Zobrazeno 1 - 10
of 32 150
pro vyhledávání: '"Brant, A."'
We propose a generalisation of the logistic regression model, that aims to account for non-linear main effects and complex interactions, while keeping the model inherently explainable. This is obtained by starting with log-odds that are linear in the
Externí odkaz:
http://arxiv.org/abs/2410.08803
Autor:
Robertson, Islay O., Johnson, Brett C., Thalassinos, Giannis, Scholten, Sam C., Rietwyk, Kevin J., Gibson, Brant, Tetienne, Jean-Philippe, Broadway, David A.
Optically addressable solid-state spins have been proposed as robust radiofrequency (RF)-optical transducers sensitive to a specific RF frequency tuned by an external static magnetic field, but often require precise field alignment with the system's
Externí odkaz:
http://arxiv.org/abs/2410.00430
Autor:
Akins, Hollis B., Casey, Caitlin M., Berg, Danielle A., Chisholm, John, Franco, Maximilien, Finkelstein, Steven L., Fujimoto, Seiji, Kokorev, Vasily, Lambrides, Erini, Robertson, Brant E., Taylor, Anthony J., Coulter, David A., Fox, Ori, Karmen, Mitchell
JWST has now revealed a population of broad-line AGN at $z>4$ characterized by a distinctive SED shape, with very red rest-frame optical and very blue rest-frame UV continuum. While the optical continuum is thought to originate from the accretion dis
Externí odkaz:
http://arxiv.org/abs/2410.00949
Autor:
Tanaka, Takumi S., Silverman, John D., Nakazato, Yurina, Onoue, Masafusa, Shimasaku, Kazuhiro, Fudamoto, Yoshinobu, Fujimoto, Seiji, Ding, Xuheng, Faisst, Andreas L., Valentino, Francesco, Jin, Shuowen, Hayward, Christopher C., Kokorev, Vasily, Ceverino, Daniel, Kalita, Boris S., Casey, Caitlin M., Liu, Zhaoxuan, Kaminsky, Aidan, Fei, Qinyue, Andika, Irham T., Lambrides, Erini, Akins, Hollis B., Kartaltepe, Jeyhan S., Koekemoer, Anton M., McCracken, Henry Joy, Rhodes, Jason, Robertson, Brant E., Franco, Maximilien, Liu, Daizhong, Chartab, Nima, Gillman, Steven, Gozaliasl, Ghassem, Hirschmann, Michaela, Huertas-Company, Marc, Massey, Richard, Roy, Namrata, Sattari, Zahra, Shuntov, Marko, Sterling, Joseph, Toft, Sune, Trakhtenbrot, Benny, Yoshida, Naoki, Zavala, Jorge A.
The current paradigm for the co-evolution of galaxies and their supermassive black holes postulates that dust-obscured active galactic nuclei (AGNs) represent a transitional phase towards a more luminous and unobscured state. However, our understandi
Externí odkaz:
http://arxiv.org/abs/2410.00104
Autor:
Hainline, Kevin N., Maiolino, Roberto, Juodzbalis, Ignas, Scholtz, Jan, Ubler, Hannah, D'Eugenio, Francesco, Helton, Jakob M., Sun, Yang, Sun, Fengwu, Robertson, Brant, Tacchella, Sandro, Bunker, Andrew J., Carniani, Stefano, Charlot, Stephane, Curtis-Lake, Emma, Egami, Eiichi, Johnson, Benjamin D., Lin, Xiaojing, Lyu, Jianwei, Perez-Gonzalez, Pablo G., Rinaldi, Pierluigi, Silcock, Maddie S., Williams, Christina C., Willmer, Christopher N. A., Willott, Chris, Zhang, Junyu, Zhu, Yongda
Recently, a large number of compact sources at $z > 4$ with blue UV slopes and extremely red rest-frame optical slopes have been found in James Webb Space Telescope (JWST) extragalactic surveys. As a subsample of these sources, commonly called ``litt
Externí odkaz:
http://arxiv.org/abs/2410.00100
Autor:
Carniani, Stefano, D'Eugenio, Francesco, Ji, Xihan, Parlanti, Eleonora, Scholtz, Jan, Sun, Fengwu, Venturi, Giacomo, Bakx, Tom J. L. C., Curti, Mirko, Maiolino, Roberto, Tacchella, Sandro, Zavala, Jorge A., Hainline, Kevin, Witstok, Joris, Johnson, Benjamin D., Alberts, Stacey, Bunker, Andrew J., Charlot, Stéphane, Eisenstein, Daniel J., Helton, Jakob M., Jakobsen, Peter, Kumari, Nimisha, Robertson, Brant, Saxena, Aayush, Übler, Hannah, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris
JADES-GS-z14-0 is the most distant spectroscopically confirmed galaxy so far, at $z>14$. With a UV magnitude of -20.81, it is one of the most luminous galaxies at cosmic dawn and its half-light radius of 260 pc means that stars dominate the observed
Externí odkaz:
http://arxiv.org/abs/2409.20533
Autor:
Ji, Zhiyuan, Williams, Christina C., Rieke, George H., Lyu, Jianwei, Alberts, Stacey, Sun, Fengwu, Helton, Jakob M., Rieke, Marcia, Shivaei, Irene, D'Eugenio, Francesco, Tacchella, Sandro, Robertson, Brant, Zhu, Yongda, Maiolino, Roberto, Bunker, Andrew J., Sun, Yang, Willmer, Christopher N. A.
A major unsolved problem in galaxy evolution is the early appearance of massive quiescent galaxies that no longer actively form stars only $ \sim 1$ billion years after the Big Bang. Their high stellar masses and extremely compact structure indicate
Externí odkaz:
http://arxiv.org/abs/2409.17233
Autor:
Zhu, Yongda, Rieke, Marcia J., Ji, Zhiyuan, Simmonds, Charlotte, Sun, Fengwu, Sun, Yang, Alberts, Stacey, Bhatawdekar, Rachana, Bunker, Andrew J., Cargile, Phillip A., Carniani, Stefano, de Graaff, Anna, Hainline, Kevin, Helton, Jakob M., Jones, Gareth C., Lyu, Jianwei, Rieke, George H., Rinaldi, Pierluigi, Robertson, Brant, Scholtz, Jan, Übler, Hannah, Williams, Christina C., Willmer, Christopher N. A.
For the first time, we systematically search for galaxies with extended emission line and potential outflows features using medium-band images in the GOODS-S field by comparing the morphology in medium-band images to adjacent continuum and UV bands.
Externí odkaz:
http://arxiv.org/abs/2409.11464
Autor:
Sun, Yang, Lyu, Jianwei, Rieke, George H., Ji, Zhiyuan, Sun, Fengwu, Zhu, Yongda, Bunker, Andrew J., Cargile, Phillip A., Circosta, Chiara, D'Eugenio, Francesco, Egami, Eiichi, Hainline, Kevin, Helton, Jakob M., Rinaldi, Pierluigi, Robertson, Brant E., Scholtz, Jan, Shivaei, Irene, Stone, Meredith A., Tacchella, Sandro, Williams, Christina C., Willmer, Christopher N. A., Willott, Chris
Over the past two decades, tight correlations between black hole masses ($M_\bullet$) and their host galaxy properties have been firmly established at low-$z$ ($z<1$), indicating coevolution of supermassive black holes and galaxies. However, the situ
Externí odkaz:
http://arxiv.org/abs/2409.06796
Autor:
Jones, Gareth C., Bunker, Andrew J., Saxena, Aayush, Arribas, Santiago, Bhatawdekar, Rachana, Boyett, Kristan, Carniani, Stefano, Charlot, Stephane, Curtis-Lake, Emma, Hainline, Kevin, Johnson, Benjamin D., Kumari, Nimisha, Maseda, Michael V., Rix, Hans-Walter, Robertson, Brant E., Tacchella, Sandro, Übler, Hannah, Williams, Christina C., Willott, Chris, Witstok, Joris, Zhu, Yongda
Ly$\alpha$ is the transition to the ground state from the first excited state of hydrogen (the most common element). Resonant scattering of this line by neutral hydrogen greatly impedes its emergence from galaxies, so the fraction of galaxies which s
Externí odkaz:
http://arxiv.org/abs/2409.06405