Zobrazeno 1 - 10
of 314
pro vyhledávání: '"Williams, Christina C."'
Autor:
Price, Sedona H., Bezanson, Rachel, Labbe, Ivo, Furtak, Lukas J., de Graaff, Anna, Greene, Jenny E., Kokorev, Vasily, Setton, David J., Suess, Katherine A., Brammer, Gabriel, Cutler, Sam E., Leja, Joel, Pan, Richard, Wang, Bingjie, Weaver, John R., Whitaker, Katherine E., Atek, Hakim, Burgasser, Adam J., Chemerynska, Iryna, Dayal, Pratika, Feldmann, Robert, Schreiber, Natascha M. Förster, Fudamoto, Yoshinobu, Fujimoto, Seiji, Glazebrook, Karl, Goulding, Andy D., Khullar, Gourav, Kriek, Mariska, Marchesini, Danilo, Maseda, Michael V., Miller, Tim B., Muzzin, Adam, Nanayakkara, Themiya, Nelson, Erica, Oesch, Pascal A., Shipley, Heath, Smit, Renske, Taylor, Edward N., van Dokkum, Pieter, Williams, Christina C., Zitrin, Adi
We present the design and observations of low resolution JWST/NIRSpec PRISM spectroscopy from the Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization (UNCOVER) Cycle 1 JWST Treasury program. Targets are selected using JWST/NIRC
Externí odkaz:
http://arxiv.org/abs/2408.03920
Autor:
Gibson, Justus L., Nelson, Erica, Williams, Christina C., Price, Sedona H., Whitaker, Katherine E., Suess, Katherine A., de Graaff, Anna, Johnson, Benjamin D., Bunker, Andrew J., Baker, William M., Bhatawdekar, Rachana, Boyett, Kristan, Charlot, Stephane, Curtis-Lake, Emma, Eisenstein, Daniel J., Hainline, Kevin, Hausen, Ryan, Maiolino, Roberto, Rieke, George, Rieke, Marcia, Robertson, Brant, Tacchella, Sandro, Willott, Chris
One of the more surprising findings after the first year of JWST observations is the large number of spatially extended galaxies (ultra-red flattened objects, or UFOs) among the optically-faint galaxy population otherwise thought to be compact. Lever
Externí odkaz:
http://arxiv.org/abs/2408.02726
Autor:
Hainline, Kevin N., D'Eugenio, Francesco, Sun, Fengwu, Helton, Jakob M., Miles, Brittany E., Marley, MArk S., Lew, Ben W. P., Leisenring, Jarron M., Bunker, Andrew J., Cargile, Phillip A., Carniani, Stefano, Eisenstein, Daniel J., Juodzbalis, Ignas, Johnson, Benjamin D., Robertson, Brant, Tacchella, Sandro, Williams, Christina C., Willmer, Christopher N. A.
Large area observations of extragalactic deep fields with the James Webb Space Telescope (JWST) have provided a wealth of candidate low-mass L- and T-class brown dwarfs. The existence of these sources, which are at derived distances of hundreds of pa
Externí odkaz:
http://arxiv.org/abs/2407.08781
Autor:
Juodžbalis, Ignas, Ji, Xihan, Maiolino, Roberto, D'Eugenio, Francesco, Scholtz, Jan, Risaliti, Guido, Fabian, Andrew C., Mazzolari, Giovanni, Gilli, Roberto, Prandoni, Isabella, Arribas, Santiago, Bunker, Andrew J., Carniani, Stefano, Charlot, Stéphane, Curtis-Lake, Emma, de Graaff, Anna, Hainline, Kevin, Parlanti, Eleonora, Perna, Michele, Pérez-González, Pablo G., Robertson, Brant, Tacchella, Sandro, Übler, Hannah, Williams, Christina C., Willott, Chris, Witstok, Joris
JWST has discovered a large population of Active Galactic Nuclei (AGN) at high redshift. Many of these newly discovered AGN have broad permitted lines (typically H$\alpha$), but are extremely weak in the X-rays. Here we present the NIRSpec spectrum o
Externí odkaz:
http://arxiv.org/abs/2407.08643
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-/mid-infrared images to date (down to $\sim$30 ABmag) over $\sim$25 arcmin$^2$ in the GOODS-S field in two sets of observations wi
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