Zobrazeno 1 - 10
of 3 520
pro vyhledávání: '"Baker, P. M."'
Autor:
Rinaldi, P., Bonaventura, N., Rieke, G. H., Alberts, S., Caputi, K. I., Baker, W. M., Baum, S., Bhatawdekar, R., Bunker, A. J., Carniani, S., Curtis-Lake, E., D'Eugenio, F., Egami, E., Ji, Z., Hainline, K., Helton, J. M., Lin, X., Lyu, J., Johnson, B. D., Ma, Z., Maiolino, R., Pérez-González, P. G., Rieke, M., Robertson, B. E., Shivaei, I., Stone, M., Sun, Y., Tacchella, S., Übler, H., Williams, C. C., Willmer, C. N. A., Willott, C., Zhang, J., Zhu, Y.
We analyze 99 photometrically selected Little Red Dots (LRDs) at z ~ 4-8 in the GOODS fields, leveraging ultra-deep JADES NIRCam short-wavelength (SW) data. We examine the morphology of 30 LRDs; the remaining 69 are predominantly compact, i.e. are st
Externí odkaz:
http://arxiv.org/abs/2411.14383
Autor:
Baker, William M., Lim, Seunghwan, D'Eugenio, Francesco, Maiolino, Roberto, Ji, Zhiyuan, Arribas, Santiago, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, de Graaff, Anna, Hainline, Kevin, Looser, Tobias J., Lyu, Jianwei, Rinaldi, Pierluigi, Robertson, Brant, Schaller, Matthieu, Schaye, Joop, Scholtz, Jan, Ubler, Hannah, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris, Zhu, Yongda
We use NIRSpec/MSA spectroscopy and NIRCam imaging to study a sample of 18 massive ($\log\; M_{*}/M_{\odot} \gt 10\;$dex), central quiescent galaxies at $2\leq z \leq 5$ in the GOODS fields, to investigate their number density, star-formation histori
Externí odkaz:
http://arxiv.org/abs/2410.14773
Autor:
Simmonds, C., Tacchella, S., Hainline, K., Johnson, B. D., Puskás, D., Robertson, B., Baker, W. M., Bhatawdekar, R., Boyett, K., Bunker, A. J., Cargile, P. A., Carniani, S., Chevallard, J., Curti, M., Curtis-Lake, E., Ji, Z., Jones, G. C., Kumari, N., Laseter, I., Maiolino, R., Maseda, M. V., Rinaldi, P., Stoffers, A., Übler, H., Villanueva, N. C., Williams, C. C., Willot, C., Witstok, J., Zhu, Y.
We use NIRCam imaging from the JWST Advanced Deep Extragalactic Survey (JADES) to study the ionising properties of a sample of 15721 galaxies at $3 \leq z_{\rm{phot}} \leq 9$, 90\% complete in stellar mass down to log(M$_{\star}$/[M$_{\odot}$])$\appr
Externí odkaz:
http://arxiv.org/abs/2409.01286
Autor:
Witstok, Joris, Jakobsen, Peter, Maiolino, Roberto, Helton, Jakob M., Johnson, Benjamin D., Robertson, Brant E., Tacchella, Sandro, Cameron, Alex J., Smit, Renske, Bunker, Andrew J., Saxena, Aayush, Sun, Fengwu, Alberts, Stacey, Arribas, Santiago, Baker, William M., Bhatawdekar, Rachana, Boyett, Kristan, Cargile, Phillip A., Carniani, Stefano, Charlot, Stéphane, Chevallard, Jacopo, Curti, Mirko, Curtis-Lake, Emma, D'Eugenio, Francesco, Eisenstein, Daniel J., Hainline, Kevin N., Jones, Gareth C., Kumari, Nimisha, Maseda, Michael V., Pérez-González, Pablo G., Rinaldi, Pierluigi, Scholtz, Jan, Übler, Hannah, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris, Zhu, Yongda
$\require{mediawiki-texvc}$Cosmic Reionisation commenced when ultraviolet (UV) radiation produced in the first galaxies began illuminating the cold, neutral gas that filled the primordial Universe. Recent James Webb Space Telescope (JWST) observation
Externí odkaz:
http://arxiv.org/abs/2408.16608
Autor:
Sethi, Sayam, Baker, Jonathan M.
Quantum error correction (QEC) is necessary to run large scale quantum programs. Regardless of error correcting code, hardware platform, or systems architecture, QEC systems are limited by the types of gates which they can perform efficiently. In ord
Externí odkaz:
http://arxiv.org/abs/2408.14708
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:
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:
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., Kumari, Nimisha, Maseda, Michael V., Parlanti, Eleonora, Pérez-González, Pablo G., 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.
Publikováno v:
Nature 633 (2024), 318-322
The first observations of JWST have revolutionized our understanding of the Universe by identifying for the first time galaxies at $z\sim13$. In addition, the discovery of many luminous galaxies at Cosmic Dawn ($z>10$) has suggested that galaxies dev
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