Zobrazeno 1 - 10
of 237
pro vyhledávání: '"Smolčić, Vernesa"'
Autor:
Long, Arianna S., Casey, Caitlin M., McKinney, Jed, Zavala, Jorge A., Akins, Hollis B., Cooper, Olivia R., Lambrides, Matthieu Bethermin Erini L., Franco, Maximilien, Caputi, Karina, Champagne, Jaclyn B., Man, Allison W. S., Treister, Ezequiel, Manning, Sinclaire M., Sanders, David B., Talia, Margherita, Aravena, Manuel, Clements, D. L., da Cunha, Elisabete, Faisst, Andreas L., Gentile, Fabrizio, Hodge, Jacqueline, Brammer, Gabriel, Brusa, Marcella, Finkelstein, Steven L., Fujimoto, Seiji, Hayward, Christopher C., Ilbert, Olivier, Jolly, Jean-Baptiste, Kartaltepe, Jeyhan S., Knudsen, Kirsten, Koekemoer, Anton M., Liu, Daizhong, Magdis, Georgios, McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant E., Scoville, Nick, Sheth, Kartik, Smolcic, Vernesa, Spilker, Justin, Taniguchi, Yoshiaki, Toft, Sune, Urry, C. Megan, Yun, Min
One of the greatest challenges in galaxy evolution over the last decade has been constraining the prevalence of heavily dust-obscured galaxies in the early Universe. At $z>3$, these galaxies are increasingly rare, and difficult to identify as they ar
Externí odkaz:
http://arxiv.org/abs/2408.14546
Autor:
Gentile, Fabrizio, Talia, Margherita, Daddi, Emanuele, Giulietti, Marika, Lapi, Andrea, Massardi, Marcella, Pozzi, Francesca, Zamorani, Giovanni, Behiri, Meriem, Enia, Andrea, Bethermin, Matthieu, Dallacasa, Daniele, Delvecchio, Ivan, Faisst, Andreas L., Gruppioni, Carlotta, Loiacono, Federica, Traina, Alberto, Vaccari, Mattia, Vallini, Livia, Vignali, Cristian, Smolcic, Vernesa, Cimatti, Andrea
Publikováno v:
A&A 687, A288 (2024)
We present the first spectroscopic ALMA follow-up for a pilot sample of nine Radio-Selected NIRdark galaxies in the COSMOS field. These sources were initially selected as radio-detected sources (S(3GHz)>12.65 uJy), lacking an optical/NIR counterpart
Externí odkaz:
http://arxiv.org/abs/2402.05994
Autor:
Gentile, Fabrizio, Talia, Margherita, Behiri, Meriem, Zamorani, Gianni, Barchiesi, Luigi, Vignali, Cristian, Pozzi, Francesca, Bethermin, Matthieu, Enia, Andrea F., Faisst, Andreas L., Giulietti, Marika, Gruppioni, Carlotta, Lapi, Andrea, Massardi, Marcella, Smolcic, Vernesa, Vaccari, Mattia, Cimatti, Andrea
In the last decades, an increasing scientific interest has been growing in the elusive population of "dark" (i.e. lacking an optical/NIR counterpart) Dusty Star-Forming Galaxies (DSFGs). Although extremely promising for their likely contribution to t
Externí odkaz:
http://arxiv.org/abs/2312.05305
Autor:
Behiri, Meriem, Talia, Margherita, Cimatti, Andrea, Lapi, Andrea, Massardi, Marcella, Enia, Andrea F., Vignali, Cristian, Bethermin, Matthieu, Faisst, Andreas L., Gentile, Fabrizio, Giulietti, Marika, Gruppioni, Carlotta, Pozzi, Francesca, Smolcic, Vernesa, Zamorani, Gianni
About 12 billion years ago, the Universe was first experiencing light again after the dark ages, and galaxies filled the environment with stars, metals and dust. How efficient was this process? How fast did these primordial galaxies form stars and du
Externí odkaz:
http://arxiv.org/abs/2309.00050
Autor:
Ceraj, Lana, Smolčić, Vernesa, Delvecchio, Ivan, Butler, Andrew, Tisanić, Krešimir, Delhaize, Jacinta, Horellou, Cathy, Kartaltepe, Jeyhan, Kolokythas, Konstantinos, Leslie, Sarah, Marchesi, Stefano, Novak, Mladen, Pierre, Marguerite, Plionis, Manolis, Vardoulaki, Eleni, Zamorani, Giovanni
Publikováno v:
A&A 642, A125 (2020)
We studied a sample of 274 radio and X-ray selected quasars (XQSOs) detected in the COSMOS and XXL-S radio surveys at 3 GHz and 2.1 GHz, respectively. This sample was identified by adopting a conservative threshold in X-ray luminosity, Lx [2-10\ keV]
Externí odkaz:
http://arxiv.org/abs/2106.08786
Autor:
Molnar, Daniel Cs., Sargent, Mark T., Leslie, Sarah, Magnelli, Benjamin, Schinnerer, Eva, Zamorani, Giovanni, Delhaize, Jacinta, Smolcic, Vernesa, Tisanic, Kresimir, Vardoulaki, Eleni
The infrared-radio correlation (IRRC) underpins many commonly used radio luminosity-star formation rate (SFR) calibrations. In preparation for the new generation of radio surveys we revisit the IRRC of low-$z$ galaxies by (a) drawing on the best curr
Externí odkaz:
http://arxiv.org/abs/2103.04803
Autor:
Talia, Margherita, Cimatti, Andrea, Giulietti, Marika, Zamorani, Gianni, Bethermin, Matthieu, Faisst, Andreas, Fèvre, Olivier Le, Smolčić, Vernesa
How and when did galaxies form and assemble their stars and stellar mass? The answer to these questions, so crucial to astrophysics and cosmology, requires the full reconstruction of the so called cosmic star formation rate density (SFRD), i.e. the e
Externí odkaz:
http://arxiv.org/abs/2011.03051
Autor:
Leslie, Sarah, Schinnerer, Eva, Liu, Daizhong, Magnelli, Benjamin, Algera, Hiddo, Karim, Alexander, Davidzon, Iary, Gozaliasl, Ghassem, Jiménez-Andrade, Eric F., Lang, Philipp, Sargent, Mark, Novak, Mladen, Groves, Brent, Smolčić, Vernesa, Zamorani, Giovanni, Vaccari, Mattia, Battisti, Andrew, Vardoulaki, Eleni, Peng, Yingjie, Kartaltepe, Jeyhan
We provide a coherent, uniform measurement of the evolution of the logarithmic star formation rate (SFR) - stellar mass ($M_*$) relation, called the main sequence of star-forming galaxies (MS), for galaxies out to $z\sim5$. We measure the MS using me
Externí odkaz:
http://arxiv.org/abs/2006.13937
Autor:
Cassata, Paolo, Liu, Daizhong, Groves, Brent, Schinnerer, Eva, Ibar, Eduardo, Sargent, Mark, Karim, Alexander, Talia, Margherita, Fevre, Olivier Le, Tasca, Lidia, Lemaux, Brian C., Ribeiro, Bruno, Fiore, Stefano, Romano, Michael, Mancini, Chiara, Morselli, Laura, Rodighiero, Giulia, Rodriguez-Munoz, Lucia, Enia, Andrea, Smolcic, Vernesa
We present the detection of CO(5-4) with S/N> 7 - 13 and a lower CO transition with S/N > 3 (CO(4-3) for 4 galaxies, and CO(3-2) for one) with ALMA in band 3 and 4 in five main sequence star-forming galaxies with stellar masses 3-6x10^10 M/M_sun at 3
Externí odkaz:
http://arxiv.org/abs/2002.04040
Autor:
Okabe, Nobuhiro, Dicker, Simon, Eckert, Dominique, Mroczkowski, Tony, Gastaldello, Fabio, Lin, Yen-Ting, Devlin, Mark, Romero, Charles E., Birkinshaw, Mark, Sarazin, Craig, Horellou, Cathy, Kitayama, Tetsu, Umetsu, Keiichi, Sereno, Mauro, Mason, Brian S., ZuHone, John A., Honda, Ayaka, Akamatsu, Hiroki, Chiu, I-Non, Kohno, Kotaro, Lin, Kai-Yang, Medezinski, Elinor, Miyazaki, Satoshi, Mitsuishi, Ikuyuki, Nishizawa, Atsushi J., Oguri, Masamune, Ota, Naomi, Pacaud, Florian, Pierre, Marguerite, Sievers, Jonathan, Smolcic, Vernesa, Stanchfield, Sara, Tanaka, Keigo, Yamamoto, Ryoichi, Yang, Chong, Yoshida, Atsushi
We present results from simultaneous modeling of high angular resolution GBT/MUSTANG-2 90 GHz Sunyaev-Zel'dovich effect (SZE) measurements and XMM-XXL X-ray images of three rich galaxy clusters selected from the HSC-SSP Survey. The combination of hig
Externí odkaz:
http://arxiv.org/abs/1911.09236