Zobrazeno 1 - 10
of 85
pro vyhledávání: '"Mccracken, Henry J."'
Autor:
Gentile, Fabrizio, Casey, Caitlin M., Akins, Hollis B., Franco, Maximilien, McKinney, Jed, Berman, Edward, Cooper, Olivia R., Drakos, Nicole E., Hirschmann, Michaela, Long, Arianna S., Magdis, Georgios, Koekemoer, Anton M., Kokorev, Vasily, Shuntov, Marko, Talia, Margherita, Allen, Natalie, Harish, Santosh, Ilbert, Olivier, McCracken, Henry J., Kartaltepe, Jeyhan S., Liu, Daizhong, Paquereau, Louise, Rhodes, Jason, Rich, Michael R., Robertson, Brant, Toft, Sune, Gozaliasl, Ghassem
We present the properties of two candidate massive ($M_\star\sim10^{11}M_\odot$) and dusty ($A_{\rm v}>2.5$ mag) galaxies at $z=5-7$ in the first 0.28 deg$^2$ of the COSMOS-Web survey. One object is spectroscopically confirmed at $z_{\rm spec}=5.051$
Externí odkaz:
http://arxiv.org/abs/2408.10305
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:
Gould, Katriona M. L., Brammer, Gabriel, Valentino, Francesco, Whitaker, Katherine E., Weaver, John R., Lagos, Claudia del P., Rizzo, Francesca, Franco, Maximilien, Hseih, Bau-Ching, Ilbert, Olivier, Jin, Shuowen, Magdis, Georgios, McCracken, Henry J., Mobasher, Bahram, Shuntov, Marko, Steinhardt, Charles L., Strait, Victoria, Toft, Sune
We select and characterise a sample of massive (log(M$_{*}/$M$_{\odot})>10.6$) quiescent galaxies (QGs) at $3
Externí odkaz:
http://arxiv.org/abs/2302.10934
Autor:
Ito, Kei, Tanaka, Masayuki, Valentino, Francesco, Toft, Sune, Brammer, Gabriel, Gould, Katriona M. L., Ilbert, Olivier, Kashikawa, Nobunari, Kubo, Mariko, Liang, Yongming, McCracken, Henry J., Weaver, John R.
Protoclusters of galaxies have been found in the last quarter century. However, most of them have been found through the overdensity of star-forming galaxies, and there had been no known structures identified by multiple spectroscopically confirmed q
Externí odkaz:
http://arxiv.org/abs/2301.08845
Autor:
Chartab, Nima, Mobasher, Bahram, Cooray, Asantha, Hemmati, Shoubaneh, Sattari, Zahra, Ferguson, Henry C., Sanders, David B., Weaver, John R., Stern, Daniel, McCracken, Henry J., Masters, Daniel C., Toft, Sune, Capak, Peter L., Davidzon, Iary, Dickinson, Mark, Rhodes, Jason, Moneti, Andrea, Ilbert, Olivier, Zalesky, Lukas, McPartland, Conor, Szapudi, Istvan, Koekemoer, Anton M., Teplitz, Harry I., Giavalisco, Mauro
We present a new method based on information theory to find the optimal number of bands required to measure the physical properties of galaxies with a desired accuracy. As a proof of concept, using the recently updated COSMOS catalog (COSMOS2020), we
Externí odkaz:
http://arxiv.org/abs/2208.14781
Autor:
Stefanon, Mauro, Labbé, Ivo, Bouwens, Rychard J., Oesch, Pascal, Ashby, Matthew L. N., Caputi, Karina I., Franx, Marijn, Fynbo, Johan P. U., Illingworth, Garth D., Fèvre, Olivier Le, Marchesini, Danilo, McCracken, Henry J., Milvang-Jensen, Bo, Muzzin, Adam, van Dokkum, Pieter
We present 16 new ultrabright $H_{AB}\lesssim25$ galaxy candidates at z~8 identified over the COSMOS/UltraVISTA field. The new search takes advantage of the deepest-available ground-based optical and near-infrared observations, including the DR3 rele
Externí odkaz:
http://arxiv.org/abs/1902.10713
Autor:
Gozaliasl, Ghassem, Finoguenov, Alexis, Tanaka, Masayuki, Dolag, Klaus, Montanari, Francesco, Kirkpatrick, Charles C., Vardoulaki, Eleni, Khosroshahi, Habib G., Salvato, Mara, Laigle, Clotilde, McCracken, Henry J., Ilbert, Olivier, Cappelluti, Nico, Daddi, Emanuele, Hasinger, Guenther, Capak, Peter, Scoville, Nick Z., Toft, Sune, Civano, Francesca, Griffiths, Richard E., Balogh, Michael, Li, Yanxia, Ahoranta, Jussi, Mei, Simona, Iovino, Angela, Henriques, Bruno M. B., Erfanianfar, Ghazaleh
Publikováno v:
MNRAS, 483 (2019), 3545-3565
We present the results of a search for galaxy clusters and groups in the $\sim2$ square degree of the COSMOS field using all available X-ray observations from the XMM-Newton and Chandra observatories. We reach an X-ray flux limit of $3\times10^{-16}\
Externí odkaz:
http://arxiv.org/abs/1812.01604
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Ashby, M. L. N., Caputi, Karina I., Cowley, Will, Deshmukh, Smaran, Dunlop, James S., Milvang-Jensen, Bo, Fynbo, Johan P. U., Muzzin, Adam, McCracken, Henry J., Fevre, Olivier Le, Huang, Jia-Sheng, Zhang, Jessica
This paper describes new deep 3.6 and 4.5 micron imaging of three UltraVISTA near-infrared survey stripes within the COSMOS field. The observations were carried out with Spitzer's Infrared Array Camera (IRAC) for the Spitzer Matching Survey of the Ul
Externí odkaz:
http://arxiv.org/abs/1801.02660
Autor:
Gozaliasl, Ghassem, Finoguenov, Alexis, Khosroshahi, Habib G., Henriques, Bruno M. B., Tanaka, Masayuki, Ilbert, Olivier, Wuyts, Stijn, McCracken, Henry J., Montanari, Francesco
We performed a detailed study of the evolution of the star formation rate (SFR) and stellar mass of the brightest group galaxies (BGGs) and their relative contribution to the total baryon budget within $R_{200}$ ($f^{BGG}_{b,200}$). The sample compri
Externí odkaz:
http://arxiv.org/abs/1801.01492