Zobrazeno 1 - 10
of 510
pro vyhledávání: '"Climent, Jose"'
Autor:
Rezaie, Mehdi, Ross, Ashley J., Seo, Hee-Jong, Kong, Hui, Porredon, Anna, Samushia, Lado, Chaussidon, Edmond, Krolewski, Alex, de Mattia, Arnaud, Beutler, Florian, Aguilar, Jessica Nicole, Ahlen, Steven, Alam, Shadab, Avila, Santiago, Bahr-Kalus, Benedict, Bermejo-Climent, Jose, Brooks, David, Claybaugh, Todd, Cole, Shaun, Dawson, Kyle, de la Macorra, Axel, Doel, Peter, Font-Ribera, Andreu, Forero-Romero, Jaime E., Gontcho, Satya Gontcho A, Guy, Julien, Honscheid, Klaus, Huterer, Dragan, Kisner, Theodore, Landriau, Martin, Levi, Michael, Manera, Marc, Meisner, Aaron, Miquel, Ramon, Mueller, Eva-Maria, Myers, Adam, Newman, Jeffrey A., Nie, Jundan, Palanque-Delabrouille, Nathalie, Percival, Will, Poppett, Claire, Rossi, Graziano, Sanchez, Eusebio, Schubnell, Michael, Tarlé, Gregory, Weaver, Benjamin Alan, Yèche, Christophe, Zhou, Zhimin, Zou, Hu
We use angular clustering of luminous red galaxies from the Dark Energy Spectroscopic Instrument (DESI) imaging surveys to constrain the local primordial non-Gaussianity parameter $\fnl$. Our sample comprises over 12 million targets, covering 14,000
Externí odkaz:
http://arxiv.org/abs/2307.01753
Autor:
Bermejo-Climent, José R., Ballardini, Mario, Finelli, Fabio, Paoletti, Daniela, Maartens, Roy, Rubiño-Martin, José A., Valenziano, Luca
Publikováno v:
Phys. Rev. D 103, 103502 (2021)
The cross-correlation between the cosmic microwave background (CMB) fields and matter tracers carries important cosmological information. In this paper, we forecast by a signal-to-noise ratio analysis the information contained in the cross-correlatio
Externí odkaz:
http://arxiv.org/abs/2106.05267
Publikováno v:
Phys. Rev. D 102, 023502 (2020)
The ratio between the CMB lensing/galaxy counts and the galaxy shear/galaxy counts cross-correlations combines the information from different cosmological probes to infer cosmographic measurements that are less dependent on astrophysical uncertaintie
Externí odkaz:
http://arxiv.org/abs/1911.11766
Autor:
Delabrouille, Jacques, Abitbol, Maximilian H., Aghanim, Nabila, Ali-Haimoud, Yacine, Alonso, David, Alvarez, Marcelo, Banday, Anthony J., Bartlett, James G., Baselmans, Jochem, Basu, Kaustuv, Battaglia, Nicholas, Climent, Jose Ramon Bermejo, Bernal, Jose L., Béthermin, Matthieu, Bolliet, Boris, Bonato, Matteo, Bouchet, François R., Breysse, Patrick C., Burigana, Carlo, Cai, Zhen-Yi, Chluba, Jens, Churazov, Eugene, Dannerbauer, Helmut, De Bernardis, Paolo, De Zotti, Gianfranco, Di Valentino, Eleonora, Dimastrogiovanni, Emanuela, Endo, Akira, Erler, Jens, Ferraro, Simone, Finelli, Fabio, Fixsen, Dale, Hanany, Shaul, Hart, Luke, Hernandez-Monteagudo, Carlos, Hill, J. Colin, Hotinli, Selim C., Karatsu, Kenichi, Karkare, Kirit, Keating, Garrett K., Khabibullin, Ildar, Kogut, Alan, Kohri, Kazunori, Kovetz, Ely D., Lagache, Guilaine, Lesgourgues, Julien, Madhavacheril, Mathew, Maffei, Bruno, Mandolesi, Nazzareno, Martins, Carlos, Masi, Silvia, Mather, John, Melin, Jean-Baptiste, Dizgah, Azadeh Moradinezhad, Mroczkowski, Tony, Mukherjee, Suvodip, Nagai, Daisuke, Negrello, Mattia, Palanque-Delabrouille, Nathalie, Paoletti, Daniela, Patil, Subodh P., Piacentini, Francesco, Raghunathan, Srinivasan, Ravenni, Andrea, Remazeilles, Mathieu, Revéret, Vincent, Rodriguez, Louis, Rotti, Aditya, Martin, Jose-Alberto Rubino, Sayers, Jack, Scott, Douglas, Silk, Joseph, Silva, Marta, Souradeep, Tarun, Sugiyama, Naonori, Sunyaev, Rashid, Switzer, Eric R., Tartari, Andrea, Trombetti, Tiziana, Zubeldia, Inigo
This paper discusses the science case for a sensitive spectro-polarimetric survey of the microwave sky. Such a survey would provide a tomographic and dynamic census of the three-dimensional distribution of hot gas, velocity flows, early metals, dust,
Externí odkaz:
http://arxiv.org/abs/1909.01591
Autor:
Alía, Ricardo1 (AUTHOR) alia@inia.csic.es, Climent, Jose1 (AUTHOR), Santos-del-Blanco, Luis1 (AUTHOR), Gonzalez-Arrojo, Amelia2 (AUTHOR), Feito, Isabel3 (AUTHOR), Grivet, Delphine1 (AUTHOR), Majada, Juan2 (AUTHOR)
Publikováno v:
BMC Plant Biology. 1/9/2024, Vol. 24 Issue 1, p1-11. 11p.
Autor:
Sacco, Antonio, Desantis, Vanessa, Celay, Jon, Giustini, Viviana, Rigali, Fabio, Savino, Francesco D., Cea, Michele, Soncini, Debora, Cagnetta, Antonia, Solimando, Antonio G., D’Aliberti, Deborah, Spinelli, Silvia, Ramazzotti, Daniele, Almici, Camillo, Todoerti, Katia, Neri, Antonino, Anastasia, Antonella, Tucci, Alessandra, Motta, Marina, Chiarini, Marco, Kawano, Yawara, Martinez-Climent, Jose A., Piazza, Rocco, Roccaro, Aldo M.
Publikováno v:
In Blood 25 May 2023 141(21):2615-2628
Autor:
Peris, Irene, Romero-Murillo, Silvia, Martínez-Balsalobre, Elena, Farrington, Caroline C., Arriazu, Elena, Marcotegui, Nerea, Jiménez-Muñoz, Marta, Alburquerque-Prieto, Cristina, Torres-López, Andrea, Fresquet, Vicente, Martínez-Climent, Jose A., Mateos, Maria C., Cayuela, Maria L., Narla, Goutham, Odero, Maria D. ∗∗, ∗, Vicente, Carmen ∗, ∗
Publikováno v:
In Blood 2 March 2023 141(9):1047-1059
Autor:
Félix-Soriano, Elisa, Sáinz, Neira, Fernández-Galilea, Marta, Gil-Iturbe, Eva, Celay, Jon, Martínez-Climent, José A., Moreno-Aliaga, María J.
Publikováno v:
In The Journal of Nutritional Biochemistry January 2023 111
Akademický článek
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Autor:
Bermejo-Climent, Jose R., Battaglia, Giuseppina, Gallart, Carme, Di Cintio, Arianna, Brook, Chris B., Cicuendez, Luis, Monelli, Matteo, Leaman, Ryan, Mayer, Lucio, Penarrubia, Jorge, Read, Justin I.
According to star formation histories (SFHs), Local Group dwarf galaxies can be broadly classified in two types: those forming most of their stars before $z=2$ (${\it fast}$) and those with more extended SFHs (${\it slow}$). The most precise SFHs are
Externí odkaz:
http://arxiv.org/abs/1806.07679