Zobrazeno 1 - 10
of 91
pro vyhledávání: '"F Poidevin"'
Autor:
J. D. R. Pierel, A. B. Newman, S. Dhawan, M. Gu, B. A. Joshi, T. Li, S. Schuldt, L. G. Strolger, S. H. Suyu, G. B. Caminha, S. H. Cohen, J. M. Diego, J. C. J. DŚilva, S. Ertl, B. L. Frye, G. Granata, C. Grillo, A. M. Koekemoer, J. Li, A. Robotham, J. Summers, T. Treu, R. A. Windhorst, A. Zitrin, S. Agarwal, A. Agrawal, N. Arendse, S. Belli, C. Burns, R. Cañameras, S. Chakrabarti, W. Chen, T. E. Collett, D. A. Coulter, R. S. Ellis, M. Engesser, N. Foo, O. D. Fox, C. Gall, N. Garuda, S. Gezari, S. Gomez, K. Glazebrook, J. Hjorth, X. Huang, S. W. Jha, P. S. Kamieneski, P. Kelly, C. Larison, L. A. Moustakas, M. Pascale, I. Pérez-Fournon, T. Petrushevska, F. Poidevin, A. Rest, M. Shahbandeh, A. J. Shajib, M. Siebert, C. Storfer, M. Talbot, Q. Wang, T. Wevers, Y. Zenati
Publikováno v:
The Astrophysical Journal Letters, Vol 967, Iss 2, p L37 (2024)
A bright ( m _F150W,AB = 24 mag), z = 1.95 supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply imaged as a result of strong gravitational lensing by a foreground galaxy cluster, detected in
Externí odkaz:
https://doaj.org/article/2158c50abcc04d72963ef0b011df2e1a
Autor:
J. D. R. Pierel, B. L. Frye, M. Pascale, G. B. Caminha, W. Chen, S. Dhawan, D. Gilman, M. Grayling, S. Huber, P. Kelly, S. Thorp, N. Arendse, S. Birrer, M. Bronikowski, R. Cañameras, D. Coe, S. H. Cohen, C. J. Conselice, S. P. Driver, J. C. J. DŚilva, M. Engesser, N. Foo, C. Gall, N. Garuda, C. Grillo, N. A. Grogin, J. Henderson, J. Hjorth, R. A. Jansen, J. Johansson, P. S. Kamieneski, A. M. Koekemoer, C. Larison, M. A. Marshall, L. A. Moustakas, M. Nonino, R. Ortiz III, T. Petrushevska, N. Pirzkal, A. Robotham, R. E. Ryan Jr., S. Schuldt, L. G. Strolger, J. Summers, S. H. Suyu, T. Treu, C. N. A. Willmer, R. A. Windhorst, H. Yan, A. Zitrin, A. Acebron, S. Chakrabarti, D. A. Coulter, O. D. Fox, X. Huang, S. W. Jha, G. Li, P. A. Mazzali, A. K. Meena, I. Pérez-Fournon, F. Poidevin, A. Rest, A. G. Riess
Publikováno v:
The Astrophysical Journal, Vol 967, Iss 1, p 50 (2024)
Supernova (SN) SN H0pe is a gravitationally lensed, triply imaged, Type Ia SN (SN Ia) discovered in James Webb Space Telescope imaging of the PLCK G165.7+67.0 cluster of galaxies. Well-observed multiply imaged SNe provide a rare opportunity to constr
Externí odkaz:
https://doaj.org/article/5060013de8ee41a58fc63301fe908ece
Autor:
J. D. R. Pierel, N. Arendse, S. Ertl, X. Huang, L. A. Moustakas, S. Schuldt, A. J. Shajib, Y. Shu, S. Birrer, M. Bronikowski, J. Hjorth, S. H. Suyu, S. Agarwal, A. Agnello, A. S. Bolton, S. Chakrabarti, C. Cold, F. Courbin, J. M. Della Costa, S. Dhawan, M. Engesser, Ori D. Fox, C. Gall, S. Gomez, A. Goobar, S. W. Jha, C. Jimenez, J. Johansson, C. Larison, G. Li, R. Marques-Chaves, S. Mao, P. A. Mazzali, I. Perez-Fournon, T. Petrushevska, F. Poidevin, A. Rest, W. Sheu, R. Shirley, E. Silver, C. Storfer, L. G. Strolger, T. Treu, R. Wojtak, Y. Zenati
Publikováno v:
The Astrophysical Journal, Vol 948, Iss 2, p 115 (2023)
Supernovae (SNe) that have been multiply imaged by gravitational lensing are rare and powerful probes for cosmology. Each detection is an opportunity to develop the critical tools and methodologies needed as the sample of lensed SNe increases by orde
Externí odkaz:
https://doaj.org/article/63cfead8b06546c2b2dbe83eda03824a
Autor:
D Tramonte, R T Génova-Santos, J A Rubiño-Martín, P Vielva, F Poidevin, C H López-Caraballo, M W Peel, M Ashdown, E Artal, R B Barreiro, F J Casas, E de la Hoz, M Fernández-Torreiro, F Guidi, D Herranz, R J Hoyland, A N Lasenby, E Martinez-Gonzalez, L Piccirillo, R Rebolo, B Ruiz-Granados, F Vansyngel, R A Watson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 519:3432-3459
We present new intensity and polarisation maps obtained with the QUIJOTE experiment towards the Galactic regions W49, W51 and IC443, covering the frequency range from 10 to 20 GHz at $\sim$ 1 deg angular resolution, with a sensitivity in the range 35
Autor:
D Herranz, M López-Caniego, C H López-Caraballo, R T Génova-Santos, Y C Perrott, J A Rubiño-Martín, R Rebolo, E Artal, M Ashdown, R B Barreiro, F J Casas, E de la Hoz, M Fernández-Torreiro, F Guidi, R J Hoyland, A N Lasenby, E Martínez-González, M W Peel, L Piccirillo, F Poidevin, B Ruiz-Granados, D Tramonte, F Vansyngel, P Vielva, R A Watson
We present the catalogue of Q-U-I JOint TEnerife (QUIJOTE) Wide Survey radio sources extracted from the maps of the Multi-Frequency Instrument compiled between 2012 and 2018. The catalogue contains 786 sources observed in intensity and polarization,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::94039e62444f647293241f4a14a33b92
http://arxiv.org/abs/2301.05118
http://arxiv.org/abs/2301.05118
Autor:
F Guidi, R T Génova-Santos, J A Rubiño-Martín, M W Peel, M Fernández-Torreiro, C H López-Caraballo, R Vignaga, E de la Hoz, P Vielva, R A Watson, M Ashdown, C Dickinson, E Artal, R B Barreiro, F J Casas, D Herranz, R J Hoyland, A N Lasenby, E Martinez-Gonzalez, L Piccirillo, F Poidevin, R Rebolo, B Ruiz-Granados, D Tramonte, F Vansyngel
The Haze is an excess of microwave intensity emission surrounding the Galactic centre. It is spatially correlated with the $\gamma$-ray Fermi bubbles, and with the S-PASS radio polarization plumes, suggesting a possible common provenance. The models
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d2333680b52e4784bc1140c68242c6d
http://arxiv.org/abs/2301.05115
http://arxiv.org/abs/2301.05115
Autor:
J A Rubiño-Martín, F Guidi, R T Génova-Santos, S E Harper, D Herranz, R J Hoyland, A N Lasenby, F Poidevin, R Rebolo, B Ruiz-Granados, F Vansyngel, P Vielva, R A Watson, E Artal, M Ashdown, R B Barreiro, J D Bilbao-Ahedo, F J Casas, B Casaponsa, R Cepeda-Arroita, E de la Hoz, C Dickinson, R Fernández-Cobos, M Fernández-Torreiro, R González-González, C Hernández-Monteagudo, M López-Caniego, C López-Caraballo, E Martínez-González, M W Peel, A E Peláez-Santos, Y Perrott, L Piccirillo, N Razavi-Ghods, P Scott, D Titterington, D Tramonte, R Vignaga.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 2023, 519(3), 3383-3431
We present QUIJOTE intensity and polarization maps in four frequency bands centred around 11, 13, 17 and 19GHz, and covering approximately 29000 deg$^2$, including most of the Northern sky region. These maps result from 9000 h of observations taken b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c90f5fff13134949ba751cc4052e179
Autor:
E de la Hoz, R B Barreiro, P Vielva, E Martínez-González, J A Rubiño-Martín, B Casaponsa, F Guidi, M Ashdown, R T Génova-Santos, E Artal, F J Casas, R Fernández-Cobos, M Fernández-Torreiro, D Herranz, R J Hoyland, A N Lasenby, M López-Caniego, C H López-Caraballo, M W Peel, L Piccirillo, F Poidevin, R Rebolo, B Ruiz-Granados, D Tramonte, F Vansyngel, R A Watson.
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2023, (519)3, 3504-3525
We derive linearly polarized astrophysical component maps in the Northern Sky from the QUIJOTE-MFI data at 11 and 13 GHz in combination with the WMAP K and Ka bands (23 and 33 GHz) and all Planck polarized channels (30-353 GHz), using the parametric
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5a62129fe7e8b9470d91c6425b2550bd
Autor:
F Poidevin, R T Génova-Santos, J A Rubiño-Martín, C H López-Caraballo, R A Watson, E Artal, M Ashdown, R B Barreiro, F J Casas, E de la Hoz, M Fernández-Torreiro, F Guidi, D Herranz, R J Hoyland, A N Lasenby, E Martinez-Gonzalez, M W Peel, L Piccirillo, R Rebolo, B Ruiz-Granados, D Tramonte, F Vansyngel, P Vielva
The QUIJOTE-MFI Northern Hemisphere Wide-Survey has provided maps of the sky above declinations $-30^\circ$ at 11, 13, 17 and 19$\,$GHz. These data are combined with ancillary data to produce Spectral Energy Distributions in intensity in the frequenc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c76627dff6a169aecf2a03900dfde71
Autor:
A Wong, E Hatziminaoglou, A Borkar, G Popping, I Pérez-Fournon, F Poidevin, F Stoehr, H Messias
The Atacama Large Millimetre/submillimetre Array (ALMA) is the world’s most advanced radio interferometric facility, producing science data with an average rate of about 1 TB per day. After a process of calibration, imaging and quality assurance, t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2744e90ca42207205afa99def04ef9c9