Zobrazeno 1 - 10
of 309
pro vyhledávání: '"Williams, Christina C."'
Autor:
Curti, Mirko, Witstok, Joris, Jakobsen, Peter, Kobayashi, Chiaki, Curtis-Lake, Emma, Hainline, Kevin, Ji, Xihan, D'Eugenio, Francesco, Chevallard, Jacopo, Maiolino, Roberto, Scholtz, Jan, Carniani, Stefano, Arribas, Santiago, Baker, William M., Bhatawdekar, Rachana, Boyett, Kristan, Bunker, Andrew J., Cameron, Alex, Cargile, Phillip A., Charlot, Stephane, Eisenstein, Daniel J., Ji, Zhiyuan, Johnson, Benjamin D., Kumari, Nimisha, Maseda, Michael V., Robertson, Brant, Silcock, Maddie S., Tacchella, Sandro, Ubler, Hannah, Venturi, Giacomo, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris
We analyse ultra-deep JWST observations of the galaxy JADES-GS-z9-0 at z = 9.4327, and derive detailed stellar and interstellar medium (ISM) properties of this luminous (MUV=-20.43) high-redshift system. Complementary information from NIRCam imaging
Externí odkaz:
http://arxiv.org/abs/2407.02575
Autor:
Kumari, Nimisha, Smit, Renske, Witstok, Joris, Sirianni, Marco, Maiolino, Roberto, Bunker, Andrew J., Bhatawdekar, Rachana, Boyett, Kristan, Cameron, Alex J., Carniani, Stefano, Charlot, Stephane, Curti, Mirko, Curtis-Lake, Emma, D'Eugenio, Francesco, Eisenstein, Daniel J., Hainline, Kevin, Ji, Zhiyuan, Jones, Gareth C., Robertson, Brant, Saxena, Aayush, Scholtz, Jan, Simmonds, Charlotte, Williams, Christina C., Willmer, Christopher N. A.
We investigate the physical properties of Lyman-alpha emitters (LAEs) and non-Lyman-alpha emitters (non-LAEs) at z$\sim$4.8--9.6 via a stacking analysis of 253 JWST/NIRSpec spectra of galaxies observed as part of the JWST Advanced Deep Extragalactic
Externí odkaz:
http://arxiv.org/abs/2406.11997
Autor:
DeCoursey, Christa, Egami, Eiichi, Pierel, Justin D. R., Sun, Fengwu, Rest, Armin, Coulter, David A., Engesser, Michael, Siebert, Matthew R., Hainline, Kevin N., Johnson, Benjamin D., Bunker, Andrew J., Cargile, Phillip A., Charlot, Stephane, Chen, Wenlei, Curti, Mirko, DeFour-Remy, Shea, Eisenstein, Daniel J., Fox, Ori D., Gezari, Suvi, Gomez, Sebastian, Jencson, Jacob, Joshi, Bhavin A., Khairnar, Sanvi, Lyu, Jianwei, Maiolino, Roberto, Moriya, Takashi J., Quimby, Robert M., Rieke, George H., Rieke, Marcia J., Robertson, Brant, Shahbandeh, Melissa, Strolger, Louis-Gregory, Tacchella, Sandro, Wang, Qinan, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris, Zenati, Yossef
The JWST Advanced Deep Extragalactic Survey (JADES) is a multi-cycle JWST program that has taken among the deepest near-infrared images to date (down to $\sim$30.5 ABmag) over $\sim$25 arcmin$^2$ in the GOODS-S field in two sets of observations with
Externí odkaz:
http://arxiv.org/abs/2406.05060
Autor:
Rieke, George, Alberts, Stacey, Shivaei, Irene, Lyu, Jianwei, Willmer, Christopher N. A., Perez-Gonzalez, Pablo, Williams, Christina C.
The Mid-Infrared Instrument (MIRI) for JWST is supplied with a suite of imaging bandpass filters optimized for full spectral coverage in eight intermediate-width bands from 5 to 26 microns and a narrower one at 11.3 microns. This contrasts with previ
Externí odkaz:
http://arxiv.org/abs/2406.03518
Autor:
Adamo, Angela, Atek, Hakim, Bagley, Micaela B., Bañados, Eduardo, Barrow, Kirk S. S., Berg, Danielle A., Bezanson, Rachel, Bradač, Maruša, Brammer, Gabriel, Carnall, Adam C., Chisholm, John, Coe, Dan, Dayal, Pratika, Eisenstein, Daniel J., Eldridge, Jan J., Ferrara, Andrea, Fujimoto, Seiji, de Graaff, Anna, Habouzit, Melanie, Hutchison, Taylor A., Kartaltepe, Jeyhan S., Kassin, Susan A., Kriek, Mariska, Labbé, Ivo, Maiolino, Roberto, Marques-Chaves, Rui, Maseda, Michael V., Mason, Charlotte, Matthee, Jorryt, McQuinn, Kristen B. W., Meynet, Georges, Naidu, Rohan P., Oesch, Pascal A., Pentericci, Laura, Pérez-González, Pablo G., Rigby, Jane R., Roberts-Borsani, Guido, Schaerer, Daniel, Shapley, Alice E., Stark, Daniel P., Stiavelli, Massimo, Strom, Allison L., Vanzella, Eros, Wang, Feige, Wilkins, Stephen M., Williams, Christina C., Willott, Chris J., Wylezalek, Dominika, Nota, Antonella
With stunning clarity, JWST has revealed the Universe's first billion years. The scientific community is analyzing a wealth of JWST imaging and spectroscopic data from that era, and is in the process of rewriting the astronomy textbooks. Here, 1.5 ye
Externí odkaz:
http://arxiv.org/abs/2405.21054
Autor:
Scholtz, Jan, D'Eugenio, Francesco, Maiolino, Roberto, Pérez-González, Pablo G., Circosta, Chiara, Tacchella, Sandro, Williams, Christina C., Alberts, Stacey, Arribas, Santiago, Baker, William M., Bertola, Elena, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Cresci, Giovanni, Jones, Gareth C., Kumari, Nimisha, Lamperti, Isabella, Looser, Tobias J., Del Pino, Bruno Rodríguez, Robertson, Brant, Parlanti, Eleonora, Perna, Michele, Übler, Hannah, Venturi, Giacomo, Witstok, Joris
JWST is discovering increasing numbers of quiescent galaxies 1--2 billion years after the Big Bang, whose redshift, high mass, and old stellar ages indicate that their formation and quenching were surprisingly rapid. This fast-paced evolution seems t
Externí odkaz:
http://arxiv.org/abs/2405.19401
Autor:
Carniani, Stefano, Hainline, Kevin, D'Eugenio, Francesco, Eisenstein, Daniel J., Jakobsen, Peter, Witstok, Joris, Johnson, Benjamin D., Chevallard, Jacopo, Maiolino, Roberto, Helton, Jakob M., Willott, Chris, Robertson, Brant, Alberts, Stacey, Arribas, Santiago, Baker, William M., Bhatawdekar, Rachana, Boyett, Kristan, Bunker, Andrew J., Cameron, Alex J., Cargile, Phillip A., Charlot, Stéphane, Curti, Mirko, Curtis-Lake, Emma, Egami, Eiichi, Giardino, Giovanna, Isaak, Kate, Ji, Zhiyuan, Jones, Gareth C., Maseda, Michael V., Parlanti, Eleonora, Rawle, Tim, Rieke, George, Rieke, Marcia, Del Pino, Bruno Rodríguez, Saxena, Aayush, Scholtz, Jan, Smit, Renske, Sun, Fengwu, Tacchella, Sandro, Übler, Hannah, Venturi, Giacomo, Williams, Christina C., Willmer, Christopher N. A.
The discovery by JWST of an abundance of luminous galaxies in the very early Universe suggests that galaxies developed rapidly, in apparent tension with many standard models. However, most of these galaxies lack spectroscopic confirmation, so their d
Externí odkaz:
http://arxiv.org/abs/2405.18485
Autor:
Helton, Jakob M., Rieke, George H., Alberts, Stacey, Wu, Zihao, Eisenstein, Daniel J., Hainline, Kevin N., Carniani, Stefano, Ji, Zhiyuan, Baker, William M., Bhatawdekar, Rachana, Bunker, Andrew J., Cargile, Phillip A., Charlot, Stéphane, Chevallard, Jacopo, D'Eugenio, Francesco, Egami, Eiichi, Johnson, Benjamin D., Jones, Gareth C., Lyu, Jianwei, Maiolino, Roberto, Pérez-González, Pablo G., Rieke, Marcia J., Robertson, Brant, Saxena, Aayush, Scholtz, Jan, Shivaei, Irene, Sun, Fengwu, Tacchella, Sandro, Whitler, Lily, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris, Witstok, Joris, Zhu, Yongda
The James Webb Space Telescope (JWST) has spectroscopically confirmed numerous galaxies at $z > 10$. While weak rest-ultraviolet emission lines have only been seen in a handful of sources, the stronger rest-optical emission lines are highly diagnosti
Externí odkaz:
http://arxiv.org/abs/2405.18462
Autor:
Alberts, Stacey, Lyu, Jianwei, Shivaei, Irene, Rieke, George H., Perez-Gonzalez, Pablo G., Bonventura, Nina, Zhu, Yongda, Helton, Jakob M., Ji, Zhiyuan, Morrison, Jane, Robertson, Brant E., Stone, Meredith A., Sun, Yang, Williams, Christina C., Willmer, Christopher N. A.
The James Webb Space Telescope (JWST) is revolutionizing our view of the Universe through unprecedented sensitivity and resolution in the infrared, with some of the largest gains realized at its longest wavelengths. We present the Systematic Mid-infr
Externí odkaz:
http://arxiv.org/abs/2405.15972
Autor:
Ji, Xihan, Maiolino, Roberto, Ferland, Gary, D'Eugenio, Francesco, Bhatawdekar, Rachana, Charlot, Stéphane, Chevallard, Jacopo, Curti, Mirko, Curtis-Lake, Emma, Hainline, Kevin, Ji, Zhiyuan, Robertson, Brant, Del Pino, Bruno Rodríguez, Scholtz, Jan, Tacchella, Sandro, Williams, Christina C., Witstok, Joris
We report the detection of continuum excess in the rest-frame UV between 3000 {\AA} and 3550 {\AA} in the JWST/NIRSpec spectrum of GN-z11, a galaxy hosting an active galactic nucleus (AGN) at z = 10.603. The shape of the continuum excess resembles a
Externí odkaz:
http://arxiv.org/abs/2405.05772