Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Cassara, Letizia P."'
Autor:
Hung, Denise, Lemaux, Brian C., Cucciati, Olga, Forrest, Ben, Shah, Ekta A., Gal, Roy R., Giddings, Finn, Sikorski, Derek, Golden-Marx, Emmet, Lubin, Lori M., Hathi, Nimish, Zamorani, Giovanni, Bardelli, Sandro, Cassara, Letizia P., De Lucia, Gabriella, Fontanot, Fabio, Garilli, Bianca, Guaita, Lucia, Hirschmann, Michaela Monika, Lee, Kyoung-Soo, Newman, Andrew B., Ramakrishnan, Vandana, Vergani, Daniela, Xie, Lizhi, Zucca, Elena
The Charting Cluster Construction with VUDS and ORELSE (C3VO) survey is an ongoing imaging and spectroscopic campaign aiming to map out the growth of structure up to $z\sim5$ and was born from the combination of the VIMOS Ultra Deep Survey (VUDS) and
Externí odkaz:
http://arxiv.org/abs/2410.00237
Autor:
Shah, Ekta A., Lemaux, Brian C., Forrest, Benjamin, Hathi, Nimish, Shen, Lu, Cucciati, Olga, Hung, Denise, Giddings, Finn, Sikorski, Derek, Lubin, Lori, Gal, Roy R., Zamorani, Giovanni, Golden-Marx, Emmet, Bardelli, Sandro, Cassara, Letizia Pasqua, Garilli, Bianca, Gururajan, Gayathri, Suh, Hyewon, Vergani, Daniela, Zucca, Elena
We conduct a study on the relationship between galaxy environments and their active galactic nuclei (AGN) activity at high redshifts ($2.0
Externí odkaz:
http://arxiv.org/abs/2409.02996
Autor:
Forrest, Ben, Lemaux, Brian C., Shah, Ekta A., Staab, Priti, Gal, Roy R., Lubin, Lori M., Cooper, M. C., Cucciati, Olga, Hung, Denise, McConachie, Ian, Muzzin, Adam, Wilson, Gillian, Bardelli, Sandro, Cassarà, Letizia P., Chang, Wenjun, Giddings, Finn, Golden-Marx, Emmet, Hathi, Nimish, Stawinski, Stephanie M. Urbano, Zucca, Elena
We present an analysis of the number density of galaxies as a function of stellar mass (i.e., the stellar mass function, SMF) in the COSMOS field at z~3.3, making a comparison between the SMF in overdense environments and the SMF in the coeval field.
Externí odkaz:
http://arxiv.org/abs/2405.18491
Autor:
Staab, Priti, Lemaux, Brian C., Forrest, Ben, Shah, Ekta, Cucciati, Olga, Lubin, Lori, Gal, Roy R., Hung, Denise, Shen, Lu, Giddings, Finn, Khusanova, Yana, Zamorani, Giovanni, Bardelli, Sandro, Cassara, Letizia Pasqua, Cassata, Paolo, Chiang, Yi-Kuan, Fudamoto, Yoshinobu, Fukushima, Shuma, Garilli, Bianca, Giavalisco, Mauro, Gruppioni, Carlotta, Guaita, Lucia, Gururajan, Gayathri, Hathi, Nimish, Kashino, Daichi, Scoville, Nick, Talia, Margherita, Vergani, Daniela, Zucca, Elena
Simulations predict that the galaxy populations inhabiting protoclusters may contribute considerably to the total amount of stellar mass growth of galaxies in the early universe. In this study, we test these predictions observationally, focusing on t
Externí odkaz:
http://arxiv.org/abs/2312.11465
Autor:
Shah, Ekta A., Lemaux, Brian, Forrest, Benjamin, Cucciati, Olga, Hung, Denise, Staab, Priti, Hathi, Nimish, Lubin, Lori, Gal, Roy R., Shen, Lu, Zamorani, Giovanni, Giddings, Finn, Bardelli, Sandro, Cassara, Letizia Pasqua, Cassata, Paolo, Contini, Thierry, Golden-Marx, Emmet, Guaita, Lucia, Gururajan, Gayathri, Koekemoer, Anton M., McLeod, Derek, Tasca, Lidia A. M., Tresse, Laurence, Vergani, Daniela, Zucca, Elena
We present six spectroscopically confirmed massive protostructures, spanning a redshift range of $2.5
Externí odkaz:
http://arxiv.org/abs/2312.04634
Autor:
Zhong, Fucheng, Napolitano, Nicola R., Heneka, Caroline, Li, Rui, Bauer, Franz Erik, Bouche, Nicolas, Comparat, Johan, Kim, Young-Lo, Krogager, Jens-Kristian, Longhetti, Marcella, Loveday, Jonathan, Roukema, Boudewijn F., Rouse, Benedict L., Salvato, Mara, Tortora, Crescenzo, Assef, Roberto J., Cassarà, Letizia P., Costantin, Luca, Croom, Scott, Davies, Luke J M, Fritz, Alexander, Guiglion, Guillaume, Humphrey, Andrew, Pompei, Emanuela, Ricci, Claudio, Sifón, Cristóbal, Tempel, Elmo, Zafar, Tayyaba
Large sky spectroscopic surveys have reached the scale of photometric surveys in terms of sample sizes and data complexity. These huge datasets require efficient, accurate, and flexible automated tools for data analysis and science exploitation. We p
Externí odkaz:
http://arxiv.org/abs/2311.04146
Autor:
Forrest, Ben, Lemaux, Brian C., Shah, Ekta, Staab, Priti, McConachie, Ian, Cucciati, Olga, Gal, Roy R., Hung, Denise, Lubin, Lori M., Cassarà, Letizia P., Cassata, Paolo, Chang, Wenjun, Cooper, M. C., Decarli, Roberto, Gomez, Percy, Gururajan, Gayathri, Hathi, Nimish, Kashino, Daichi, Marchesini, Danilo, Marsan, Z. Cemile, McDonald, Michael, Muzzin, Adam, Shen, Lu, Stawinski, Stephanie Urbano, Talia, Margherita, Vergani, Daniela, Wilson, Gillian, Zamorani, Giovanni
Motivated by spectroscopic confirmation of three overdense regions in the COSMOS field at $z\sim3.35$, we analyze the uniquely deep multi-wavelength photometry and extensive spectroscopy available in the field to identify any further related structur
Externí odkaz:
http://arxiv.org/abs/2307.15113
Autor:
Schulze, Steve, Fransson, Claes, Kozyreva, Alexandra, Chen, Ting-Wan, Yaron, Ofer, Jerkstrand, Anders, Gal-Yam, Avishay, Sollerman, Jesper, Yan, Lin, Kangas, Tuomas, Leloudas, Giorgos, Omand, Conor M. B., Smartt, Stephen J., Yang, Yi, Nicholl, Matt, Sarin, Nikhil, Yao, Yuhan, Brink, Thomas G., Sharon, Amir, Rossi, Andrea, Chen, Ping, Chen, Zhihao, Cikota, Aleksandar, De, Kishalay, Drake, Andrew J., Filippenko, Alexei V., Fremling, Christoffer, Freour, Laurane, Fynbo, Johan P. U., Ho, Anna Y. Q., Inserra, Cosimo, Irani, Ido, Kuncarayakti, Hanindyo, Lunnan, Ragnhild, Mazzali, Paolo, Ofek, Eran O., Palazzi, Eliana, Perley, Daniel A., Pursiainen, Miika, Rothberg, Barry, Shingles, Luke J., Smith, Ken, Taggart, Kirsty, Tartaglia, Leonardo, Zheng, WeiKang, Anderson, Joseph P., Cassara, Letizia, Christensen, Eric, Djorgovski, S. George, Galbany, Lluis, Gkini, Anamaria, Graham, Matthew J., Gromadzki, Mariusz, Groom, Steven L., Hiramatsu, Daichi, Howell, D. Andrew, Kasliwal, Mansi M., McCully, Curtis, Müller-Bravo, Tomas E., Paiano, Simona, Paraskeva, Emmanouela, Pessi, Priscila J., Polishook, David, Rau, Arne, Rigault, Mickael, Rusholme, Ben
Abridged - Stars with ZAMS masses between 140 and $260 M_\odot$ are thought to explode as pair-instability supernovae (PISNe). During their thermonuclear runaway, PISNe can produce up to several tens of solar masses of radioactive nickel, resulting i
Externí odkaz:
http://arxiv.org/abs/2305.05796
Autor:
Bisogni, Susanna, Gargiulo, Adriana, Fumana, Marco, Franzetti, Paolo, Cassarà, Letizia Pasqua, Scodeggio, Marco, Garilli, Bianca, Vietri, Giustina
SIPGI is a spectroscopic pipeline for the data reduction of optical/near-infrared data acquired by slit-based spectrographs. SIPGI is a complete spectroscopic data reduction environment retaining the high level of flexibility and accuracy typical of
Externí odkaz:
http://arxiv.org/abs/2212.05580
Autor:
Casasola, Viviana, Bianchi, Simone, Magrini, Laura, Mosenkov, Aleksandr V., Salvestrini, Francesco, Baes, Maarten, Calura, Francesco, Cassara', Letizia P., Clark, Christopher J. R., Corbelli, Edvige, Fritz, Jacopo, Galliano, Frederic, Liuzzo, Elisabetta, Madden, Suzanne, Nersesian, Angelos, Pozzi, Francesca, Roychowdhury, Sambit, Baronchelli, Ivano, Bonato, Matteo, Gruppioni, Carlotta, Pantoni, Lara
Publikováno v:
A&A 668, A130 (2022)
We perform a homogeneous analysis of an unprecedented set of spatially resolved scaling relations (SRs) between ISM components and other properties in the range of scales 0.3-3.4 kpc. We also study some ratios: dust-to-stellar, dust-to-gas, and dust-
Externí odkaz:
http://arxiv.org/abs/2210.15993