Zobrazeno 1 - 10
of 609
pro vyhledávání: '"De Vicente, Juan"'
Autor:
Torralba-Torregrosa, Alberto, Renard, Pablo, Spinoso, Daniele, Arnalte-Mur, Pablo, Gurung-López, Siddhartha, Fernández-Soto, Alberto, Gaztañaga, Enrique, Navarro-Gironés, David, Cai, Zheng, Carretero, Jorge, Castander, J. Francisco, Eriksen, Martin, Garcia-Bellido, Juan, Hildebrandt, Hendrik, Hoekstra, Henk, Miquel, Ramon, Sanchez, Eusebio, Tallada-Crespí, Pau, De Vicente, Juan, Fernandez, Enrique
Publikováno v:
A&A 690, A388 (2024)
We present the Lyman-$\alpha$ (Ly$\alpha$) and ultraviolet (UV) luminosity function (LF), in bins of redshift, of quasars selected in the Physics of the Accelerating Universe Survey (PAUS). A sample of 915 objects was selected at $2.7
Externí odkaz:
http://arxiv.org/abs/2407.19020
Autor:
Csizi, Benjamin, Tortorelli, Luca, Siudek, Małgorzata, Gruen, Daniel, Renard, Pablo, Tallada-Crespí, Pau, Sanchez, Eusebio, Miquel, Ramon, Padilla, Cristobal, García-Bellido, Juan, Gaztañaga, Enrique, Casas, Ricard, Serrano, Santiago, De Vicente, Juan, Fernandez, Enrique, Eriksen, Martin, Manzoni, Giorgio, Baugh, Carlton M., Carretero, Jorge, Castander, Francisco J.
Publikováno v:
A&A 689, A37 (2024)
Narrowband galaxy surveys have recently gained interest as a promising method to achieve the necessary accuracy on the photometric redshift estimate of individual galaxies for stage-IV cosmological surveys. One key advantage is the ability to provide
Externí odkaz:
http://arxiv.org/abs/2405.20385
Autor:
Demirbozan, Umut, Nadathur, Seshadri, Ferrero, Ismael, Fosalba, Pablo, Kovacs, Andras, Miquel, Ramon, Davies, Christopher T., Pandey, Shivam, Adamow, Monika, Bechtol, Keith, Drlica-Wagner, Alex, Gruendl, Robert, Hartley, Will, Pieres, Adriano, Ross, Ashley, Rykoff, Eli, Sheldon, Erin, Yanny, Brian, Abbott, Tim, Aguena, Michel, Allam, Sahar, Alves, Otavio, Bacon, David, Bertin, Emmanuel, Bocquet, Sebastian, Brooks, David, Rosell, Aurelio Carnero, Carretero, Jorge, Cawthon, Ross, da Costa, Luiz, Pereira, Maria Elidaiana da Silva, De Vicente, Juan, Desai, Shantanu, Doel, Peter, Everett, Spencer, Flaugher, Brenna, Friedel, Douglas, Frieman, Josh, Gatti, Marco, Gaztanaga, Enrique, Giannini, Giulia, Gutierrez, Gaston, Hinton, Samuel, Hollowood, Devon L., James, David, Jeffrey, Niall, Kuehn, Kyler, Lahav, Ofer, Lee, Sujeong, Marshall, Jennifer, Mena-Fernández, Juan, Mohr, Joe, Myles, Justin, Ogando, Ricardo, Malagón, Andrés Plazas, Roodman, Aaron, Sanchez, Eusebio, Sevilla, Ignacio, Smith, Mathew, Soares-Santos, Marcelle, Suchyta, Eric, Swanson, Molly, Tarle, Gregory, Weaverdyck, Noah, Weller, Jochen, Wiseman, Philip
$ $Low density cosmic voids gravitationally lens the cosmic microwave background (CMB), leaving a negative imprint on the CMB convergence $\kappa$. This effect provides insight into the distribution of matter within voids, and can also be used to stu
Externí odkaz:
http://arxiv.org/abs/2404.18278
Autor:
Riquelme, Walter, Avila, Santiago, Garcia-Bellido, Juan, Porredon, Anna, Ferrero, Ismael, Chan, Kwan Chuen, Rosenfeld, Rogerio, Camacho, Hugo, Adame, Adrian G., Rosell, Aurelio Carnero, Crocce, Martin, De Vicente, Juan, Eifler, Tim, Elvin-Poole, Jack, Fang, Xiao, Krause, Elisabeth, Monroy, Martin Rodriguez, Ross, Ashley J., Sanchez, Eusebio, Sevilla, Ignacio
Local primordial non-Gaussianity (PNG) is a promising observable of the underlying physics of inflation, characterised by $f_{\rm NL}^{\rm loc}$. We present the methodology to measure $f_{\rm NL}^{\rm loc}$ from the Dark Energy Survey (DES) data usin
Externí odkaz:
http://arxiv.org/abs/2209.07187
Autor:
Renard, Pablo, Siudek, Małgorzata, Eriksen, Martin B., Cabayol, Laura, Cai, Zheng, Carretero, Jorge, Casas, Ricard, Castander, Francisco J., Fernandez, Enrique, García-Bellido, Juan, Gaztanaga, Enrique, Hoekstra, Henk, Joachimi, Benjamin, Miquel, Ramon, Navarro-Girones, David, Padilla, Cristóbal, Sanchez, Eusebio, Serrano, Santiago, Tallada-Crespí, Pau, De Vicente, Juan, Wittje, Anna, Wright, Angus H.
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 515, Issue 1, September 2022, Pages 146-166
The D4000 spectral break index is one of the most important features in the visible spectrum, as it is a proxy for stellar ages and is also used in galaxy classification. However, its direct measurement has always been reserved to spectroscopy. Here,
Externí odkaz:
http://arxiv.org/abs/2201.04411
Autor:
Tucker, Douglas, Wiesner, Matthew, Allam, Sahar, Soares-Santos, Marcelle, de Bom, Clecio, Butner, Melissa, Garcia, Alyssa, Morgan, Robert, Olivares, Felipe, Palmese, Antonella, Santana-Silva, Luidhy, Shrivastava, Anushka, Annis, James, Garcia-Bellido, Juan, Gill, Mandeep, Herner, Kenneth, Kilpatrick, Charles, Makler, Martin, Sherman, Nora, Amara, Adam, Lin, Huan, Smith, Mathew, Swann, Elizabeth, Arcavi, Iair, Bachmann, Tristan, Bechtol, Keith, Berlfein, Federico, Briceno, Cesar, Brout, Dillon, Butler, Bobby, Cartier, Regis, Casares, Jorge, Chen, Hsin-Yu, Conselice, Christopher, Contreras, Carlos, Cook, E., Cooke, Jeff, Dage, Kristen, D'Andrea, Chris, Davis, Tamara, de Carvalho, Reinaldo, Diehl, Tom, Dietrich, Joerg, Doctor, Zoheyr, Drlica-Wagner, Alex, Drout, Maria, Farr, Ben, Finley, David, Fishbach, Maya, Foley, Ryan, Foerster-Buron, Francisco, Fosalba, Pablo, Friedel, Douglas, Frieman, Josh, Frohmaier, Christopher, Gruendl, Robert, Hartley, Will, Hiramatsu, Daichi, Holz, Daniel, Howell, Andy, Kawash, Adam, Kessler, Richard, Kuropatkin, Nikolay, Lahav, Ofer, Lundgren, Andrew, Lundquist, Michael, Malik, Umang, Mann, Andrew, Marriner, John, Marshall, Jennifer, Martinez-Vazquez, Clara, McCully, Curtis, Menanteau, Felipe, Meza, Nico, Narayan, Gautham, Neilsen, Eric, Nicolaou, Constantina, Nichol, Bob, Paz-Chinchon, Francisco, Pereira, Maria, Pineda, Jonathan, Points, Sean, Quirola-Vasquez, Jonathan, Rembold, Sandro, Rest, Armin, Rodriguez, Osmar, Romer, Kathy, Sako, Masao, Salim, Samir, Scolnic, Daniel, Smith, J. Allyn, Strader, Jay, Sullivan, Mark, Swanson, Molly, Thomas, Daniel, Valenti, Stefano, Varga, Tamas Norbert, Walker, Alistair, Weller, Jochen, Wood, Mackenna, Yanny, Brian, Zenteno, Alfredo, Aguena, Michel, Andrade-Oliveira, Felipe, Bertin, Emmanuel, Brooks, David, Burke, David, Rosell, Aurelio Carnero, Kind, Matias Carrasco, Carretero, Jorge, Costanzi, Matteo, da Costa, Luiz, De Vicente, Juan, Desai, Shantanu, Everett, Spencer, Ferrero, Ismael, Flaugher, Brenna, Gaztanaga, Enrique, Gerdes, David, Gruen, Daniel, Gschwend, Julia, Gutierrez, Gaston, Hinton, Samuel, Hollowood, Devon L., Honscheid, Klaus, James, David, Kuehn, Kyler, Lima, Marcos, Maia, Marcio, Miquel, Ramon, Ogando, Ricardo, Pieres, Adriano, Malagon, Andres Plazas, Rodriguez-Monroy, Martin, Sanchez, Eusebio, Scarpine, Vic, Schubnell, Michael, Serrano, Santiago, Sevilla-Noarbe, Ignacio, Suchyta, Eric, Tarle, Gregory, To, Chun-Hao, Zhang, Yuanyuan
Publikováno v:
ApJ, 929, 115 (2022)
On 2019 August 14 at 21:10:39 UTC, the LIGO/Virgo Collaboration (LVC) detected a possible neutron star-black hole merger (NSBH), the first ever identified. An extensive search for an optical counterpart of this event, designated GW190814, was underta
Externí odkaz:
http://arxiv.org/abs/2109.13351
Autor:
Chocarro-Wrona, Carlos, López de Andrés, Julia, Rioboó-Legaspi, Pablo, Pleguezuelos-Beltrán, Paula, Antich, Cristina, De Vicente, Juan, Gálvez-Martín, Patricia, López-Ruiz, Elena, Marchal, Juan Antonio
Publikováno v:
In Biomedicine & Pharmacotherapy August 2024 177
Autor:
de Vicente, Juan Pablo, Soto, Alvaro
Current datasets to train social behaviors are usually borrowed from surveillance applications that capture visual data from a bird's-eye perspective. This leaves aside precious relationships and visual cues that could be captured through a first-per
Externí odkaz:
http://arxiv.org/abs/2107.09170
Autor:
Tortorelli, Luca, Siudek, Malgorzata, Moser, Beatrice, Kacprzak, Tomasz, Berner, Pascale, Refregier, Alexandre, Amara, Adam, García-Bellido, Juan, Cabayol, Laura, Carretero, Jorge, Castander, Francisco J., De Vicente, Juan, Eriksen, Martin, Fernandez, Enrique, Gaztanaga, Enrique, Hildebrandt, Hendrik, Joachimi, Benjamin, Miquel, Ramon, Sevilla-Noarbe, Ignacio, Padilla, Cristóbal, Renard, Pablo, Sanchez, Eusebio, Serrano, Santiago, Tallada-Crespí, Pau, Wright, Angus H.
Narrow-band imaging surveys allow the study of the spectral characteristics of galaxies without the need of performing their spectroscopic follow-up. In this work, we forward-model the Physics of the Accelerating Universe Survey (PAUS) narrow-band da
Externí odkaz:
http://arxiv.org/abs/2106.02651