Zobrazeno 1 - 10
of 12
pro vyhledávání: '"Siudek, Malgorzata"'
Autor:
Hahn, ChangHoon, Aguilar, Jessica Nicole, Alam, Shadab, Ahlen, Steven, Brooks, David, Cole, Shaun, de la Macorra, Axel, Doel, Peter, Font-Ribera, Andreu A., Forero-Romero, Jaime E., Gontcho, Satya Gontcho A, Honscheid, Klaus, Huang, Song, Kisner, Theodore, Kremin, Anthony, Landriau, Martin, Manera, Marc, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Nie, Jundan, Poppett, Claire, Rossi, Graziano, Saintonge, Amélie, Sanchez, Eusebio, Saulder, Christoph, Schubnell, Michael, Seo, Hee-Jong, Siudek, Małgorzata, Speranza, Federico, Tarlé, Gregory, Weaver, Benjamin A., Wechsler, Risa H., Yuan, Sihan, Zhou, Zhimin, Zou, Hu
We present the probabilistic stellar mass function (pSMF) of galaxies in the DESI Bright Galaxy Survey (BGS), observed during the One-Percent Survey. The One-Percent Survey was one of DESI's survey validation programs conducted from April to May 2021
Externí odkaz:
http://arxiv.org/abs/2306.06318
Autor:
Hahn, ChangHoon, Kwon, K. J., Tojeiro, Rita, Siudek, Malgorzata, Canning, Rebecca E. A., Mezcua, Mar, Tinker, Jeremy L., Brooks, David, Doel, Peter, Fanning, Kevin, Gaztañaga, Enrique, Kehoe, Robert, Landriau, Martin, Meisner, Aaron, Moustakas, John, Poppett, Claire, Tarle, Gregory, Weiner, Benjamin, Zou, Hu
The PRObabilistic Value-Added Bright Galaxy Survey (PROVABGS) catalog will provide measurements of galaxy properties, such as stellar mass ($M_*$), star formation rate (${\rm SFR}$), stellar metallicity ($Z_{\rm MW}$), and stellar age ($t_{\rm age, M
Externí odkaz:
http://arxiv.org/abs/2202.01809
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:
Hashemizadeh, Abdolhosein, Driver, Simon P., Davies, Luke J. M., Robotham, Aaron S. G., Bellstedt, Sabine, Windhorst, Rogier A., Bremer, Malcolm, Phillipps, Steven, Jarvis, Matt, Holwerda, Benne W., Lagos, Claudia del P., Koushan, Soheil, Siudek, Malgorzata, Maddox, Natasha, Thorne, Jessica E., Elahi, Pascal
Using high-resolution Hubble Space Telescope imaging data, we perform a visual morphological classification of $\sim 36,000$ galaxies at $z < 1$ in the DEVILS/COSMOS region. As the main goal of this study, we derive the stellar mass function (SMF) an
Externí odkaz:
http://arxiv.org/abs/2102.13377
Autor:
Koushan, Soheil, Driver, Simon P., Bellstedt, Sabine, Davies, Luke J., Robotham, Aaron S. G., Lagos, Claudia del P, Hashemizadeh, Abdolhosein, Obreschkow, Danail, Thorne, Jessica E., Bremer, Malcolm, Holwerda, B. W., Hopkins, Andrew M., Jarvis, Matt J., Siudek, Malgorzata, Windhorst, Rogier A.
We present a revised measurement of the optical extragalactic background light (EBL), based on the contribution of resolved galaxies to the integrated galaxy light (IGL). The cosmic optical background radiation (COB), encodes the light generated by s
Externí odkaz:
http://arxiv.org/abs/2102.12323
Autor:
Soo, John Y. H., Joachimi, Benjamin, Eriksen, Martin, Siudek, Małgorzata, Alarcon, Alex, Cabayol, Laura, Carretero, Jorge, Casas, Ricard, Castander, Francisco J., Fernández, Enrique, Garciá-Bellido, Juan, Gaztanaga, Enrique, Hildebrandt, Hendrik, Hoekstra, Henk, Miquel, Ramon, Padilla, Cristobal, Sánchez, Eusebio, Serrano, Santiago, Tallada-Crespí, Pau
We study the performance of the hybrid template-machine-learning photometric redshift (photo-$z$) algorithm Delight, which uses Gaussian processes, on a subset of the early data release of the Physics of the Accelerating Universe Survey (PAUS). We ca
Externí odkaz:
http://arxiv.org/abs/2101.03723
Autor:
Johnston, Harry, Joachimi, Benjamin, Norberg, Peder, Hoekstra, Henk, Eriksen, Martin, Fortuna, Maria Cristina, Manzoni, Giorgio, Serrano, Santiago, Siudek, Malgorzata, Tortorelli, Luca, Cabayol, Laura, Carretero, Jorge, Casas, Ricard, Castander, Francisco, Fernandez, Enrique, García-Bellido, Juan, Gaztanaga, Enrique, Hildebrandt, Hendrik, Miquel, Ramon, Padilla, Cristobal, Sanchez, Eusebio, Sevilla-Noarbe, Ignacio, Tallada-Crespí, Pau
Publikováno v:
A&A 646, A147 (2021)
We present the first measurements of the projected clustering and intrinsic alignments (IA) of galaxies observed by the Physics of the Accelerating Universe Survey (PAUS). With photometry in 40 narrow optical passbands ($450\rm{nm}-850\rm{nm}$), the
Externí odkaz:
http://arxiv.org/abs/2010.09696
Autor:
Alarcon, Alex, Gaztanaga, Enrique, Eriksen, Martin, Baugh, Carlton M., Cabayol, Laura, Casas, Ricard, Carretero, Jorge, Castander, Francisco J., De Vicente, Juan, Fernandez, Enrique, Garcia-Bellido, Juan, Hildebrandt, Hendrik, Hoekstra, Henk, Joachimi, Benjamin, Manzoni, Giorgio, Miquel, Ramon, Norberg, Peder, Padilla, Cristobal, Renard, Pablo, Sanchez, Eusebio, Serrano, Santiago, Sevilla-Noarbe, Ignacio, Siudek, Malgorzata, Tallada-Crespí, Pau
We present -- and make publicly available -- accurate and precise photometric redshifts in the ACS footprint from the COSMOS field for objects with $i_{\mathrm{AB}}\leq 23$. The redshifts are computed using a combination of narrow band photometry fro
Externí odkaz:
http://arxiv.org/abs/2007.11132
Autor:
Rodriguez, Facundo, Gonzalez, Elizabeth J., O'Mill, Ana L., Gaztañaga, Enrique, Fosalba, Pablo, Lambas, Diego García, Mezcua, Mar, Siudek, Małgorzata
Publikováno v:
A&A 634, A123 (2020)
Context. Studies of galaxy pairs can provide valuable information to jointly understand the formation and evolution of galaxies and galaxy groups. Consequently, taking into account the new high precision photo-z surveys, it is important to have relia
Externí odkaz:
http://arxiv.org/abs/2001.07217
Autor:
The MSE Science Team, Babusiaux, Carine, Bergemann, Maria, Burgasser, Adam, Ellison, Sara, Haggard, Daryl, Huber, Daniel, Kaplinghat, Manoj, Li, Ting, Marshall, Jennifer, Martell, Sarah, McConnachie, Alan, Percival, Will, Robotham, Aaron, Shen, Yue, Thirupathi, Sivarani, Tran, Kim-Vy, Yeche, Christophe, Yong, David, Adibekyan, Vardan, Aguirre, Victor Silva, Angelou, George, Asplund, Martin, Balogh, Michael, Banerjee, Projjwal, Bannister, Michele, Barría, Daniela, Battaglia, Giuseppina, Bayo, Amelia, Bechtol, Keith, Beck, Paul G., Beers, Timothy C., Bellinger, Earl P., Berg, Trystyn, Bestenlehner, Joachim M., Bilicki, Maciej, Bitsch, Bertram, Bland-Hawthorn, Joss, Bolton, Adam S., Boselli, Alessandro, Bovy, Jo, Bragaglia, Angela, Buzasi, Derek, Caffau, Elisabetta, Cami, Jan, Carleton, Timothy, Casagrande, Luca, Cassisi, Santi, Catelan, Márcio, Chang, Chihway, Cortese, Luca, Damjanov, Ivana, Davies, Luke J. M., de Grijs, Richard, de Rosa, Gisella, Deason, Alis, di Matteo, Paola, Drlica-Wagner, Alex, Erkal, Denis, Escorza, Ana, Ferrarese, Laura, Fleming, Scott W., Font-Ribera, Andreu, Freeman, Ken, Gänsicke, Boris T., Gabdeev, Maksim, Gallagher, Sarah, Gandolfi, Davide, García, Rafael A., Gaulme, Patrick, Geha, Marla, Gennaro, Mario, Gieles, Mark, Gilbert, Karoline, Gordon, Yjan, Goswami, Aruna, Greco, Johnny P., Grillmair, Carl, Guiglion, Guillaume, Hénault-Brunet, Vincent, Hall, Patrick, Handler, Gerald, Hansen, Terese, Hathi, Nimish, Hatzidimitriou, Despina, Haywood, Misha, Santisteban, Juan V. Hernández, Hillenbrand, Lynne, Hopkins, Andrew M., Howlett, Cullan, Hudson, Michael J., Ibata, Rodrigo, Ilić, Dragana, Jablonka, Pascale, Ji, Alexander, Jiang, Linhua, Juneau, Stephanie, Karakas, Amanda, Karinkuzhi, Drisya, Kim, Stacy Y., Kong, Xu, Konstantopoulos, Iraklis, Krogager, Jens-Kristian, Lagos, Claudia, Lallement, Rosine, Laporte, Chervin, Lebreton, Yveline, Lee, Khee-Gan, Lewis, Geraint F., Lianou, Sophia, Liu, Xin, Lodieu, Nicolas, Loveday, Jon, Mészáros, Szabolcs, Makler, Martin, Mao, Yao-Yuan, Marchesini, Danilo, Martin, Nicolas, Mateo, Mario, Melis, Carl, Merle, Thibault, Miglio, Andrea, Mohammad, Faizan Gohar, Molaverdikhani, Karan, Monier, Richard, Morel, Thierry, Mosser, Benoit, Nataf, David, Necib, Lina, Neilson, Hilding R., Newman, Jeffrey A., Nierenberg, A. M., Nord, Brian, Noterdaeme, Pasquier, O'Dea, Chris, Oshagh, Mahmoudreza, Pace, Andrew B., Palanque-Delabrouille, Nathalie, Pandey, Gajendra, Parker, Laura C., Pawlowski, Marcel S., Peter, Annika H. G., Petitjean, Patrick, Petric, Andreea, Placco, Vinicius, Popović, Luka Č., Price-Whelan, Adrian M., Prsa, Andrej, Ravindranath, Swara, Rich, R. Michael, Ruan, John, Rybizki, Jan, Sakari, Charli, Sanderson, Robyn E., Schiavon, Ricardo, Schimd, Carlo, Serenelli, Aldo, Siebert, Arnaud, Siudek, Malgorzata, Smiljanic, Rodolfo, Smith, Daniel, Sobeck, Jennifer, Starkenburg, Else, Stello, Dennis, Szabó, Gyula M., Szabo, Robert, Taylor, Matthew A., Thanjavur, Karun, Thomas, Guillaume, Tollerud, Erik, Toonen, Silvia, Tremblay, Pier-Emmanuel, Tresse, Laurence, Tsantaki, Maria, Valentini, Marica, Van Eck, Sophie, Variu, Andrei, Venn, Kim, Villaver, Eva, Walker, Matthew G., Wang, Yiping, Wang, Yuting, Wilson, Michael J., Wright, Nicolas, Xu, Siyi, Yildiz, Mutlu, Zhang, Huawei, Zwintz, Konstanze, Anguiano, Borja, Bedell, Megan, Chaplin, William, Collet, Remo, Cuillandre, Jean-Charles, Duc, Pierre-Alain, Flagey, Nicolas, Hermes, JJ, Hill, Alexis, Kamath, Devika, Laychak, Mary Beth, Małek, Katarzyna, Marley, Mark, Sheinis, Andy, Simons, Doug, Sousa, Sérgio G., Szeto, Kei, Ting, Yuan-Sen, Vegetti, Simona, Wells, Lisa, Babas, Ferdinand, Bauman, Steve, Bosselli, Alessandro, Côté, Pat, Colless, Matthew, Comparat, Johan, Courtois, Helene, Crampton, David, Croom, Scott, Davies, Luke, Denny, Kelly, Devost, Daniel, Driver, Simon, Fernandez-Lorenzo, Mirian, Guhathakurta, Raja, Han, Zhanwen, Higgs, Clare, Hill, Vanessa, Ho, Kevin, Hopkins, Andrew, Hudson, Mike, Isani, Sidik, Jarvis, Matt, Johnson, Andrew, Jullo, Eric, Kaiser, Nick, Kneib, Jean-Paul, Koda, Jun, Koshy, George, Mignot, Shan, Murowinski, Rick, Newman, Jeff, Nusser, Adi, Pancoast, Anna, Peng, Eric, Peroux, Celine, Pichon, Christophe, Poggianti, Bianca, Richard, Johan, Salmon, Derrick, Seibert, Arnaud, Shastri, Prajval, Smith, Dan, Sutaria, Firoza, Tao, Charling, Taylor, Edwar, Tully, Brent, van Waerbeke, Ludovic, Vermeulen, Tom, Walker, Matthew, Willis, Jon, Willot, Chris, Withington, Kanoa
(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unveil the composition and dynamics of the faint Universe and impact nearly
Externí odkaz:
http://arxiv.org/abs/1904.04907