Zobrazeno 1 - 10
of 49
pro vyhledávání: '"G. S. Wright"'
Autor:
K. I. Caputi, P. Rinaldi, E. Iani, P. G. Pérez-González, G. Östlin, L. Colina, T. R. Greve, H. U. Nørgaard-Nielsen, G. S. Wright, J. Álvarez-Márquez, A. Eckart, J. Hjorth, A. Labiano, O. Le Fèvre, F. Walter, P. van der Werf, L. Boogaard, L. Costantin, A. Crespo Gómez, S. Gillman, I. Jermann, D. Langeroodi, J. Melinder, F. Peissker, M. Güdel, Th. Henning, P. O. Lagage, T. P. Ray
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 2, p 159 (2024)
We investigate the properties of strong (H β + [O iii ]) emitters before and after the end of the “Epoch of Reionization” from z = 8 to z = 5.5. We make use of ultradeep JWST / NIRCam imaging in the parallel field (P2) of the MIRI Deep Imaging S
Externí odkaz:
https://doaj.org/article/5319802472844334b1516c6b4d57f021
Autor:
P. Rinaldi, K. I. Caputi, E. Iani, L. Costantin, S. Gillman, P. G. Perez Gonzalez, G. Östlin, L. Colina, T. R. Greve, H. U. Nørgard-Nielsen, G. S. Wright, J. Álvarez-Márquez, A. Eckart, M. García-Marín, J. Hjorth, O. Ilbert, S. Kendrew, A. Labiano, O. Le Fèvre, J. Pye, T. Tikkanen, F. Walter, P. van der Werf, M. Ward, M. Annunziatella, R. Azzollini, A. Bik, L. Boogaard, S. E. I. Bosman, A. Crespo Gómez, I. Jermann, D. Langeroodi, J. Melinder, R. A. Meyer, T. Moutard, F. Peissker, E. van Dishoeck, M. Güdel, Th. Henning, P.-O. Lagage, T. Ray, B. Vandenbussche, C. Waelkens, Pratika Dayal
Publikováno v:
The Astrophysical Journal, Vol 969, Iss 1, p 12 (2024)
By using an ultradeep JWST/MIRI image at 5.6 μ m in the Hubble eXtreme Deep Field, we constrain the role of strong H α emitters (HAEs) during “cosmic reionization” at z ≃ 7–8. Our sample of HAEs is comprised of young (
Externí odkaz:
https://doaj.org/article/ed1420ab6cf5413f93017aa975eb17b4
Autor:
P. Bouchet, R. Gastaud, A. Coulais, M. J. Barlow, C. Fransson, P. J. Kavanagh, J. Larsson, T. Temim, O. C. Jones, A. S. Hirschauer, T. Tikkanen, J. A. D. L. Blommaert, O. D. Fox, A. Glasse, N. Habel, J. Hjorth, J. Jaspers, O. Krause, R. M. Lau, L. Lenkić, M. Meixner, O. Nayak, A. Rest, B. Sargent, R. Wesson, G. S. Wright, L. Colina, E. F. van Dishoeck, M. Güdel, Th. Henning, P.-O. Lagage, G. Östlin, T. P. Ray, B. Vandenbussche
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 1, p 51 (2024)
There exist very few mid-infrared (IR) observations of supernovae (SNe) in general. Therefore, SN 1987A, the closest visible SN in 400 yr, gives us the opportunity to explore the mid-IR properties of SNe, the dust in their ejecta, and the surrounding
Externí odkaz:
https://doaj.org/article/523ede7d35f64fc8a49e9fd61097e41d
Autor:
J. Larsson, C. Fransson, B. Sargent, O. C. Jones, M. J. Barlow, P. Bouchet, M. Meixner, J. A. D. L. Blommaert, A. Coulais, O. D. Fox, R. Gastaud, A. Glasse, N. Habel, A. S. Hirschauer, J. Hjorth, J. Jaspers, P. J. Kavanagh, O. Krause, R. M. Lau, L. Lenkić, O. Nayak, A. Rest, T. Temim, T. Tikkanen, R. Wesson, G. S. Wright
Publikováno v:
The Astrophysical Journal Letters, Vol 949, Iss 2, p L27 (2023)
We present initial results from JWST NIRSpec integral field unit observations of the nearby supernova SN 1987A. The observations provide the first spatially resolved spectroscopy of the ejecta and equatorial ring (ER) over the 1–5 μ m range. We co
Externí odkaz:
https://doaj.org/article/4c718bd7bd004042b3c8166ca3ee0cce
Autor:
O. C. Jones, P. J. Kavanagh, M. J. Barlow, T. Temim, C. Fransson, J. Larsson, J. A. D. L. Blommaert, M. Meixner, R. M. Lau, B. Sargent, P. Bouchet, J. Hjorth, G. S. Wright, A. Coulais, O. D. Fox, R. Gastaud, A. Glasse, N. Habel, A. S. Hirschauer, J. Jaspers, O. Krause, L. Lenkić, O. Nayak, A. Rest, T. Tikkanen, R. Wesson, L. Colina, E. F. van Dishoeck, M. Güdel, Th. Henning, P.-O. Lagage, G. Östlin, T. P. Ray, B. Vandenbussche
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 1, p 95 (2023)
Supernova (SN) 1987A is the nearest supernova in ∼400 yr. Using the JWST MIRI Medium Resolution Spectrograph, we spatially resolved the ejecta, equatorial ring (ER), and outer rings in the mid-infrared 12,927 days (35.4 yr) after the explosion. The
Externí odkaz:
https://doaj.org/article/32ad682312054cacb5d6830b91740247
Autor:
P. Rinaldi, K. I. Caputi, L. Costantin, S. Gillman, E. Iani, P. G. Pérez-González, G. Östlin, L. Colina, T. R. Greve, H. U. Noorgard-Nielsen, G. S. Wright, A. Alonso-Herrero, J. Álvarez-Márquez, A. Eckart, M. García-Marín, J. Hjorth, O. Ilbert, S. Kendrew, A. Labiano, O. Le Fèvre, J. Pye, T. Tikkanen, F. Walter, P. van der Werf, M. Ward, M. Annunziatella, R. Azzollini, A. Bik, L. Boogaard, S. E. I. Bosman, A. Crespo Gómez, I. Jermann, D. Langeroodi, J. Melinder, R. A. Meyer, T. Moutard, F. Peissker, M. Topinka, E. van Dishoeck, M. Güdel, Th. Henning, P.-O. Lagage, T. Ray, B. Vandenbussche, C. Waelkens, R. Navarro-Carrera, V. Kokorev
Publikováno v:
The Astrophysical Journal, Vol 952, Iss 2, p 143 (2023)
We make use of JWST medium-band and broadband NIRCam imaging, along with ultradeep MIRI 5.6 μ m imaging, in the Hubble eXtreme Deep Field to identify prominent line emitters at z ≃ 7–8. Out of a total of 58 galaxies at z ≃ 7–8, we find 18 ro
Externí odkaz:
https://doaj.org/article/55f3c11c599045efaa5e2bc815acbada
Autor:
A. Boccaletti, C. Cossou, P. Baudoz, P. O. Lagage, D. Dicken, A. Glasse, D. C. Hines, J. Aguilar, O. Detre, B. Nickson, A. Noriega-Crespo, A. Gáspár, A. Labiano, C. Stark, D. Rouan, J. M. Reess, G. S. Wright, G. Rieke, M. Garcia Marin, C. Lajoie, J. Girard, M. Perrin, R. Soummer, L. Pueyo
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 667, pp.A165. ⟨10.1051/0004-6361/202244578⟩
Astronomy and Astrophysics-A&A, 2022, 667, pp.A165. ⟨10.1051/0004-6361/202244578⟩
Characterization of directly imaged exoplanets is one of the most eagerly anticipated science functions of the James Webb Space Telescope. MIRI, the mid-IR instrument has the capability to provide unique spatially resolved photometric data points in
Autor:
Olivia Jones, Vincent Geers, Adrian M. Glauser, A. Coulais, A. D. O'Brien, David R. Law, Benjamin A. Sargent, Kristen Murray, C. Cossou, Steven Beard, W. De Meester, G. S. Wright, Alistair Glasse, Jeroen Bouwman, R. Gastaud, Ruyman Azzollini, J. Schreiber, Misty Cracraft, M. Topinka, Pamela Klaassen, Patrick J. Kavanagh
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (3), pp.2813-2821. ⟨10.1093/mnras/staa3416⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (3), pp.2813-2821. ⟨10.1093/mnras/staa3416⟩
The Mid-Infrared Instrument (MIRI) on the James Webb Space Telescope (JWST), has imaging, four coronagraphs and both low and medium resolution spectroscopic modes . Being able to simulate MIRI observations will help commissioning of the instrument, a
Autor:
M. Wells, Giovanna Tinetti, Subhajit Sarkar, S. Prasad, G. S. Wright, A. Vora, B. M. Shaughnessy, Jonathan Tennyson, C. Arena, T. Y. Brooke, Paul Eccleston, Chris Saunders, Mark Leese, Jon Mason, P. Knowles, J. Williams, William Taylor, P. Curry, R. V. Sudiwala, Andreas Papageorgiou, Keith Barnes, A. Saad, Marcell Tessenyi, Naidu Bezawada, Les Hipwood, Berend Winter, Tiziano Zingales, Ian Bryson, Ian Tosh, Jonathan Friend, G. Johnston, Manish R. Patel, Matthew Joseph Griffin, Peter A. R. Ade, A. Macleod, S. Jason, Martin Crook, Giorgio Savini, En. Pascale, A. M. Smith
Publikováno v:
Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave
Twinkle is a space mission designed for visible and near-IR spectroscopic observations of extrasolar planets. Twinkle’s highly stable instrument will allow the photometric and spectroscopic observation of a wide range of planetary classes around di
Autor:
George H. Rieke, Bart Vandenbussche, Alistair Glasse, E. Bauwens, Michael E. Ressler, Tuomo Tikkanen, Macarena Garcia-Marin, Steffen Rost, G. S. Wright
Publikováno v:
Publications of the Astronomical Society of the Pacific. 127:686-695
We present an estimate of the performance that will be achieved during on orbit operations of the JWST Mid Infrared Instrument, MIRI. The efficiency of the main imager and spectrometer systems in detecting photons from an astronomical target are pres