Zobrazeno 1 - 10
of 4 706
pro vyhledávání: '"A Puskas"'
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:
Muthiah, Dinakar, Puskás, Anna
The Kac-Moody affine Hecke algebra $\mathcal{H}$ was first constructed as the Iwahori-Hecke algebra of a $p$-adic Kac-Moody group by work of Braverman, Kazhdan, and Patnaik, and by work of Bardy-Panse, Gaussent, and Rousseau. Since $\mathcal{H}$ has
Externí odkaz:
http://arxiv.org/abs/2406.14447
Autor:
D'Eugenio, Francesco, Cameron, Alex J., Scholtz, Jan, Carniani, Stefano, Willott, Chris J., Curtis-Lake, Emma, Bunker, Andrew J., Parlanti, Eleonora, Maiolino, Roberto, Willmer, Christopher N. A., Jakobsen, Peter, Robertson, Brant E., Johnson, Benjamin D., Tacchella, Sandro, Cargile, Phillip A., Rawle, Tim, Arribas, Santiago, Chevallard, Jacopo, Curti, Mirko, Egami, Eiichi, Eisenstein, Daniel J., Kumari, Nimisha, Looser, Tobias J., Rieke, Marcia J., Del Pino, Bruno Rodríguez, Saxena, Aayush, Übler, Hannah, Venturi, Giacomo, Witstok, Joris, Baker, William M., Bhatawdekar, Rachana, Bonaventura, Nina, Boyett, Kristan, Charlot, Stéphane, Danhaive, A. Lola, Hainline, Kevin N., Hausen, Ryan, Helton, Jakob M., Ji, Xihan, Ji, Zhiyuan, Jones, Gareth C., Joudžbalis, Ignas, Maseda, Michael V., Pérez-González, Pablo G., Perna, Michele, Puskás, Dávid, Shivaei, Irene, Silcock, Maddie S., Simmonds, Charlotte, Smit, Renske, Sun, Fengwu, Villanueva, Natalia C., Williams, Christina C., Zhu, Yongda
We present the third data release of JADES, the JWST Advanced Deep Extragalactic Survey, providing both imaging and spectroscopy in the two GOODS fields. Spectroscopy consists of medium-depth and deep NIRSpec/MSA spectra of 4,000 targets, covering th
Externí odkaz:
http://arxiv.org/abs/2404.06531
Autor:
Tacchella, Sandro, McClymont, William, Scholtz, Jan, Maiolino, Roberto, Ji, Xihan, Villanueva, Natalia C., Charlot, Stéphane, D'Eugenio, Francesco, Helton, Jakob M., Williams, Christina C., Witstok, Joris, Bhatawdekar, Rachana, Carniani, Stefano, Chevallard, Jacopo, Curti, Mirko, Hainline, Kevin, Ji, Zhiyuan, Johnson, Benjamin D., Leja, Joel, Li, Yijia, Maseda, Michael V., Puskás, Dávid, Rieke, Marcia, Robertson, Brant, Shivaei, Irene, Silcock, Maddie S., Simmonds, Charlotte, Übler, Hannah, Willmer, Christopher N. A., Willott, Chris
Understanding the sources that power nebular emission in high-redshift galaxies is fundamentally important not only for shedding light onto the drivers of reionisation, but to constrain stellar populations and the growth of black holes. Here we focus
Externí odkaz:
http://arxiv.org/abs/2404.02194
Autor:
Pérez-González, Pablo G., Barro, Guillermo, Rieke, George H., Lyu, Jianwei, Rieke, Marcia, Alberts, Stacey, Williams, Christina, Hainline, Kevin, Sun, Fengwu, Puskas, David, Annunziatella, Marianna, Baker, William M., Bunker, Andrew J., Egami, Eiichi, Ji, Zhiyuan, Johnson, Benjamin D., Robertson, Brant, Del Pino, Bruno Rodriguez, Rujopakarn, Wiphu, Shivaei, Irene, Tacchella, Sandro, Willmer, Christopher N. A., Willott, Chris
We study little red dots (LRD) detected by JADES and covered by the SMILES MIRI survey. Our sample contains 31 sources, $\sim70$% detected in the two bluest MIRI bands, 40% in redder filters. The median/quartiles redshifts are $z=6.9_{5.9}^{7.7}$ (55
Externí odkaz:
http://arxiv.org/abs/2401.08782
Autor:
Robertson, Brant, Johnson, Benjamin D., Tacchella, Sandro, Eisenstein, Daniel J., Hainline, Kevin, Arribas, Santiago, Baker, William M., Bunker, Andrew J., Carniani, Stefano, Carreira, Courtney, Cargile, Phillip A., Charlot, Stéphane, Chevallard, Jacopo, Curti, Mirko, Curtis-Lake, Emma, D'Eugenio, Francesco, Egami, Eiichi, Hausen, Ryan, Helton, Jakob M., Jakobsen, Peter, Ji, Zhiyuan, Jones, Gareth C., Maiolino, Roberto, Maseda, Michael V., Nelson, Erica, Pérez-González, Pablo G., Puskás, Dávid, Rieke, Marcia, Smit, Renske, Sun, Fengwu, Übler, Hannah, Whitler, Lily, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris, Witstok, Joris
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters spanning $0.4-0.9\mu\mathrm{m}$) and novel JWST images with 1
Externí odkaz:
http://arxiv.org/abs/2312.10033
Autor:
Eisenstein, Daniel J., Johnson, Benjamin D., Robertson, Brant, Tacchella, Sandro, Hainline, Kevin, Jakobsen, Peter, Maiolino, Roberto, Bonaventura, Nina, Bunker, Andrew J., Cameron, Alex J., Cargile, Phillip A., Curtis-Lake, Emma, Hausen, Ryan, Puskás, Dávid, Rieke, Marcia, Sun, Fengwu, Willmer, Christopher N. A., Willott, Chris, Alberts, Stacey, Arribas, Santiago, Baker, William M., Baum, Stefi, Bhatawdekar, Rachana, Carniani, Stefano, Charlot, Stephane, Chen, Zuyi, Chevallard, Jacopo, Curti, Mirko, DeCoursey, Christa, D'Eugenio, Francesco, de Graaff, Anna, Egami, Eiichi, Helton, Jakob M., Ji, Zhiyuan, Jones, Gareth C., Kumari, Nimisha, Lützgendorf, Nora, Laseter, Isaac, Looser, Tobias J., Lyu, Jianwei, Maseda, Michael V., Nelson, Erica, Parlanti, Eleonora, Rauscher, Bernard J., Rawle, Tim, Rieke, George, Rix, Hans-Walter, Rujopakarn, Wiphu, Sandles, Lester, Saxena, Aayush, Scholtz, Jan, Sharpe, Katherine, Shivaei, Irene, Simmonds, Charlotte, Smit, Renske, Topping, Michael W., Übler, Hannah, Venturi, Giacomo, Williams, Christina C., Witstok, Joris, Woodrum, Charity
We summarize the properties and initial data release of the JADES Origins Field (JOF), which will soon be the deepest imaging field yet observed with the James Webb Space Telescope (JWST). This field falls within the GOODS-S region about 8' south-wes
Externí odkaz:
http://arxiv.org/abs/2310.12340
Publikováno v:
ACS Omega, Vol 9, Iss 37, Pp 38385-38395 (2024)
Externí odkaz:
https://doaj.org/article/916cd3c3a0f944ac9a01b353fbcd1b5d
A connected 1-factorisation is a 1-factorisation of a hypergraph for which the union of each pair of distinct 1-factors is a connected hypergraph. A uniform 1-factorisation is a 1-factorisation of a hypergraph for which the union of each pair of dist
Externí odkaz:
http://arxiv.org/abs/2307.13196
Autor:
Endsley, Ryan, Stark, Daniel P., Whitler, Lily, Topping, Michael W., Johnson, Benjamin D., Robertson, Brant, Tacchella, Sandro, Alberts, Stacey, Baker, William M., Bhatawdekar, Rachana, Boyett, Kristan, Bunker, Andrew J., Cameron, Alex J., Carniani, Stefano, Charlot, Stéphane, Chen, Zuyi, Chevallard, Jacopo, Curtis-Lake, Emma, Danhaive, A. Lola, Egami, Eiichi, Eisenstein, Daniel J., Hainline, Kevin, Helton, Jakob M., Ji, Zhiyuan, Looser, Tobias J., Maiolino, Roberto, Nelson, Erica, Puskás, Dávid, Rieke, George, Rieke, Marcia, Rix, Hans-Walter, Sandles, Lester, Saxena, Aayush, Simmonds, Charlotte, Smit, Renske, Sun, Fengwu, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris, Witstok, Joris
Reionization is thought to be driven by faint star-forming galaxies, but characterizing this population has long remained very challenging. Here we utilize deep nine-band NIRCam imaging from JADES to study the star-forming and ionizing properties of
Externí odkaz:
http://arxiv.org/abs/2306.05295