Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Ashdown, Mark"'
Autor:
López-Caraballo, Carlos Hugo, Ruiz-Granados, Beatriz, Santos, Ricardo Genova, Fernández-Torreiro, Mateo, Rubiño-Martin, Jose Alberto, Peel, Mike, Poidevin, Frederick, Artal, Eduardo, Ashdown, Mark, Barreiro, Rita Belen, Casas, Francisco Javier, de la Hoz, Elena, González-González, Raul, Guidi, Federica, Herranz, Diego, Hoyland, Roger, Lasenby, Anthony N, Martinez-Gonzalez, Enrique, Piccirillo, Lucio, Rebolo, Rafael, Tramonte, Denis, Vansyngel, Flavien, Vielva, Patricio, Watson, Robert
We use the new QUIJOTE-MFI wide survey (11, 13, 17 and 19 GHz) to produce spectral energy distributions (SEDs), on an angular scale of 1 deg, of the supernova remnants (SNRs) CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9. We provide new measureme
Externí odkaz:
http://arxiv.org/abs/2307.15518
Autor:
Perrott, Yvette C., López-Caniego, Marcos, Génova-Santos, Ricardo T., Rubiño-Martín, Jose Alberto, Ashdown, Mark, Herranz, Diego, Lähteenmäki, Anne, Lasenby, Anthony N., López-Caraballo, Carlos H., Poidevin, Frédérick, Tornikoski, Merja
We observed 51 sources in the Q-U-I JOint TEnerife (QUIJOTE) cosmological fields which were brighter than 1 Jy at 30 GHz in the Planck Point Source Catalogue (version 1), with the Very Large Array at 28 -- 40 GHz, in order to characterise their high-
Externí odkaz:
http://arxiv.org/abs/2102.04520
Autor:
Challinor, Anthony, Allison, Rupert, Carron, Julien, Errard, Josquin, Feeney, Stephen, Kitching, Thomas, Lesgourgues, Julien, Lewis, Antony, Zubeldía, Íñigo, Achucarro, Ana, Ade, Peter, Ashdown, Mark, Ballardini, Mario, Banday, A. J., Banerji, Ranajoy, Bartlett, James, Bartolo, Nicola, Basak, Soumen, Baumann, Daniel, Bersanelli, Marco, Bonaldi, Anna, Bonato, Matteo, Borrill, Julian, Bouchet, François, Boulanger, François, Brinckmann, Thejs, Bucher, Martin, Burigana, Carlo, Buzzelli, Alessandro, Cai, Zhen-Yi, Calvo, Martino, Carvalho, Carla-Sofia, Castellano, Gabriella, Chluba, Jens, Clesse, Sebastien, Colantoni, Ivan, Coppolecchia, Alessandro, Crook, Martin, d'Alessandro, Giuseppe, de Bernardis, Paolo, de Gasperis, Giancarlo, De Zotti, Gianfranco, Delabrouille, Jacques, Di Valentino, Eleonora, Diego, Jose-Maria, Fernandez-Cobos, Raul, Ferraro, Simone, Finelli, Fabio, Forastieri, Francesco, Galli, Silvia, Genova-Santos, Ricardo, Gerbino, Martina, González-Nuevo, Joaquin, Grandis, Sebastian, Greenslade, Joshua, Hagstotz, Steffen, Hanany, Shaul, Handley, Will, Hernandez-Monteagudo, Carlos, Hervías-Caimapo, Carlos, Hills, Matthew, Hivon, Eric, Kiiveri, Kimmo, Kisner, Ted, Kunz, Martin, Kurki-Suonio, Hannu, Lamagna, Luca, Lasenby, Anthony, Lattanzi, Massimiliano, Liguori, Michele, Lindholm, Valtteri, López-Caniego, Marcos, Luzzi, Gemma, Maffei, Bruno, Martinez-González, Enrique, Martins, C. J. A. P., Masi, Silvia, McCarthy, Darragh, Melchiorri, Alessandro, Melin, Jean-Baptiste, Molinari, Diego, Monfardini, Alessandro, Natoli, Paolo, Negrello, Mattia, Notari, Alessio, Paiella, Alessandro, Paoletti, Daniela, Patanchon, Guillaume, Piat, Michel, Pisano, Giampaolo, Polastri, Linda, Polenta, Gianluca, Pollo, Agnieszka, Poulin, Vivian, Quartin, Miguel, Remazeilles, Mathieu, Roman, Matthieu, Rubino-Martin, Jose-Alberto, Salvati, Laura, Tartari, Andrea, Tomasi, Maurizio, Tramonte, Denis, Trappe, Neil, Trombetti, Tiziana, Tucker, Carole, Valiviita, Jussi, Van de Weijgaert, Rien, van Tent, Bartjan, Vennin, Vincent, Vielva, Patricio, Vittorio, Nicola, Young, Karl, Zannoni, Mario
Lensing of the CMB is now a well-developed probe of large-scale clustering over a broad range of redshifts. By exploiting the non-Gaussian imprints of lensing in the polarization of the CMB, the CORE mission can produce a clean map of the lensing def
Externí odkaz:
http://arxiv.org/abs/1707.02259
Autor:
Challinor, Anthony D., Mortlock, Daniel J., van Leeuwen, Floor, Lasenby, Anthony N., Hobson, Michael P., Ashdown, Mark A. J., Efstathiou, George P.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 331 (2002) 994
Despite the fact that the physics of the cosmic microwave background anisotropies is most naturally expressed in Fourier space, pixelised maps are almost always used in the analysis and simulation of microwave data. A complementary approach is invest
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112277
Autor:
van Leeuwen, Floor, Challinor, Anthony D., Mortlock, Daniel J., Ashdown, Mark A. J., Hobson, Michael P., Lasenby, Anthony N., Efstathiou, George P., Shellard, E. Paul. S., Munshi, Dipak, Stolyarov, Vladislav
Publikováno v:
Mon.Not.Roy.Astron.Soc. 331 (2002) 975
We present a harmonic model for the data analysis of an all-sky cosmic microwave background survey, such as Planck, where the survey is obtained through ring-scans of the sky. In this model, resampling and pixelisation of the data are avoided. The sp
Externí odkaz:
http://arxiv.org/abs/astro-ph/0112276
Autor:
Challinor, Anthony, Fosalba, Pablo, Mortlock, Daniel, Ashdown, Mark, Wandelt, Benjamin, Gorski, Krzysztof
Publikováno v:
Phys. Rev. D 62, 123002 (2000)
We discuss all-sky convolution of the instrument beam with the sky signal in polarimetry experiments, such as the Planck mission which will map the temperature anisotropy and polarization of the cosmic microwave background (CMB). To account properly
Externí odkaz:
http://arxiv.org/abs/astro-ph/0008228
Autor:
Galcerán, Enrique, Sánchez-Expósito, Susana, Garrido, Julián, Ashdown, Mark, Moldón, Javier, Verdes-Montenegro, Lourdes
This document contains the conclusions of the analysis done on the validity of IVOA’s Provenance Data Model ([RD.1]) with regards to the Square Kilometre Array’ Science Data Processor. A brief description of what the Provenance information entail
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4dff04d57f71124a2db1d0748b1915c3
Provenance is a vital aspect in scientific studies, due to the need for reproducibility for every experiment to verify its quality, reliability, traceability or identification and location of an error. To be able to achieve a consistent method for th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4addd7d333be9aeff30b9d403c65f36d
Autor:
Perrott, Yvette C, López-Caniego, Marcos, Génova-Santos, Ricardo T, Rubiño-Martín, Jose Alberto, Ashdown, Mark, Herranz, Diego, Lähteenmäki, Anne, Lasenby, Anthony N, López-Caraballo, Carlos H, Poidevin, Frédérick, Tornikoski, Merja
Publikováno v:
Monthly Notices of the Royal Astronomical Society; 4/30/2021, Vol. 502 Issue 4, p4779-4793, 15p
Autor:
Challinor , Anthony, Allison , Rupert, Carron , Julien, Errard , Josquin, Feeney , Stephen, Kitching , Thomas, Lesgourgues , Julien, Lewis , Antony, Zubeldía , Íñigo, Achucarro , Ana, Ade , Peter, Ashdown , Mark, Ballardini , Mario, Banday , A.J., Banerji , Ranajoy, Bartlett , James, Bartolo , Nicola, Basak , Soumen, Baumann , Daniel, Bersanelli , Marco, Bonaldi , Anna, Bonato , Matteo, Borrill , Julian, Bouchet , François, Boulanger , François, Brinckmann , Thejs, Bucher , Martin, Burigana , Carlo, Buzzelli , Alessandro, Cai , Zhen-Yi, Calvo , Martino, Carvalho , Carla-Sofia, Castellano , Gabriella, Chluba , Jens, Clesse , Sebastien, Colantoni , Ivan, Coppolecchia , Alessandro, Crook , Martin, D'Alessandro , Giuseppe, De Bernardis , Paolo, De Gasperis , Giancarlo, De Zotti , Gianfranco, Delabrouille , Jacques, Di Valentino , Eleonora, Diego , Jose-Maria, Fernandez-Cobos , Raul, Ferraro , Simone, Finelli , Fabio, Forastieri , Francesco, Galli , Silvia, Genova-Santos , Ricardo, Gerbino , Martina, González-Nuevo , Joaquin, Grandis , Sebastian, Greenslade , Joshua, Hagstotz , Steffen, Hanany , Shaul, Handley , Will, Hernandez-Monteagudo , Carlos, Hervías-Caimapo , Carlos, Hills , Matthew, Luzzi , Gemma, Maffei , Bruno, Martinez-González , Enrique, Martins , C.J.A.P., Masi , Silvia, McCarthy , Darragh, Melchiorri , Alessandro, Melin , Jean-Baptiste, Molinari , Diego, Monfardini , Alessandro, Natoli , Paolo, Negrello , Mattia, Notari , Alessio, Paiella , Alessandro, Paoletti , Daniela, Patanchon , Guillaume, Piat , Michel, Pisano , Giampaolo, Polastri , Linda, Polenta , Gianluca, Pollo , Agnieszka, Poulin , Vivian, Quartin , Miguel, Remazeilles , Mathieu, Roman , Matthieu, Rubino-Martin , Jose-Alberto, Salvati , Laura, Tartari , Andrea, Tomasi , Maurizio, Tramonte , Denis, Trappe , Neil, Trombetti , Tiziana, Tucker , Carole, Valiviita , Jussi, Van De Weijgaert , Rien, Van Tent , Bartjan, Vennin , Vincent, Vielva , Patricio, Vittorio , Nicola, Young , Karl, Zannoni , Mario
Publikováno v:
JCAP
JCAP, 2018, 04 (04), pp.018. 〈10.1088/1475-7516/2018/04/018〉
JCAP, 2018, 04 (04), pp.018. 〈10.1088/1475-7516/2018/04/018〉
International audience; Lensing of the cosmic microwave background (CMB) is now a well-developed probe of the clustering of the large-scale mass distribution over a broad range of redshifts. By exploiting the non-Gaussian imprints of lensing in the p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______3379::045effe18e78778ff0b4043e23d8e2aa
https://hal.archives-ouvertes.fr/hal-01763818
https://hal.archives-ouvertes.fr/hal-01763818