Zobrazeno 1 - 10
of 191
pro vyhledávání: '"Rieke, Marcia J."'
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:
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:
Lawson, Kellen, Schlieder, Joshua E., Leisenring, Jarron M., Bogat, Ell, Beichman, Charles A., Bryden, Geoffrey, Gáspár, András, Groff, Tyler D., McElwain, Michael W., Meyer, Michael R., Barclay, Thomas, Calissendorff, Per, De Furio, Matthew, Li, Yiting, Rieke, Marcia J., Ygouf, Marie, Greene, Thomas P., Girard, Julien H., Gennaro, Mario, Kammerer, Jens, Rest, Armin, Roellig, Thomas L., Sunnquist, Ben
Observations of debris disks offer important insights into the formation and evolution of planetary systems. Though M dwarfs make up approximately 80% of nearby stars, very few M-dwarf debris disks have been studied in detail -- making it unclear how
Externí odkaz:
http://arxiv.org/abs/2405.00573
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:
Hodapp, Klaus W., Chu, Laurie L., Greene, Thomas, Meyer, Michael R., Johnstone, Doug, Rieke, Marcia J., Stansberry, John, Boyer, Martha, Beichman, Charles, Horner, Scott, Roellig, Tom, Rieke, George, Young, Eric T.
The isolated globule B335 contains a single, low luminosity Class 0 protostar associated with a bipolar nebula and outflow system seen nearly perpendicular to its axis. We observed the innermost regions of this outflow as part of JWST/NIRCam GTO prog
Externí odkaz:
http://arxiv.org/abs/2401.02881
Autor:
Alberts, Stacey, Williams, Christina C., Helton, Jakob M., Suess, Katherine A., Ji, Zhiyuan, Shivaei, Irene, Lyu, Jianwei, Rieke, George, Baker, William M., Bonaventura, Nina, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Curtis-Lake, Emma, D'Eugenio, Francesco, Eisenstein, Daniel J., de Graaff, Anna, Hainline, Kevin N., Hausen, Ryan, Johnson, Benjamin D., Maiolino, Roberto, Parlanti, Eleonora, Rieke, Marcia J., Robertson, Brant E., Sun, Yang, Tacchella, Sandro, Willmer, Christopher N. A., Willott, Chris J.
We present the robust selection of quiescent (QG) and post-starburst (PSB) galaxies using ultra-deep NIRCam and MIRI imaging from the JWST Advanced Deep Extragalactic Survey (JADES). Key to this is MIRI 7.7$\mu$m imaging which breaks the degeneracy b
Externí odkaz:
http://arxiv.org/abs/2312.12207
Autor:
Williams, Christina C., Alberts, Stacey, Ji, Zhiyuan, Hainline, Kevin N., Lyu, Jianwei, Rieke, George, Endsley, Ryan, Suess, Katherine A., Johnson, Benjamin D., Florian, Michael, Shivaei, Irene, Rujopakarn, Wiphu, Baker, William M., Bhatawdekar, Rachana, Boyett, Kristan, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Curtis-Lake, Emma, DeCoursey, Christa, de Graaff, Anna, Egami, Eiichi, Eisenstein, Daniel J., Gibson, Justus L., Hausen, Ryan, Helton, Jakob M., Maiolino, Roberto, Maseda, Michael V., Nelson, Erica J., Perez-Gonzalez, Pablo G., Rieke, Marcia J., Robertson, Brant E., Sun, Fengwu, Tacchella, Sandro, Willmer, Christopher N. A., Willott, Chris J.
Using deep JWST imaging from JADES, JEMS and SMILES, we characterize optically-faint and extremely red galaxies at $z>3$ that were previously missing from galaxy census estimates. The data indicate the existence of abundant, dusty and post-starburst-
Externí odkaz:
http://arxiv.org/abs/2311.07483
Autor:
Helton, Jakob M., Sun, Fengwu, Woodrum, Charity, Hainline, Kevin N., Willmer, Christopher N. A., Rieke, Marcia J., Rieke, George H., Alberts, Stacey, Eisenstein, Daniel J., Tacchella, Sandro, Robertson, Brant, Johnson, Benjamin D., Baker, William M., Bhatawdekar, Rachana, Bunker, Andrew J., Chen, Zuyi, Egami, Eiichi, Ji, Zhiyuan, Maiolino, Roberto, Willott, Chris, Witstok, Joris
We conduct a systematic search for high-redshift galaxy overdensities at $4.9 < z_{\,\mathrm{spec}} < 8.9$ in both the GOODS-N and GOODS-S fields using JWST/NIRCam imaging from JADES and JEMS in addition to JWST/NIRCam wide field slitless spectroscop
Externí odkaz:
http://arxiv.org/abs/2311.04270
Autor:
Sun, Fengwu, Helton, Jakob M., Egami, Eiichi, Hainline, Kevin N., Rieke, George H., Willmer, Christopher N. A., Eisenstein, Daniel J., Johnson, Benjamin D., Rieke, Marcia J., Robertson, Brant, Tacchella, Sandro, Alberts, Stacey, Baker, William M., Bhatawdekar, Rachana, Boyett, Kristan, Bunker, Andrew J., Charlot, Stephane, Chen, Zuyi, Chevallard, Jacopo, Curtis-Lake, Emma, Danhaive, A. Lola, DeCoursey, Christa, Ji, Zhiyuan, Lyu, Jianwei, Maiolino, Roberto, Rujopakarn, Wiphu, Sandles, Lester, Shivaei, Irene, Ubler, Hannah, Willott, Chris, Witstok, Joris
HDF850.1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at $z = 5.18$. With nine-band NIRCam images at 0.8-5.0 $\mu$m obtained thro
Externí odkaz:
http://arxiv.org/abs/2309.04529
Autor:
Bell, Taylor J., Welbanks, Luis, Schlawin, Everett, Line, Michael R., Fortney, Jonathan J., Greene, Thomas P., Ohno, Kazumasa, Parmentier, Vivien, Rauscher, Emily, Beatty, Thomas G., Mukherjee, Sagnick, Wiser, Lindsey S., Boyer, Martha L., Rieke, Marcia J., Stansberry, John A.
The abundances of major carbon and oxygen bearing gases in the atmospheres of giant exoplanets provide insights into atmospheric chemistry and planet formation processes. Thermochemistry suggests that methane should be the dominant carbon-bearing spe
Externí odkaz:
http://arxiv.org/abs/2309.04042