Zobrazeno 1 - 10
of 173
pro vyhledávání: '"Bonne, Nicolas"'
Autor:
Middleton, Hannah, Berry, Christopher P L, Arnaud, Nicolas, Blair, David, Bondell, Jacqueline, Bonne, Nicolas, Chatterjee, Debarati, Chaty, Sylvain, Colloms, Storm, Cominsky, Lynn, Conti, Livia, Cordero-Carrión, Isabel, Coyne, Robert, Doctor, Zoheyr, Freise, Andreas, Geller, Aaron, Gupta, Jen, Holz, Daniel, Katzman, William, Keitel, David, Key, Joey Shapiro, Kijbunchoo, Nutsinee, Knox, Carl, Krawczyk, Coleman, Lang, Ryan N, Larson, Shane L, North, Chris, Rieger, Sascha, Simonnet, Aurore, Spencer, Andrew
The LIGO-Virgo-KAGRA (LVK) Collaboration has made breakthrough discoveries in gravitational-wave astronomy, a new field of astronomy that provides a different means of observing our Universe. Gravitational-wave discoveries are possible thanks to the
Externí odkaz:
http://arxiv.org/abs/2407.18638
Publikováno v:
In Aerospace Science and Technology November 2024 154
Autor:
Bonne, Nicolas-Xavier
Contexte : Le schwannome vestibulaire (SV) est une tumeur bénigne de la gaine du nerf vestibulaire. La plupart des SV présentent une inactivation somatique bi-allèlique du gène suppresseur de tumeur NF2. L’inactivation congénitale du gène NF2
Externí odkaz:
http://www.theses.fr/2018LIL2S017/document
Autor:
Bonne, Nicolas
Le phénomène d’interaction onde de choc/couche limite (CL) est omniprésent en aérodynamique. De manière générale, il génère des oscillations basses fréquences qui peuvent être néfastes pour les machines. L’exemple typique est le tremb
Externí odkaz:
http://www.theses.fr/2018SACLX025/document
We measure the cosmic star formation history out to z = 1.3 using a sample of 918 radio-selected star forming galaxies within the 2 square degree COSMOS field. To increase our sample size, we combine 1.4 GHz flux densities from the VLA-COSMOS catalog
Externí odkaz:
http://arxiv.org/abs/1901.11222
We have measured the relationships between HI mass, stellar mass and star formation rate using the HI Parkes All Sky-Survey Catalogue (HICAT) and the Wide-field Infrared Survey Explorer (WISE). Of the 3,513 HICAT sources, we find 3.4 micron counterpa
Externí odkaz:
http://arxiv.org/abs/1807.06246
Autor:
Fraser-McKelvie, Amelia, Brown, Michael J. I., Pimbblet, Kevin, Dolley, Tim, Bonne, Nicolas J.
We examine the properties of a sample of 35 nearby passive spiral galaxies in order to determine their dominant quenching mechanism(s). All five low mass ($\textrm{M}_{\star} < 1 \times 10^{10} \textrm{M}_{\odot}$) passive spiral galaxies are located
Externí odkaz:
http://arxiv.org/abs/1710.10843
Autor:
Brown, Michael J. I., Moustakas, John, Kennicutt, Robert C., Bonne, Nicolas J., Intema, Huib T., de Gasperin, Francesco, Boquien, Mederic, Jarrett, T. H., Cluver, Michelle E., Smith, J. -D. T., da Cunha, Elisabete, Imanishi, Masatoshi, Armus, Lee, Brandl, Bernhard R., Peek, J. E. G.
We present calibrations for star formation rate indicators in the ultraviolet, mid-infrared and radio continuum bands, including one of the first direct calibrations of 150 MHz as a star formation rate indicator. Our calibrations utilize 66 nearby st
Externí odkaz:
http://arxiv.org/abs/1709.00183
Autor:
Fraser-McKelvie, Amelia, Brown, Michael J. I., Pimbblet, Kevin A., Dolley, Tim, Crossett, Jacob P., Bonne, Nicolas J.
We have identified a population of passive spiral galaxies from photometry and integral field spectroscopy. We selected z<0.035 spiral galaxies that have WISE colours consistent with little mid-infrared emission from warm dust. Matched aperture photo
Externí odkaz:
http://arxiv.org/abs/1606.03781
We have determined K-band luminosity functions for 13,325 local Universe galaxies as a function of morphology and color (for K_tot <= 10.75). Our sample is drawn from the 2MASS Extended Source Catalog, with all sample galaxies having measured morphol
Externí odkaz:
http://arxiv.org/abs/1411.6110