Zobrazeno 1 - 10
of 128
pro vyhledávání: '"ANDRADE, E. F."'
Autor:
Castillo, Marta Frias, Rybak, Matus, Hodge, Jacqueline A., Van der Werk, Paul, Smail, Ian, Butterworth, Joshua, Jansen, Jasper, Topkaras, Theodoros, Chen, Chian-Chou, Chapman, Scott C., Weiss, Axel, Algera, Hiddo, Birkin, Jack E., da Cunha, Elisabete, Chen, Jianhang, Dannerbauer, Helmut, Jiménez-Andrade, E. F., Ikarashi, Soh, Liao, Cheng-Lin, Murphy, Eric J., Swinbank, A. M., Walter, Fabian, Rivera, Gabriela Calistro, Ivison, R. J., Lagos, Claudia del P.
The CO(1--0) and [\ion{C}{1}](1--0) emission lines are well-established tracers of cold molecular gas mass in local galaxies. At high redshift, where the interstellar medium (ISM) is likely to be denser, there have been limited direct comparisons of
Externí odkaz:
http://arxiv.org/abs/2404.05596
Publikováno v:
A&A 675, A126 (2023)
Radio used as a star formation rate (SFR) tracer presents enormous advantages by being unaffected by dust and radio sources being pinpointed at the sub-arc-second level. The interpretation of the low frequency 1.4 GHz luminosity is hampered by the di
Externí odkaz:
http://arxiv.org/abs/2304.13758
Autor:
Fujimoto, Seiji, Finkelstein, Steven L., Burgarella, Denis, Carilli, Chris L., Buat, Véronique, Casey, Caitlin M., Ciesla, Laure, Tacchella, Sandro, Zavala, Jorge A., Brammer, Gabriel, Fudamoto, Yoshinobu, Ouchi, Masami, Valentino, Francesco, Cooper, M. C., Dickinson, Mark, Franco, Maximilien, Giavalisco, Mauro, Hutchison, Taylor A., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Kojima, Takashi, Larson, Rebecca L., Murphy, Eric J., Papovich, Casey, Pérez-González, Pablo G., Somerville, Rachel S., Yoon, Ilsang, Wilkins, Stephen M., Yung, L. Y. Aaron, Akins, Hollis, Amorín, Ricardo O., Haro, Pablo Arrabal, Bagley, Micaela B., Chworowsky, Katherine, Cleri, Nikko J., Cooper, Olivia R., Costantin, Luca, Daddi, Emanuele, Ferguson, Henry C., Grogin, Norman A., Jiménez-Andrade, E. F., Juneau, Stéphanie, Kirkpatrick, Allison, Kocevski, Dale D., Bail, Aurélien Le, Long, Arianna, Lucas, Ray A., Magnelli, Benjamin, McKinney, Jed, Rose, Caitlin, Seillé, Lise-Marie, Simons, Raymond C., Weiner, Benjamin J.
We present ALMA Band~7 observations of a remarkably bright galaxy candidate at $z_{\rm phot}$=$16.7^{+1.9}_{-0.3}$ ($M_{\rm UV}$=$-21.6$), S5-z17-1, identified in JWST Early Release Observation data of Stephen's Quintet. We do not detect the dust con
Externí odkaz:
http://arxiv.org/abs/2211.03896
Autor:
Jiménez-Andrade, E. F., Cantalupo, S., Magnelli, B., Romano-Díaz, E., Gómez-Guijarro, C., Mackenzie, R., Smolčić, V., Murphy, E., Matthee, J., Toft, S.
Ly$\alpha$ $\lambda$1216 (Ly$\alpha$) emission extending over $\gtrsim\,\rm 10\,kiloparsec\,(kpc)$ around dusty, massive starbursts at $z\gtrsim3$ might represent a short-lived phase in the evolution of present-day, massive quiescent galaxies. To obt
Externí odkaz:
http://arxiv.org/abs/2210.07982
Autor:
Zavala, Jorge A., Buat, Veronique, Casey, Caitlin M., Burgarella, Denis, Finkelstein, Steven L., Bagley, Micaela B., Ciesla, Laure, Daddi, Emanuele, Dickinson, Mark, Ferguson, Henry C., Franco, Maximilien, Jim'enez-Andrade, E. F., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Bail, Aurélien Le, Murphy, E. J., Papovich, Casey, Tacchella, Sandro, Wilkins, Stephen M., Aretxaga, Itziar, Behroozi, Peter, Champagne, Jaclyn B., Fontana, Adriano, Giavalisco, Mauro, Grazian, Andrea, Grogin, Norman A., Kewley, Lisa J., Kocevski, Dale D., Kirkpatrick, Allison, Lotz, Jennifer M., Pentericci, Laura, Perez-Gonzalez, Pablo G., Pirzkal, Nor, Ravindranath, Swara, Somerville, Rachel S., Trump, Jonathan R., Yang, Guang, Yung, L. Y. Aaron, Almaini, Omar, Amorin, Ricardo O., Annunziatella, Marianna, Haro, Pablo Arrabal, Backhaus, Bren E., Barro, Guillermo, Bell, Eric F., Bhatawdekar, Rachana, Bisigello, Laura, Buitrago, Fernando, Calabro, Antonello, Castellano, Marco, Ortiz, Oscar A. Chavez, Chworowsky, Katherine, Cleri, Nikko J., Cohen, Seth H., Cole, Justin W., Cooke, Kevin C., Cooper, M. C., Cooray, Asantha R., Costantin, Luca, Cox, Isabella G., Croton, Darren, Dave, Romeel, de la Vega, Alexander, Dekel, Avishai, Elbaz, David, Estrada-Carpenter, Vicente, Fernández, Vital, Finkelstein, Keely D., Freundlich, Jonathan, Fujimoto, Seiji, García-Argumánez, Ángela, Gardner, Jonathan P., Gawiser, Eric, Gómez-Guijarro, Carlos, Guo, Yuchen, Hamilton, Timothy S., Hathi, Nimish P., Holwerda, Benne W., Hirschmann, Michaela, Huertas-Company, Marc, Hutchison, Taylor A., Iyer, Kartheik G., Jaskot, Anne E., Jha, Saurabh W., Jogee, Shardha, Juneau, Stéphanie, Jung, Intae, Kassin, Susan A., Kurczynski, Peter, Larson, Rebecca L., Leung, Gene C. K., Long, Arianna, Lucas, Ray A., Magnelli, Benjamin, Mantha, Kameswara Bharadwaj, Matharu, Jasleen, McGrath, Elizabeth J., McIntosh, Daniel H., Medrano, Aubrey, Merlin, Emiliano, Mobasher, Bahram, Morales, Alexa M., Newman, Jeffrey A., Nicholls, David C., Pandya, Viraj, Rafelski, Marc, Ronayne, Kaila, Rose, Caitlin, Ryan Jr., Russell E., Santini, Paola, Seillé, Lise-Marie, Shah, Ekta A., Shen, Lu, Simons, Raymond C., Snyder, Gregory F., Stanway, Elizabeth R., Straughn, Amber N., Teplitz, Harry I., Vanderhoof, Brittany N., Vega-Ferrero, Jesús, Wang, Weichen, Weiner, Benjamin J., Willmer, Christopher N. A., Wuyts, Stijn
Publikováno v:
ApJL 943 L9 (2023)
Lyman Break Galaxy (LBG) candidates at z>10 are rapidly being identified in JWST/NIRCam observations. Due to the (redshifted) break produced by neutral hydrogen absorption of rest-frame UV photons, these sources are expected to drop out in the bluer
Externí odkaz:
http://arxiv.org/abs/2208.01816
Autor:
Heywood, I., Murphy, E. J., Jiménez-Andrade, E. F., Armus, L., Cotton, W. D., DeCoursey, C., Dickinson, M., Lazio, T. J. W., Momjian, E., Penner, K., Smail, I., Smirnov, O. M.
The Frontier Fields project is an observational campaign targeting six galaxy clusters, with the intention of using the magnification provided by gravitational lensing to study galaxies that are extremely faint or distant. We used the Karl G. Jansky
Externí odkaz:
http://arxiv.org/abs/2103.07806
Autor:
Jiménez-Andrade, E. F., Murphy, E. J., Heywood, I., Smail, I., Penner, K., Momjian, E., Dickinson, M., Armus, L., Lazio, T. J. W.
To investigate the growth history of galaxies, we measure the rest-frame radio, ultraviolet (UV), and optical sizes of 98 radio-selected, star-forming galaxies (SFGs) distributed over $0.3 \lesssim z \lesssim 3$ and median stellar mass of $\log(M_\st
Externí odkaz:
http://arxiv.org/abs/2103.07807
Autor:
Fraternali, F., Karim, A., Magnelli, B., Gómez-Guijarro, C., Jiménez-Andrade, E. F., Posses, A. C.
Publikováno v:
A&A 647, A194 (2021)
Massive starburst galaxies in the early Universe are estimated to have depletion times of $\sim 100$ Myr and thus be able to convert their gas very quickly into stars, possibly leading to a rapid quenching of their star formation. For these reasons,
Externí odkaz:
http://arxiv.org/abs/2011.05340
Autor:
Harrington, Kevin C., Weiss, Axel, Yun, Min S., Magnelli, Benjamin, Sharon, C. E., Leung, T. K. D., Vishwas, A., Wang, Q. D., Jimenez-Andrade, E. F., Frayer, D. T., Liu, D., Garcia, P., Romano-Diaz, E., Frye, B. L., Jarugula, S., Badescu, T., Berman, D., Dannerbauer, H., Diaz-Sanchez, A., Grassitelli, L., Kamieneski, P., Kim, W. J., Kirkpatrick, A., Lowenthal, J. D., Messias, H., Puschnig, J., Stacey, G. J., Torne, P., Bertoldi, F.
Dusty star-forming galaxies at high redshift (1 < z < 3) represent the most intense star-forming regions in the Universe. Key aspects to these processes are the gas heating and cooling mechanisms. Although it is well known that these galaxies are gas
Externí odkaz:
http://arxiv.org/abs/2010.16231
Autor:
Vardoulaki, E., Andrade, E. F. Jiménez, Delvecchio, I., Smolčić, V., Schinnerer, E., Sargent, M. T., Gozaliasl, G., Finoguenov, A., Bondi, M., Zamorani, G., Badescu, T., Leslie, S. K., Ceraj, L., Tisanić, K., Karim, A., Magnelli, B., Bertoldi, F., Romano-Diaz, E., Harrington, K.
Publikováno v:
A&A 648, A102 (2021)
($ABRIDGED$) We probe the physical properties and large-scale environment of radio AGN in the faintest FR population to-date, and link them to their radio structure. We use the VLA-COSMOS Large Project at 3 GHz, with resolution and sensitivity of 0".
Externí odkaz:
http://arxiv.org/abs/2009.10721