Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Adrien Picquenot"'
Publikováno v:
The Astrophysical Journal, Vol 963, Iss 2, p 147 (2024)
Recent X-ray studies of starburst galaxies have found that charge exchange (CX) commonly occurs between outflowing hot plasma and cold gas, possibly from swept-up clouds. However, the total CX flux and the regions where CX occurs have been poorly und
Externí odkaz:
https://doaj.org/article/61477e43574045e09e7efe4269a84d34
Autor:
Benson T. Guest, Kazimierz J. Borkowski, Parviz Ghavamian, Robert Petre, Adrien Picquenot, Stephen P. Reynolds, Ivo R. Seitenzahl, Brian J. Williams
Publikováno v:
The Astrophysical Journal, Vol 946, Iss 1, p 44 (2023)
The nature of Type Ia supernovae remains controversial. The youngest remnants of Ia supernovae hold clues to the explosion and to the immediate surroundings. We present a third epoch of Chandra observations of the ∼600 yr old Type Ia remnant 0519
Externí odkaz:
https://doaj.org/article/cbdb2bd3a230453ea2e6c161eecdbaad
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 646, pp.A82. ⟨10.1051/0004-6361/202039170⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 646, pp.A82. ⟨10.1051/0004-6361/202039170⟩
Astronomy and Astrophysics-A&A, 2021, 646, pp.A82. ⟨10.1051/0004-6361/202039170⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 646, pp.A82. ⟨10.1051/0004-6361/202039170⟩
Recent simulations have shown that asymmetries in the ejecta distribution of supernova remnants (SNR) can still reflect asymmetries from the initial supernova explosion. Thus, their study provides a great means to test and constrain model predictions
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ac7918c1f2cbd42ba2fc57f7026f5ed
https://hal.archives-ouvertes.fr/hal-02960278/document
https://hal.archives-ouvertes.fr/hal-02960278/document
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, pp.A139. ⟨10.1051/0004-6361/201834933⟩
Astronomy and Astrophysics-A&A, 2019, 627, pp.A139. ⟨10.1051/0004-6361/201834933⟩
Astronomy & Astrophysics
Astronomy and Astrophysics-A&A, EDP Sciences, 2019, 627, pp.A139. ⟨10.1051/0004-6361/201834933⟩
Astronomy and Astrophysics-A&A, 2019, 627, pp.A139. ⟨10.1051/0004-6361/201834933⟩
Astronomy & Astrophysics
In high-energy astronomy, spectro-imaging instruments such as X-ray detectors allow investigation of the spatial and spectral properties of extended sources including galaxy clusters, galaxies, diffuse interstellar medium, supernova remnants, and pul
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c389fce5dca67150c89f778ec7427b38
https://hal.archives-ouvertes.fr/hal-02160434
https://hal.archives-ouvertes.fr/hal-02160434
Publikováno v:
CAMSAP 2019
CAMSAP 2019, Dec 2019, Guadeloupe, France
2019 IEEE 8th International Workshop on Computational Advances in Multi-Sensor Adaptive Processing (CAMSAP)
CAMSAP
CAMSAP 2019, Dec 2019, Guadeloupe, France
2019 IEEE 8th International Workshop on Computational Advances in Multi-Sensor Adaptive Processing (CAMSAP)
CAMSAP
In this article, we investigate how the prior knowledge based on examples of physical spectra can be exploited in sparse Blind Source Separation (sBSS), based on the projection onto the barycentric span of these examples. For that purpose, we investi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::110629fc481b2f8143ebadcc17112cd0
https://hal.science/hal-02426994
https://hal.science/hal-02426994
Publikováno v:
IEEE Transactions on Image Processing
Blind source separation (BSS) aims at recovering signals from linear mixtures. This problem has been extensively studied when the noise is additive and Gaussian. This is however not the case when the measurements follow Poisson or shot noise statisti