Zobrazeno 1 - 10
of 53
pro vyhledávání: '"Fauvet, L."'
Autor:
Tibbs, C. T., Israel, F. P., Laureijs, R. J., Tauber, J. A., Partridge, B., Peel, M. W., Fauvet, L.
We have performed a comprehensive investigation of the global integrated flux density of M33 from radio to ultraviolet wavelengths, finding that the data between $\sim$100 GHz and 3 THz are accurately described by a single modified blackbody curve wi
Externí odkaz:
http://arxiv.org/abs/1803.10135
Autor:
Catalano, A., Ade, P., Atik, Y., Benoit, A., Bréele, E., Bock, J. J., Camus, P., Chabot, M., Charra, M., Crill, B. P., Coron, N., Coulais, A., Désert, F. -X., Fauvet, L., Giraud-Héraud, Y., Guillaudin, O., Holmes, W., Jones, W. C., Lamarre, J. -M., Macías-Pérez, J., Martinez, M., Miniussi, A., Monfardini, A., Pajot, F., Patanchon, G., Pelissier, A., Piat, M., Puget, J. -L., Renault, C., Rosset, C., Santos, D., Sauvé, A., Spencer, L. D., Sudiwala, R.
Publikováno v:
A&A 569, A88 (2014)
The Planck High Frequency Instrument (HFI) surveyed the sky continuously from August 2009 to January 2012. Its noise and sensitivity performance were excellent, but the rate of cosmic ray impacts on the HFI detectors was unexpectedly high. Furthermor
Externí odkaz:
http://arxiv.org/abs/1403.6592
Autor:
Catalano, A., Ade, P., Atik, Y., Benoit, A., Bréele, E., Bock, J. J., Camus, P., Charra, M., Crill, B. P., Coron, N., Coulais, A., Désert, F. -X., Fauvet, L., Giraud-Héraud, Y., Guillaudin, O., Holmes, W., Jones, W. C., Lamarre, J. -M., Macías-Pérez, J., Martinez, M., Miniussi, A., Monfardini, A., Pajot, F., Patanchon, G., Pelissier, A., Piat, M., Puget, J. -L., Renault, C., Rosset, C., Santos, D., Sauvé, A., Spencer, L., Sudiwala, R.
The Planck High Frequency Instrument (HFI) has been surveying the sky continuously from the second Lagrangian point (L2) between August 2009 and January 2012. It operates with 52 high impedance bolometers cooled at 100mK in a range of frequency betwe
Externí odkaz:
http://arxiv.org/abs/1403.5639
Autor:
Jaffe, T. R., Ferrière, K. M., Banday, A. J., Strong, A. W., Orlando, E., Macías-Pérez, J. F., Fauvet, L., Combet, C., Falgarone, E.
As the next step toward an improved large scale Galactic magnetic field model, we present a simple comparison of polarised synchrotron and thermal dust emission on the Galactic plane. We find that the field configuration in our previous model that re
Externí odkaz:
http://arxiv.org/abs/1302.0143
Using the Archeops and WMAP data we perform a study of the anti-center Galactic diffuse emissions - thermal dust, synchrotron, free-free and anomalous emission - at degree scales. The high frequency data are used to infer the thermal dust electromagn
Externí odkaz:
http://arxiv.org/abs/1212.6854
Autor:
Delabrouille, J., Betoule, M., Melin, J. -B., Miville-Deschênes, M. -A., Gonzalez-Nuevo, J., Jeune, M. Le, Castex, G., de Zotti, G., Basak, S., Ashdown, M., Aumont, J., Baccigalupi, C., Banday, A., Bernard, J. -P., Bouchet, F. R., Clements, D. L., da Silva, A., Dickinson, C., Dodu, F., Dolag, K., Elsner, F., Fauvet, L., Faÿ, G., Giardino, G., Leach, S., Lesgourgues, J., Liguori, M., Macias-Perez, J. F., Massardi, M., Matarrese, S., Mazzotta, P., Montier, L., Mottet, S., Paladini, R., Partridge, B., Piffaretti, R., Prezeau, G., Prunet, S., Ricciardi, S., Roman, M., Schaefer, B., Toffolatti, L.
We present the Planck Sky Model (PSM), a parametric model for the generation of all-sky, few arcminute resolution maps of sky emission at submillimetre to centimetre wavelengths, in both intensity and polarisation. Several options are implemented to
Externí odkaz:
http://arxiv.org/abs/1207.3675
We present 3D models of the Galactic magnetic field including regular and turbulent components, and of the distribution of matter in the Galaxy including relativistic electrons and dust grains. By integrating along the line of sight, we construct map
Externí odkaz:
http://arxiv.org/abs/1204.3659
We explore in this paper the ability to constrain the Galactic magnetic field intensity and spatial distribution with the incoming data from the Planck satellite experiment. We perform realistic simulations of the Planck observations at the polarized
Externí odkaz:
http://arxiv.org/abs/1201.5742
Autor:
Fauvet, L., Macias-Perez, J. F.
The Planck satellite experiment, which was launched the 14th of may 2009, will give an accurate measurement of the anisotropies of the Cosmic Microwave Background (CMB) in temperature and polarization. This measurement is polluted by the presence of
Externí odkaz:
http://arxiv.org/abs/1007.3198
The PLANCK satellite mission has been launched the 14th of May 2009 and is dedicated to the measurement of the Cosmic Microwave Background (CMB) in temperature and polarization. The presence of diffuse galactic polarized emission contaminates the mea
Externí odkaz:
http://arxiv.org/abs/1007.3195