Zobrazeno 1 - 10
of 323
pro vyhledávání: '"Scoville, Nick"'
Autor:
Darvish, Behnam, Chartab, Nima, Sattari, Zahra, Taamoli, Sina, Shivaei, Irene, Scoville, Nick, Hemmati, Shoubaneh, Sanders, David
We spectroscopically confirm a new protocluster in the COSMOS field at $z$=2.24430 with Keck/MOSFIRE, dubbed CC2.2B, which is in the immediate vicinity of CC2.2A protocluster, originally presented in \cite{Darvish20}. CC2.2B and CC2.2A centroids are
Externí odkaz:
http://arxiv.org/abs/2410.15177
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:
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:
Taamoli, Sina, Mobasher, Bahram, Chartab, Nima, Darvish, Behnam, Weaver, John R., Hemmati, Shoubaneh, Casey, Caitlin M., Sattari, Zahra, Brammer, Gabriel B., Capak, Peter L., Ilbert, Olivier, Kartaltepe, Jeyhan S., McCracken, Henry J., Moneti, Andrea, Sanders, David B., Scoville, Nick Z., Steinhardt, Charles L., Toft, Sune
To study the role of environment in galaxy evolution, we reconstruct the underlying density field of galaxies based on COSMOS2020 (The Farmer catalog) and provide the density catalog for a magnitude limited ($K_{s}<24.5$) sample of $\sim 210 \, k$ ga
Externí odkaz:
http://arxiv.org/abs/2312.10222
Autor:
Koda, Jin, Hirota, Akihiko, Egusa, Fumi, Sakamoto, Kazushi, Sawada, Tsuyoshi, Heyer, Mark, Baba, Junichi, Boissier, Samuel, Calzetti, Daniela, Meyer, Jennifer Donovan, Elmegreen, Bruce G., de Paz, Armando Gil, Harada, Nanase, Ho, Luis C., Kobayashi, Masato I. N., Kuno, Nario, Lee, Amanda M, Madore, Barry F., Maeda, Fumiya, Martin, Sergio, Muraoka, Kazuyuki, Nakanishi, Kouichiro, Onodera, Sachiko, Pineda, Jorge L., Scoville, Nick, Watanabe, Yoshimasa
We present high-fidelity CO(1-0) imaging of molecular gas across the full star-forming disk of M83, using ALMA's 12m, 7m, and TP arrays and the MIRIAD package. The data have a mass sensitivity and resolution of 10^4Msun and 40 pc. The full disk cover
Externí odkaz:
http://arxiv.org/abs/2303.12108
Autor:
Casey, Caitlin M., Kartaltepe, Jeyhan S., Drakos, Nicole E., Franco, Maximilien, Harish, Santosh, Paquereau, Louise, Ilbert, Olivier, Rose, Caitlin, Cox, Isabella G., Nightingale, James W., Robertson, Brant E., Silverman, John D., Koekemoer, Anton M., Massey, Richard, McCracken, Henry Joy, Rhodes, Jason, Akins, Hollis B., Amvrosiadis, Aristeidis, Arango-Toro, Rafael C., Bagley, Micaela B., Bongiorno, Angela, Capak, Peter L., Champagne, Jaclyn B., Chartab, Nima, Ortiz, Oscar A. Chavez, Chworowsky, Katherine, Cooke, Kevin C., Cooper, Olivia R., Darvish, Behnam, Ding, Xuheng, Faisst, Andreas L., Finkelstein, Steven L., Fujimoto, Seiji, Gentile, Fabrizio, Gillman, Steven, Gould, Katriona M. L., Gozaliasl, Ghassem, Hayward, Christopher C., He, Qiuhan, Hemmati, Shoubaneh, Hirschmann, Michaela, Jahnke, Knud, Jin, Shuowen, Khostovan, Ali Ahmad, Kokorev, Vasily, Lambrides, Erini, Laigle, Clotilde, Larson, Rebecca L., Leung, Gene C. K., Liu, Daizhong, Liaudat, Tobias, Long, Arianna S., Magdis, Georgios, Mahler, Guillaume, Mainieri, Vincenzo, Manning, Sinclaire M., Maraston, Claudia, Martin, Crystal L., McCleary, Jacqueline E., McKinney, Jed, McPartland, Conor J. R., Mobasher, Bahram, Pattnaik, Rohan, Renzini, Alvio, Rich, R. Michael, Sanders, David B., Sattari, Zahra, Scognamiglio, Diana, Scoville, Nick, Sheth, Kartik, Shuntov, Marko, Sparre, Martin, Suzuki, Tomoko L., Talia, Margherita, Toft, Sune, Trakhtenbrot, Benny, Urry, C. Megan, Valentino, Francesco, Vanderhoof, Brittany N., Vardoulaki, Eleni, Weaver, John R., Whitaker, Katherine E., Wilkins, Stephen M., Yang, Lilan, Zavala, Jorge A.
We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations. COSMOS-Web is a contiguous 0.54 deg$^2$ NIRCam imaging survey in fou
Externí odkaz:
http://arxiv.org/abs/2211.07865
Autor:
Scoville, Nick, Faisst, Andreas, Weaver, John, Toft, Sune, McCracken, Henry, Ilbert, Olivier, Diaz-Santos, Tanio, Staguhn, Johannes, Koda, Jin, Casey, Caitlin, Sanders, David, Mobasher, Bahram, Chartab, Nima, Sattari, Zahra, Capak, Peter, Bout, Paul Vanden, Bongiorno, Angela, Vlahakis, Catherine, Sheth, Kartik, Yun, Min, Aussel, Herve, Laigle, Clotilde, Masters, Dan
ALMA observations of the long wavelength dust continuum are used to estimate the gas masses in a sample of 708 star-forming (SF) galaxies at z = 0.3 to 4.5. We determine the dependence of gas masses and star formation efficiencies (SFE=SFR per unit g
Externí odkaz:
http://arxiv.org/abs/2211.07836
Autor:
Burnham, Anne D., Casey, Caitlin M., Zavala, Jorge A., Manning, Sinclaire M., Spilker, Justin S., Chapman, Scott C., Chen, Chian-Chou, Cooray, Asantha, Sanders, David B., Scoville, Nick Z.
The underlying distribution of galaxies' dust SEDs (i.e., their spectra re-radiated by dust from rest-frame $\sim$3$\mu$m-3mm) remains relatively unconstrained due to a dearth of FIR/(sub)mm data for large samples of galaxies. It has been claimed in
Externí odkaz:
http://arxiv.org/abs/2102.06250
Autor:
Sattari, Zahra, Mobasher, Bahram, Chartab, Nima, Darvish, Behnam, Shivaei, Irene, Scoville, Nick, Sobral, David
We study the mass-metallicity relation for 19 members of a spectroscopically-confirmed protocluster in the COSMOS field at $z=2.2$ (CC2.2), and compare it with that of 24 similarly selected field galaxies at the same redshift. Both samples are $\rm H
Externí odkaz:
http://arxiv.org/abs/2102.05637
Autor:
Shivaei, Irene, Darvish, Behnam, Sattari, Zahra, Chartab, Nima, Mobasher, Bahram, Scoville, Nick, Rieke, George
Publikováno v:
The Astrophysical Journal Letters 2020, Volume 903, Issue 2, id.L28, 7 pp
We use a sample of star-forming field and protocluster galaxies at z=2.0-2.5 with Keck/MOSFIRE K-band spectra, a wealth of rest-frame UV photometry, and Spitzer/MIPS and Herschel/PACS observations, to dissect the relation between the ratio of IR to U
Externí odkaz:
http://arxiv.org/abs/2010.10538