Zobrazeno 1 - 10
of 10 544
pro vyhledávání: '"Peel, M A"'
Autor:
Porayko, N. K., Usynina, P., Terol-Calvo, J., Camalich, J. Martin, Shaifullah, G. M., Castillo, A., Blas, D., Guillemot, L., Peel, M., Tiburzi, C., Postnov, K., Kramer, M., Antoniadis, J., Babak, S., Nielsen, A. -S. Bak, Barausse, E., Bassa, C. G., Blanchard, C., Bonetti, M., Bortolas, E., Brook, P. R., Burgay, M., Caballero, R. N., Chalumeau, A., Champion, D. J., Chanlaridis, S., Chen, S., Cognard, I., Desvignes, G., Falxa, M., Ferdman, R. D., Franchini, A., Gair, J. R., Goncharov, B., Graikou, E., Grießmeier, J. -M., Guo, Y. J., Hu, H., Iraci, F., Izquierdo-Villalba, D., Jang, J., Jawor, J., Janssen, G. H., Jessner, A., Karuppusamy, R., Keane, E. F., Keith, M. J., Krishnakumar, M. A., Lackeos, K., Lee, K. J., Liu, K., Liu, Y., Lyne, A. G., McKee, J. W., Main, R. A., Mickaliger, M. B., Niţu, I. C., Parthasarathy, A., Perera, B. B. P., Perrodin, D., Petiteau, A., Possenti, A., Leclere, H. Quelquejay, Samajdar, A., Sanidas, S. A., Sesana, A., Speri, L., Spiewak, R., Stappers, B. W., Susarla, S. C., Theureau, G., van der Wateren, E., Vecchio, A., Krishnan, V. Venkatraman, Wang, J., Wang, L., Wu, Z.
Ultra-light axion-like particles (ALPs) can be a viable solution to the dark matter problem. The scalar field associated with ALPs, coupled to the electromagnetic field, acts as an active birefringent medium, altering the polarisation properties of l
Externí odkaz:
http://arxiv.org/abs/2412.02232
Autor:
Macías-Pérez, J. F., Fernández-Torreiro, M., Catalano, A., Fasano, A., Aguiar, M., Beelen, A., Benoit, A., Bideaud, A., Bounmy, J., Bourrion, O., Calvo, M., Castro-Almazán, J. A., de Bernardis, P., de Petris, M., de Taoro, A. P., Garde, G., Génova-Santos, R. T., Gomez, A., Gómez-Renasco, M. F., Goupy, J., Hoarau, C., Hoyland, R., Lagache, G., Marpaud, J., Marton, M., Masi, S., Monfardini, A., Peel, M. W., Pisano, G., Ponthieu, N., Rebolo, R., Roni, S., Roudier, S., Rubiño-Martín, J. A., Tourres, D., Tucker, C., Viera-Curvelo, T., Vescovi, C.
Kinetic inductance detectors (KIDs) have been proven as reliable systems for astrophysical observations, especially in the millimetre range. Their compact size enables to optimally fill the focal plane, thus boosting sensitivity. The KISS (KIDs Inter
Externí odkaz:
http://arxiv.org/abs/2409.20272
Autor:
González-González, R., Génova-Santos, R. T., Rubiño-Martín, J. A., Peel, M. W., Guidi, F., López-Caraballo, C. H., Fernández-Torreiro, M., Rebolo, R., Hernández-Monteagudo, C., Adak, D., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Fasano, A., Herranz, D., Hoyland, R. J., Martínez-González, E., Pascual-Cisneros, G., Piccirillo, L., Poidevin, F., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P., Watson, R. A.
This work focuses on the study of the AME, an important emission mechanism between 10 and 60 GHz whose polarization properties are not yet fully understood, and is therefore a potential contaminant for future CMB polarization observations. We use new
Externí odkaz:
http://arxiv.org/abs/2409.03418
Autor:
Sueno, Y., Baselmans, J. J. A., Coppens, A. H. M., Génova-Santos, R. T, Hattori, M., Honda, S., Karatsu, K., Kutsuma, H., Lee, K., Nagasaki, T., Oguri, S., Otani, C., Peel, M., Suzuki, J., Tajima, O., Tanaka, T., Tsujii, M., Thoen, D. J., Won, E.
Understanding telescope pointing (i.e., line of sight) is important for observing the cosmic microwave background (CMB) and astronomical objects. The Moon is a candidate astronomical source for pointing calibration. Although the visible size of the M
Externí odkaz:
http://arxiv.org/abs/2308.15749
Autor:
Fernández-Torreiro, M., Génova-Santos, R. T., Rubiño-Martín, J. A., López-Caraballo, C. H., Peel, M. W., Arce-Tord, C., Rebolo, R., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Guidi, F., Herranz, D., Hoyland, R., Lasenby, A., Martínez-Gonzalez, E., Piccirillo, L., Poidevin, F., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P., Watson, R. A.
The Andromeda Galaxy (M31) is the Local Group galaxy that is most similar to the Milky Way (MW). The similarities between the two galaxies make M31 useful for studying integrated properties common to spiral galaxies. We use the data from the recent Q
Externí odkaz:
http://arxiv.org/abs/2305.08547
Autor:
Fernández-Torreiro, M., Rubiño-Martín, J. A., López-Caraballo, C. H., Génova-Santos, R. T., Peel, M. W., Guidi, F., Harper, S. E., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Herranz, D., Hoyland, R., Lasenby, A., Martínez-Gonzalez, E., Piccirillo, L., Poidevin, F., Rebolo, R., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P., Watson, R. A.
Anomalous Microwave Emission (AME) is an important emission component between 10 and 60 GHz that is not yet fully understood. It seems to be ubiquituous in our Galaxy and is observed at a broad range of angular scales. Here we use the new QUIJOTE-MFI
Externí odkaz:
http://arxiv.org/abs/2305.06762
Autor:
Harper, Stuart E., Barr, Adam, Dickinson, C., Peel, M. W., Cepeda-Arroita, Roke, Copley, C. J., Grumitt, R. D. P., Leahy, J. Patrick, Jonas, J. L., Jones, Michael E., Leech, J., Pearson, T. J., Readhead, A. C. S., Taylor, Angela C.
The Andromeda galaxy (M31) is our closest neighbouring spiral galaxy, making it an ideal target for studying the physics of the interstellar medium in a galaxy very similar to our own. Using new observations of M31 at 4.76GHz by the C-Band All-Sky Su
Externí odkaz:
http://arxiv.org/abs/2304.03875
Autor:
Herranz, D., López-Caniego, M., López-Caraballo, C. H., Génova-Santos, R. T., Perrott, Y. C., Rubiño-Martín, J. A., Rebolo, R., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Fernández-Torreiro, M., Guidi, F., Hoyland, R. J., Lasenby, A. N., Martínez-González, E., Peel, M. W., Piccirillo, L., Poidevin, F., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P., Watson, R. A.
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:
http://arxiv.org/abs/2301.05118
Autor:
de la Hoz, E., Barreiro, R. B., Vielva, P., Martínez-González, E., Rubiño-Martín, J. A., Casaponsa, B., Guidi, F., Ashdown, M., Génova-Santos, R. T., Artal, E., Casas, F. J., Fernández-Cobos, R., Fernández-Torreiro, M., Herranz, D., Hoyland, R. J., Lasenby, A. N., López-Caniego, M., López-Caraballo, C. H., Peel, M. W., Piccirillo, L., Poidevin, F., Rebolo, R., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Watson, R. A.
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:
http://arxiv.org/abs/2301.05117
Autor:
Poidevin, F., Génova-Santos, R. T., Rubiño-Martín, J. A., López-Caraballo, C. H., Watson, R. A., Artal, E., Ashdown, M., Barreiro, R. B., Casas, F. J., de la Hoz, E., Fernández-Torreiro, M., Guidi, F., Herranz, D., Hoyland, R. J., Lasenby, A. N., Martinez-Gonzalez, E., Peel, M. W., Piccirillo, L., Rebolo, R., Ruiz-Granados, B., Tramonte, D., Vansyngel, F., Vielva, P.
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:
http://arxiv.org/abs/2301.05116