Zobrazeno 1 - 10
of 31 782
pro vyhledávání: '"An Brant"'
Autor:
Saxena, Aayush, Cameron, Alex J., Katz, Harley, Bunker, Andrew J., Chevallard, Jacopo, D'Eugenio, Francesco, Arribas, Santiago, Bhatawdekar, Rachana, Boyett, Kristan, Cargile, Phillip A., Carniani, Stefano, Charlot, Stephane, Curti, Mirko, Curtis-Lake, Emma, Hainline, Kevin, Ji, Zhiyuan, Johnson, Benjamin D., Jones, Gareth C., Kumari, Nimisha, Laseter, Isaac, Maseda, Michael V., Robertson, Brant, Simmonds, Charlotte, Tacchella, Sandro, Ubler, Hannah, Williams, Christina C., Willott, Chris, Witstok, Joris, Zhu, Yongda
The UV continuum slope of galaxies, $\beta$, is a powerful diagnostic. Understanding the redshift evolution of $\beta$ and its dependence on key galaxy properties can shed light on the evolution of galaxy physical properties over cosmic time. In this
Externí odkaz:
http://arxiv.org/abs/2411.14532
Autor:
Pinto, Felipe, Heitzer, Ricardo C, Dvorquez, Eitan, Rodriguez, Roberto, Sun, Qiang, Greentree, Andrew D, Gibson, Brant C, Maze, Jeronimo R
Quantum spin Hall (QSH) insulators are materials with nontrivial topological properties, characterized by helical edge currents. In 2D strips, the application of a bias voltage along the edge generates a magnetization that can be measured using quant
Externí odkaz:
http://arxiv.org/abs/2411.11701
Autor:
Sun, Qiang, Dvorquez, Eitan, Pinto, Felipe, Mathpal, Mohan C., Maze, Jerónimo R., Gibson, Brant C., Greentree, Andrew D.
Topological insulators (TIs) are materials with unique surface conductive properties that distinguish them from normal insulators and have attracted significant interest due to their potential applications in electronics and spintronics. However, the
Externí odkaz:
http://arxiv.org/abs/2411.09103
Autor:
Mehta, Vihang, Rafelski, Marc, Sunnquist, Ben, Teplitz, Harry I., Scarlata, Claudia, Wang, Xin, Fontana, Adriano, Hathi, Nimish P., Iyer, Kartheik G., Alavi, Anahita, Colbert, James, Grogin, Norman, Koekemoer, Anton, Nedkova, Kalina V., Hayes, Matthew, Prichard, Laura, Siana, Brian, Smith, Brent M., Windhorst, Rogier, Ashcraft, Teresa, Bagley, Micaela, Baronchelli, Ivano, Barro, Guillermo, Blanche, Alex, Broussard, Adam, Carleton, Timothy, Chartab, Nima, Codoreanu, Alex, Cohen, Seth, Conselice, Christopher, Dai, Y. Sophia, Darvish, Behnam, Dave, Romeel, DeGroot, Laura, De Mello, Duilia, Dickinson, Mark, Emami, Najmeh, Ferguson, Henry, Ferreira, Leonardo, Finkelstein, Keely, Finkelstein, Steven, Gardner, Jonathan P., Gawiser, Eric, Gburek, Timothy, Giavalisco, Mauro, Grazian, Andrea, Gronwall, Caryl, Guo, Yicheng, Haro, Pablo Arrabal, Hemmati, Shoubaneh, Howell, Justin, Jansen, Rolf A., Ji, Zhiyuan, Kaviraj, Sugata, Kim, Keunho J., Kurczynski, Peter, Lazar, Ilin, Lucas, Ray A., MacKenty, John, Mantha, Kameswara Bharadwaj, Martin, Alec, Martin, Garreth, McCabe, Tyler, Mobasher, Bahram, Morales, Alexa M., O'Connell, Robert, Olsen, Charlotte, Otteson, Lillian, Ravindranath, Swara, Redshaw, Caleb, Rutkowski, Michael, Robertson, Brant, Sattari, Zahra, Soto, Emmaris, Sun, Lei, Taamoli, Sina, Vanzella, Eros, Yung, L. Y. Aaron, Zabelle, Bonnabelle
The UltraViolet imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey Fields (UVCANDELS) program provides deep HST F275W and F435W imaging over four CANDELS fields (GOODS-N, GOODS-S, COSMOS, and EGS). We combine this newly acq
Externí odkaz:
http://arxiv.org/abs/2410.16404
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
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