Zobrazeno 1 - 10
of 199
pro vyhledávání: '"Vaccari Mattia"'
Autor:
Andersson, Alex, Lintott, Chris, Fender, Rob, Lochner, Michelle, Woudt, Patrick, Eijnden, Jakob van den, van der Horst, Alexander, Horesh, Assaf, Saikia, Payaswini, Sivakoff, Gregory R., Tremou, Lilia, Vaccari, Mattia
In this work we explore the applicability of unsupervised machine learning algorithms to the task of finding radio transients. Facilities such as the Square Kilometre Array (SKA) will provide huge volumes of data in which to detect rare transients; t
Externí odkaz:
http://arxiv.org/abs/2410.01034
Autor:
Sillassen, Nikolaj B., Jin, Shuowen, Magdis, Georgios E., Daddi, Emanuele, Wang, Tao, Lu, Shiying, Sun, Hanwen, Arumugam, Vinod, Liu, Daizhong, Brinch, Malte, D'Eugenio, Chiara, Gobat, Raphael, Gómez-Guijarro, Carlos, Rich, Michael, Schinnerer, Eva, Strazzullo, Veronica, Tan, Qinghua, Valentino, Francesco, Wang, Yijun, Xiao, Mengyuan, Zhou, Luwenjia, Blánquez-Sesé, David, Cai, Zheng, Chen, Yanmei, Ciesla, Laure, Dai, Yu, Delvecchio, Ivan, Elbaz, David, Finoguenov, Alexis, Gao, Fangyou, Gu, Qiusheng, Hale, Catherine, Hao, Qiaoyang, Huang, Jiasheng, Jarvis, Matt, Kalita, Boris, Ke, Xu, Bail, Aurelien Le, Magnelli, Benjamin, Shi, Yong, Vaccari, Mattia, Whittam, Imogen, Yang, Tiancheng, Zhang, Zhiyu
Publikováno v:
A&A 690, A55 (2024)
The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at $z>2$ in six deep fields. We report spectroscopic confirmation of eight groups at $1.65\leq z\leq3.61$ in COSMOS. Homogeneously selected as sig
Externí odkaz:
http://arxiv.org/abs/2407.02973
Autor:
Wang, Lingyu, La Marca, Antonio, Gao, Fangyou, Pearson, William J., Margalef-Bentabol, Berta, Béthermin, Matthieu, Bing, Longji, Donnellan, James, Hurley, Peter D., Oliver, Seb J., Hale, Catherine L., Jarvis, Matt J., Marchetti, Lucia, Vaccari, Mattia, Whittam, Imogen H.
Publikováno v:
A&A 688, A20 (2024)
Single-dish far-infrared (far-IR) and sub-millimetre (sub-mm) point source catalogues and their connections with catalogues at other wavelengths are of paramount importance. However, due to the large mismatch in spatial resolution, cross-matching gal
Externí odkaz:
http://arxiv.org/abs/2405.18290
Autor:
Sinigaglia, Francesco, Rodighiero, Giulia, Elson, Ed, Bianchetti, Alessandro, Vaccari, Mattia, Maddox, Natasha, Ponomareva, Anastasia A., Frank, Bradley S., Jarvis, Matt J., Catinella, Barbara, Cortese, Luca, Roychowdhury, Sambit, Baes, Maarten, Collier, Jordan D., Ilbert, Olivier, Khostovan, Ali A., Kurapati, Sushma, Pan, Hengxing, Prandoni, Isabella, Rajohnson, Sambatriniaina H. A., Salvato, Mara, Sekhar, Srikrishna, Sharma, Gauri
We present the first measurement of HI mass of star-forming galaxies in different large scale structure environments from a blind survey at $z\sim 0.37$. In particular, we carry out a spectral line stacking analysis considering $2875$ spectra of colo
Externí odkaz:
http://arxiv.org/abs/2403.00734
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:
Jarvis, Matt J., Heywood, Ian, Jewell, Sophie M., Deane, Roger P., Klöckner, H. -R., Ponomareva, Anastasia A., Maddox, Natasha, Baker, Andrew J., Bianchetti, Alessandro, Hess, Kelley M., Roberts, Hayley, Rodighiero, Giulia, Ruffa, Ilaria, Sinigaglia, Francesco, Varadaraj, R. G., Whittam, I. H., Adams, Elizabeth A. K., Baes, Maarten, Murphy, Eric J., Pan, Hengxing, Vaccari, Mattia
We present the discovery of the most distant OH megamaser to be observed in the main lines, using data from the MeerKAT International Giga-Hertz Tiered Extragalactic Exploration (MIGHTEE) survey. At a newly measured redshift of $z = 0.7092$, the syst
Externí odkaz:
http://arxiv.org/abs/2312.04345
Autor:
Borsato, Edoardo, Marchetti, Lucia, Negrello, Mattia, Corsini, Enrico Maria, Wake, David, Amvrosiadis, Aristeidis, Baker, Andrew, Bakx, Tom, Beelen, Alexandre, Berta, Stefano, Clements, David, Cooray, Asantha, Cox, Pierre, Dannerbauer, Helmut, de Zotti, Gianfranco, Dye, Simon, Eales, Stephen, Enia, Andrea, Farrah, Duncan, Gonzalez-Nuevo, Joaquin, Hughes, David, Ismail, Diana, Jin, Shuowen, Lapi, Andrea, Lehnert, Matthew, Neri, Roberto, Pérez-Fournon, Ismael, Rodighiero, Giulia, Scott, Douglas, Serjeant, Stephen, Stanley, Flora, Urquhart, Sheona, van der Werf, Paul, Vaccari, Mattia, Wang, Lingyu, Yang, Chentao, Young, Anthony
We have carried out HST snapshot observations at 1.1 $\mu$m of 281 candidate strongly lensed galaxies identified in the wide-area extragalactic surveys conducted with the Herschel space observatory. Our candidates comprise systems with flux densities
Externí odkaz:
http://arxiv.org/abs/2311.01158
Autor:
Brand, Kevin, Grobler, Trienko L., Kleynhans, Waldo, Vaccari, Mattia, Prescott, Matthew, Becker, Burger
State-of-the-art radio observatories produce large amounts of data which can be used to study the properties of radio galaxies. However, with this rapid increase in data volume, it has become unrealistic to manually process all of the incoming data,
Externí odkaz:
http://arxiv.org/abs/2304.05095
Autor:
Namumba, Brenda, Román, Javier, Barroso, Jesus Falcon, Knapen, Johan H., Roger, Ianjamasimanana, Naluminsa, Elizabeth, Jozsa, Gyula I. G., Korsaga, Marie, Maddox, Natasha, Frank, Brad, Sikhosana, Sinenhlanhla, Legodi, Samuel, Carignan, Claude, Ponomareva, Anastasia A., Jarrett, Tom, Lucero, Danielle, Smirnov, Oleg M., van der Hulst, Thijs, Pisano, D. J., Malek, kasia, Marchetti, Lucia, Vaccari, Mattia, Jarvis, Matt, Baes, Maarten, Meyer, Martin, Adams, Elizabeth A. K., Delhaize, Jacinta, Chen, Hao, Rajohnson, Sambatriniaina, Kurapati, Sushma, Heywood, Ian, Verdes-Montenegro, Lourdes
The transformation and evolution of a galaxy is strongly influenced by interactions with its environment. Neutral hydrogen (\HI) is an excellent way to trace these interactions. Here, we present \HI\ observations of the spiral galaxy NGC~895, which w
Externí odkaz:
http://arxiv.org/abs/2303.09371