Zobrazeno 1 - 10
of 84
pro vyhledávání: '"Long, Arianna"'
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:
Lambrides, Erini, Chiaberge, Marco, Long, Arianna, Liu, Daizhong, Akins, Hollis B., Ptak, Andrew F., Andika, Irham Taufik, Capetti, Alessandro, Casey, Caitlin M., Champagne, Jaclyn B., Chworowsky, Katherine, Clarke, Tracy E., Cooper, Olivia R., Ding, Xuheng, Dong, Dillon Z., Faisst, Andreas L., Forman, Jordan Y., Franco, Maximilien, Gillman, Steven, Gozaliasl, Ghassem, Hall, Kirsten R., Harish, Santosh, Hayward, Christopher C., Hirschmann, Michaela, Hutchison, Taylor A., Jahnke, Knud, Jin, Shuowen, Kartaltepe, Jeyhan S., Kleiner, Emma T., Koekemoer, Anton M., Kokorev, Vasily, Manning, Sinclaire M., Martin, Crystal L., McKinney, Jed, Norman, Colin, Nyland, Kristina, Onoue, Masafusa, Robertson, Brant E., Shuntov, Marko, Silverman, John D., Stiavelli, Massimo, Trakhtenbrot, Benny, Vardoulaki, Eleni, Zavala, Jorge A., Allen, Natalie, Ilbert, Olivier, McCracken, Henry Joy, Paquereau, Louise, Rhodes, Jason, Toft, Sune
In this letter, we report the discovery of the highest redshift, heavily obscured, radio-loud AGN candidate selected using JWST NIRCam/MIRI, mid-IR, sub-mm, and radio imaging in the COSMOS-Web field. Using multi-frequency radio observations and mid-I
Externí odkaz:
http://arxiv.org/abs/2308.12823
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
Autor:
Long, Arianna S., Antwi-Danso, Jacqueline, Lambrides, Erini L., Lovell, Christopher C., de la Vega, Alexander, Valentino, Francesco, Zavala, Jorge A., Casey, Caitlin M., Wilkins, Stephen M., Yung, L. Y. Aaron, Haro, Pablo Arrabal, Bagley, Micaela B., Bisigello, Laura, Chworowsky, Katherine, Cooper, Michael C., Cooper, Olivia R., Cooray, Asantha R., Croton, Darren, Dickinson, Mark, Finkelstein, Steven L., Franco, Maximilien, Gould, Katriona M. L., Hirschmann, Michaela, Hutchison, Taylor A., Kartaltepe, Jeyhan S., Kocevski, Dale D., Koekemoer, Anton M., Lucas, Ray A., McKinney, Jed, Papovich, Casey, Perez-Gonzalez, Pablo G., Pirzkal, Nor, Santini, Paola
Substantial populations of massive quiescent galaxies at $z\ge3$ challenge our understanding of rapid galaxy growth and quenching over short timescales. In order to piece together this evolutionary puzzle, more statistical samples of these objects ar
Externí odkaz:
http://arxiv.org/abs/2305.04662
Autor:
Akins, Hollis B., Casey, Caitlin M., Allen, Natalie, Bagley, Micaela B., Dickinson, Mark, Finkelstein, Steven L., Franco, Maximilien, Harish, Santosh, Haro, Pablo Arrabal, Ilbert, Olivier, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Liu, Daizhong, Long, Arianna S., McCracken, Henry Joy, Paquereau, Louise, Papovich, Casey, Pirzkal, Nor, Rhodes, Jason, Robertson, Brant E., Shuntov, Marko, Toft, Sune, Yang, Guang, Barro, Guillermo, Bisigello, Laura, Buat, Véronique, Champagne, Jaclyn B., Cooper, Olivia, Costantin, Luca, de la Vega, Alexander, Drakos, Nicole E., Faisst, Andreas, Fontana, Adriano, Fujimoto, Seiji, Gillman, Steven, Gómez-Guijarro, Carlos, Gozaliasl, Ghassem, Hathi, Nimish P., Hayward, Christopher C., Hirschmann, Michaela, Holwerda, Benne W., Jin, Shuowen, Kocevski, Dale D., Kokorev, Vasily, Lambrides, Erini, Lucas, Ray A., Magdis, Georgios E., Magnelli, Benjamin, McKinney, Jed, Mobasher, Bahram, Pérez-González, Pablo G., Rich, R. Michael, Seillé, Lise-Marie, Talia, Margherita, Urry, C. Megan, Valentino, Francesco, Whitaker, Katherine E., Yung, L. Y. Aaron, Zavala, Jorge
We present a search for extremely red, dust-obscured, $z>7$ galaxies with $\textit{JWST}$/NIRCam+MIRI imaging over the first 20 arcmin$^2$ of publicly-available Cycle 1 data from the COSMOS-Web, CEERS, and PRIMER surveys. Based on their red color in
Externí odkaz:
http://arxiv.org/abs/2304.12347
Autor:
Champagne, Jaclyn B., Casey, Caitlin M., Finkelstein, Steven L., Bagley, Micaela, Cooper, Olivia R., Larson, Rebecca L., Long, Arianna S., Wang, Feige
The most luminous quasars at $z > 6$ are suspected to be both highly clustered and reside in the most massive dark matter halos in the early Universe, making them prime targets to search for galaxy overdensities and/or protoclusters. We search for Ly
Externí odkaz:
http://arxiv.org/abs/2304.10437
Autor:
Gómez-Guijarro, Carlos, Magnelli, Benjamin, Elbaz, David, Wuyts, Stijn, Daddi, Emanuele, Bail, Aurélien Le, Giavalisco, Mauro, Dickinson, Mark, Pérez-González, Pablo G., Haro, Pablo Arrabal, Bagley, Micaela B., Bisigello, Laura, Buat, Véronique, Burgarella, Denis, Calabrò, Antonello, Casey, Caitlin M., Cheng, Yingjie, Ciesla, Laure, Dekel, Avishai, Ferguson, Henry C., Finkelstein, Steven L., Franco, Maximilien, Grogin, Norman A., Holwerda, Benne W., Jin, Shuowen, Kartaltepe, Jeyhan S., Koekemoer, Anton M., Kokorev, Vasily, Long, Arianna S., Lucas, Ray A., Magdis, Georgios E., Papovich, Casey, Pirzkal, Nor, Seillé, Lise-Marie, Tacchella, Sandro, Tarrasse, Maxime, Valentino, Francesco, de la Vega, Alexander, Wilkins, Stephen M., Xiao, Mengyuan, Yung, L. Y. Aaron
Publikováno v:
A&A 677, A34 (2023)
In recent years, observations have uncovered a population of massive galaxies that are invisible or very faint in deep optical/near-infrared (near-IR) surveys but brighter at longer wavelengths. However, the nature of these optically dark or faint ga
Externí odkaz:
http://arxiv.org/abs/2304.08517
Autor:
McKinney, Jed, Manning, Sinclaire M., Cooper, Olivia R., Long, Arianna S., Akins, Hollis, Casey, Caitlin M., Faisst, Andreas L., Franco, Maximilien, Hayward, Christopher C., Lambrides, Erini, Magdis, Georgios, Whitaker, Katherine E., Yun, Min, Champagne, Jaclyn B., Drakos, Nicole E., Gentile, Fabrizio, Gillman, Steven, Gozaliasl, Ghassem, Ilbert, Olivier, Jin, Shuowen, Koekemoer, Anton M., Kokorev, Vasily, Liu, Daizhong, Rich, R. Michael, Robertson, Brant E., Valentino, Francesco, Weaver, John R., Zavala, Jorge A., Allen, Natalie, Kartaltepe, Jeyhan S., McCracken, Henry Joy, Paquereau, Louise, Rhodes, Jason, Shuntov, Marko, Toft, Sune
A growing number of far-infrared bright sources completely invisible in deep extragalactic optical surveys hint at an elusive population of z>4 dusty, star-forming galaxies. Cycle 1 JWST surveys are now detecting their rest-frame optical light, which
Externí odkaz:
http://arxiv.org/abs/2304.07316