG is extracted into the fluid phase after appropriate procedures, we were able to bind the 'solubilized' PAIgG to commercially obtained antihuman IgG (AHG) which had previously been coated onto polystyrene. The amount of PAIgG thus bound was subsequently measured by the addition of the enzyme reagent using p-nitro phenyl phosphate as substrate. With this technique platelets from normal donors were found to have 2.6-17.4 ng/10(6) platelets (mean +/-2 SD). These values are higher than those obtained when assay systems using intact platelets are employed. Platelets from patients with immune thrombocytopenia had PAIgG values of 8.2-98.0 ng/10(6) platelets. In a few patients with disorders other than autoimmune thrombocytopenia (AITP) increased levels of PAIgG were also demonstrated. The assumption that increased PAIgG always represents platelet autoantibody may not be valid. The relevance of PAIgG as a parameter in the diagnosis and clinical management of patients with AITP is discussed.
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Powell DK. 'Sun never sets' for staff in prevention-oriented practice. Dent Surv 1976; 52:72-4. [PMID: 1074483] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [What about the content of this article? (0)] [MESH Headings] [Subscribe] [Scholar Register] [Indexed: 12/25/2022]
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