Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Jakobsen, Peter"'
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:
Saxena, Aayush, Robertson, Brant E., Bunker, Andrew J., Endsley, Ryan, Cameron, Alex J., Charlot, Stephane, Simmonds, Charlotte, Tacchella, Sandro, Witstok, Joris, Willott, Chris, Carniani, Stefano, Curtis-Lake, Emma, Ferruit, Pierre, Jakobsen, Peter, Arribas, Santiago, Chevallard, Jacopo, Curti, Mirko, D'Eugenio, Francesco, De Graaff, Anna, Jones, Gareth C., Looser, Tobias J., Maseda, Michael V., Rawle, Tim, Rix, Hans-Walter, Del Pino, Bruno Rodríguez, Smit, Renske, Übler, Hannah, Eisenstein, Daniel J., Hainline, Kevin, Hausen, Ryan, Johnson, Benjamin D., Rieke, Marcia, Williams, Christina C., Willmer, Christopher N. A., Baker, William M., Bhatawdekar, Rachana, Bowler, Rebecca, Boyett, Kristan, Chen, Zuyi, Egami, Eiichi, Ji, Zhiyuan, Nelson, Erica, Perna, Michele, Sandles, Lester, Scholtz, Jan, Shivaei, Irene
Publikováno v:
A&A 678, A68 (2023)
We report the discovery of a remarkable Ly$\alpha$ emitting galaxy at z = 7.2782, JADES-GS-z7-LA, with EW$_0$(Ly$\alpha$) $= 388.0 \pm 88.8$\AA and UV magnitude -17.0. The spectroscopic redshift is confirmed via rest-frame optical lines [O II], H$\be
Externí odkaz:
http://arxiv.org/abs/2302.12805
Autor:
Bunker, Andrew J., Saxena, Aayush, Cameron, Alex J., Willott, Chris J., Curtis-Lake, Emma, Jakobsen, Peter, Carniani, Stefano, Smit, Renske, Maiolino, Roberto, Witstok, Joris, Curti, Mirko, D'Eugenio, Francesco, Jones, Gareth C., Ferruit, Pierre, Arribas, Santiago, Charlot, Stephane, Chevallard, Jacopo, Giardino, Giovanna, de Graaff, Anna, Looser, Tobias J., Luetzgendorf, Nora, Maseda, Michael V., Rawle, Tim, Rix, Hans-Walter, Del Pino, Bruno Rodriguez, Alberts, Stacey, Egami, Eiichi, Eisenstein, Daniel J., Endsley, Ryan, Hainline, Kevin, Hausen, Ryan, Johnson, Benjamin D., Rieke, George, Rieke, Marcia, Robertson, Brant E., Shivaei, Irene, Stark, Daniel P., Sun, Fengwu, Tacchella, Sandro, Tang, Mengtao, Williams, Christina C., Willmer, Christopher N. A., Baker, William M., Baum, Stefi, Bhatawdekar, Rachana, Bowler, Rebecca, Boyett, Kristan, Chen, Zuyi, Circosta, Chiara, Helton, Jakob M., Ji, Zhiyuan, Lyu, Jianwei, Nelson, Erica, Parlanti, Eleonora, Perna, Michele, Sandles, Lester, Scholtz, Jan, Suess, Katherine A., Topping, Michael W., Uebler, Hannah, Wallace, Imaan E. B., Whitler, Lily
Publikováno v:
A&A 677, A88 (2023)
We present JADES JWST/NIRSpec spectroscopy of GN-z11, the most luminous candidate $z>10$ Lyman break galaxy in the GOODS-North field with $M_{UV}=-21.5$. We derive a redshift of $z=10.603$ (lower than previous determinations) based on multiple emissi
Externí odkaz:
http://arxiv.org/abs/2302.07256