Zobrazeno 1 - 10
of 80
pro vyhledávání: '"Long, Arianna S"'
Autor:
Cooper, Olivia R., Brammer, Gabriel, Heintz, Kasper E., Toft, Sune, Casey, Caitlin M., Setton, David J., de Graaff, Anna, Boogaard, Leindert, Cleri, Nikko J., Gillman, Steven, Gottumukkala, Rashmi, Greene, Jenny E., Gullberg, Bitten, Hirschmann, Michaela, Hviding, Raphael E., Lambrides, Erini, Leja, Joel, Long, Arianna S., Manning, Sinclaire M., Maseda, Michael V., McConachie, Ian, McKinney, Jed, Narayanan, Desika, Price, Sedona H., Strait, Victoria, Weibel, Andrea, Williams, Christina C.
The dearth of high quality spectroscopy of dusty star-forming galaxies (DSFGs) -- the main drivers of the assembly of dust and stellar mass at the peak of activity in the Universe -- greatly hinders our ability to interpret their physical processes a
Externí odkaz:
http://arxiv.org/abs/2410.08387
Autor:
Lambrides, Erini, Garofali, Kristen, Larson, Rebecca, Ptak, Andrew, Chiaberge, Marco, Long, Arianna S., Hutchison, Taylor A., Norman, Colin, McKinney, Jed, Akins, Hollis B., Berg, Danielle A., Chisholm, John, Civano, Francesca, Cloonan, Aidan P., Endsley, Ryan, Faisst, Andreas L., Gilli, Roberto, Gillman, Steven, Hirschmann, Michaela, Kartaltepe, Jeyhan S., Kocevski, Dale D., Kokorev, Vasily, Pacucci, Fabio, Richardson, Chris T., Stiavelli, Massimo, Whalen, Kelly E.
A multitude of JWST studies reveal a surprising over-abundance of over-massive accreting super-massive blackholes (SMBHs) -- leading to a deepening tension between theory and observation in the first billion years of cosmic time. Across X-ray to infr
Externí odkaz:
http://arxiv.org/abs/2409.13047
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:
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:
McKinney, Jed, Casey, Caitlin M., Long, Arianna S., Cooper, Olivia R., Manning, Sinclaire M., Franco, Maximilien, Akin, Hollis, Lambrides, Erini, Gammon, Elaine, Silva, Camila, Gentile, Fabrizio, Zavala, Jorge A., Amvrosiadis, Aristeidis, Andika, Irma, Brinch, Malte, Champagne, Jaclyn B., Chartab, Nima, Drakos, Nicole E., Faisst, Andreas L., Fujimoto, Seiji, Gillman, Steven, Gozaliasl, Ghassem, Greve, Thomas R., Harish, Santosh, Hayward, Christopher C., Hirschmann, Michaela, Ilbert, Olivier, Kalita, Boris S., Kartaltepe, Jeyhan S., Koekemoer, Anton M., Kokorev, Vasily, Liu, Daizhong, Magdis, Georgios, McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant E., Talia, Margherita, Valentino, Francesco, Vijayan, Aswin P.
JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of sub-millimeter galaxies, revealing detail that was previously inaccessible. In this work we construct a sample of 289 sub-millimeter galaxies with d
Externí odkaz:
http://arxiv.org/abs/2408.08346
Autor:
Casey, Caitlin M., Akins, Hollis B., Kokorev, Vasily, McKinney, Jed, Cooper, Olivia R., Long, Arianna S., Franco, Maximilien, Manning, Sinclaire M.
JWST has revealed a ubiquitous population of ``little red dots'' (LRDs) at $z\gtrsim4$, selected via their red rest-frame optical emission and compact morphologies. They are thought to be reddened by dust, whether in tori of active galactic nuclei or
Externí odkaz:
http://arxiv.org/abs/2407.05094
Autor:
Akins, Hollis B., Casey, Caitlin M., Lambrides, Erini, Allen, Natalie, Andika, Irham T., Brinch, Malte, Champagne, Jaclyn B., Cooper, Olivia, Ding, Xuheng, Drakos, Nicole E., Faisst, Andreas, Finkelstein, Steven L., Franco, Maximilien, Fujimoto, Seiji, Gentile, Fabrizio, Gillman, Steven, Gozaliasl, Ghassem, Harish, Santosh, Hayward, Christopher C., Hirschmann, Michaela, Ilbert, Olivier, Kartaltepe, Jeyhan S., Kocevski, Dale D., Koekemoer, Anton M., Kokorev, Vasily, Liu, Daizhong, Long, Arianna S., McCracken, Henry Joy, McKinney, Jed, Onoue, Masafusa, Paquereau, Louise, Renzini, Alvio, Rhodes, Jason, Robertson, Brant E., Shuntov, Marko, Silverman, John D., Tanaka, Takumi S., Toft, Sune, Trakhtenbrot, Benny, Valentino, Francesco, Zavala, Jorge
JWST has revealed a population of compact and extremely red galaxies at $z>4$, which likely host active galactic nuclei (AGN). We present a sample of 434 ``little red dots'' (LRDs), selected from the 0.54 deg$^2$ COSMOS-Web survey. We fit galaxy and
Externí odkaz:
http://arxiv.org/abs/2406.10341
Autor:
Cooper, Olivia R., Casey, Caitlin M., Akins, Hollis B., Magee, Jake, Melendez, Alfonso, Fong, Mia, Stawinski, Stephanie M. Urbano, Kartaltepe, Jeyhan S., Finkelstein, Steven L., Larson, Rebecca L., Jung, Intae, Bista, Ash, Champagne, Jaclyn B., Ortiz, Oscar A. Chavez, Coffin, Sadie, Cooper, M. C., Drakos, Nicole, Faisst, Andreas L., Franco, Maximilien, Fujimoto, Seiji, Gillman, Steven, Gozaliasl, Ghassem, Harish, Santosh, Hutchison, Taylor A., Koekemoer, Anton M., Kokorev, Vasily, Lertprasertpong, Jitrapon, Liu, Daizhong, Long, Arianna S., Papovich, Casey, Rich, R. Michael, Robertson, Brant E., Talia, Margherita, Vanderhoof, Brittany N., Whitaker, Katherine E., Zavala, Jorge A.
We present the first results from the Web Epoch of Reionization Lyman-$\alpha$ Survey (WERLS), a spectroscopic survey of Lyman-$\alpha$ emission using Keck I/MOSFIRE and LRIS. WERLS targets bright ($J<26$) galaxy candidates with photometric redshifts
Externí odkaz:
http://arxiv.org/abs/2309.06656
Autor:
Casey, Caitlin M., Akins, Hollis B., Shuntov, Marko, Ilbert, Olivier, Paquereau, Louise, Franco, Maximilien, Hayward, Christopher C., Finkelstein, Steven L., Boylan-Kolchin, Michael, Robertson, Brant E., Allen, Natalie, Brinch, Malte, Cooper, Olivia R., Ding, Xuheng, Drakos, Nicole E., Faisst, Andreas L., Fujimoto, Seiji, Gillman, Steven, Harish, Santosh, Hirschmann, Michaela, Jin, Shuowen, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Kokorev, Vasily, Liu, Daizhong, Long, Arianna S., Magdis, Georgios, Maraston, Claudia, Martin, Crystal L., McCracken, Henry Joy, McKinney, Jed, Mobasher, Bahram, Rhodes, Jason, Rich, R. Michael, Sanders, David B., Silverman, John D., Toft, Sune, Vijayan, Aswin P., Weaver, John R., Wilkins, Stephen M., Yang, Lilan, Zavala, Jorge A.
We report the discovery of 15 exceptionally luminous $10\lesssim z\lesssim14$ candidate galaxies discovered in the first 0.28 deg$^2$ of JWST/NIRCam imaging from the COSMOS-Web Survey. These sources span rest-frame UV magnitudes of $-20.5>M_{\rm UV}>
Externí odkaz:
http://arxiv.org/abs/2308.10932
Autor:
Franco, Maximilien, Akins, Hollis B., Casey, Caitlin M., Finkelstein, Steven L., Shuntov, Marko, Chworowsky, Katherine, Faisst, Andreas L., Fujimoto, Seiji, Ilbert, Olivier, Koekemoer, Anton M., Liu, Daizhong, Lovell, Christopher C., Maraston, Claudia, McCracken, Henry Joy, McKinney, Jed, Robertson, Brant E., Bagley, Micaela B., Champagne, Jaclyn B., Cooper, Olivia R., Ding, Xuheng, Drakos, Nicole E., Enia, Andrea, Gillman, Steven, Hayward, Christopher C., Hirschmann, Michaela, Kokorev, Vasily, Laigle, Clotilde, Long, Arianna S., Gozaliasl, Ghassem, Harish, Santosh, Jin, Shuowen, Kartaltepe, Jeyhan S., Magdis, Georgios, Mahler, Guillaume, Martin, Crystal L., Rich, R. Michael, Trakhtenbrot, Benny, Mobasher, Bahram, Paquereau, Louise, Renzini, Alvio, Rhodes, Jason, Sheth, Kartik, Silverman, John D., Sparre, Martin, Talia, Margherita, Valentino, Francesco, Vijayan, Aswin P., Wilkins, Stephen M., Yang, Lilan, Zavala, Jorge A.
We report the identification of 15 galaxy candidates at $z\ge9$ using the initial COSMOS-Web JWST observations over 77 arcmin$^2$ through four NIRCam filters (F115W, F150W, F277W, F444W) with an overlap with MIRI (F770W) of 8.7 arcmin$^2$. We fit the
Externí odkaz:
http://arxiv.org/abs/2308.00751