Zobrazeno 1 - 10
of 13 078
pro vyhledávání: '"A, Prichard"'
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:
Dutta, Rajeshwari, Fumagalli, Michele, Fossati, Matteo, Rafelski, Marc, Revalski, Mitchell, Battaia, Fabrizio Arrigoni, D'Odorico, Valentina, Peroux, Celine, Prichard, Laura J., Swinbank, A. M.
We characterize, for the first time, the average extended emission in multiple lines ([OII], [OIII], and Hbeta) around a statistical sample of 560 galaxies at z~0.25-0.85. By stacking the Multi Unit Spectroscopic Explorer (MUSE) 3D data from two larg
Externí odkaz:
http://arxiv.org/abs/2409.02182
Autor:
Morales, Alexa, Finkelstein, Steven, Bagley, Micaela, Alavi, Anahita, Grogin, Norman, Hathi, Nimish, Koekemoer, Anton, Nedkova, Kalina, Prichard, Laura, Rafelski, Marc, Sunnquist, Ben, Taamoli, Sina, Teplitz, Harry, Wang, Xin, Windhorst, Rogier, Yung, L. Y. Aaron
We present an analysis of rest-frame UV colors of 17,243 galaxies at $z\sim2-4$ in the HST UVCANDELS fields: GOODS-N, GOODS-S, COSMOS, and EGS. Here, we study the rest-frame UV spectral slope, $\beta$, measured via model spectra obtained via spectral
Externí odkaz:
http://arxiv.org/abs/2405.20901
Autor:
Nedkova, Kalina V., Rafelski, Marc, Teplitz, Harry I., Mehta, Vihang, DeGroot, Laura, Ravindranath, Swara, Alavi, Anahita, Beckett, Alexander, Grogin, Norman A., Häußler, Boris, Koekemoer, Anton M., Oyarzún, Grecco A., Prichard, Laura, Revalski, Mitchell, Snyder, Gregory F., Sunnquist, Ben, Wang, Xin, Windhorst, Rogier A., Chartab, Nima, Conselice, Christopher J., Guo, Yicheng, Hathi, Nimish, Hayes, Matthew J., Ji, Zhiyuan, Kim, Keunho J., Lucas, Ray A., Mobasher, Bahram, O'Connell, Robert W., Sattari, Zahra, Smith, Brent M., Taamoli, Sina, Yung, L. Y. Aaron, Team, the UVCANDELS
We use the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey fields (UVCANDELS) to measure half-light radii in the rest-frame far-UV for $\sim$16,000 disk-like galaxies over $0.5\leq z \leq 3$. We compare these
Externí odkaz:
http://arxiv.org/abs/2405.10908
Autor:
Revalski, Mitchell, Rafelski, Marc, Henry, Alaina, Fossati, Matteo, Fumagalli, Michele, Dutta, Rajeshwari, Pirzkal, Norbert, Beckett, Alexander, Battaia, Fabrizio Arrigoni, Dayal, Pratika, D'Odorico, Valentina, Lusso, Elisabeta, Nedkova, Kalina V., Prichard, Laura J., Papovich, Casey, Peroux, Celine
Using more than 100 galaxies in the MUSE Ultra Deep Field with spectroscopy from the Hubble Space Telescope's Wide Field Camera 3 and the Very Large Telescope's Multi Unit Spectroscopic Explorer, we extend the gas-phase mass-metallicity relation (MZR
Externí odkaz:
http://arxiv.org/abs/2403.17047
Autor:
Smith, Brent M., Windhorst, Rogier A., Teplitz, Harry, Hayes, Matthew, Rafelski, Marc, Dickinson, Mark, Mehta, Vihang, Hathi, Nimish P., MacKenty, John, Yung, L. Y. Aaron, Koekemoer, Anton M., Soto, Emmaris, Conselice, Christopher J., Lucas, Ray A., Wang, Xin, Kim, Keunho J., Alavi, Anahita, Grogin, Norman A., Sunnquist, Ben, Prichard, Laura, Jansen, Rolf A., team, the UVCANDELS
We present the results of our search for Lyman continuum (LyC) emitting AGN at redshifts 2.3$\lesssim$z$\lesssim$4.9 from HST WFC3 F275W observations in the UVCANDELS fields. We also include LyC emission from AGN using HST WFC3 F225W, F275W, and F336
Externí odkaz:
http://arxiv.org/abs/2401.03094
Autor:
Shimasaki, Toshihiko, Bai, Yifei, Kondakci, H. Esat, Dotti, Peter, Pagett, Jared E., Dardia, Anna R., Prichard, Max, Eckardt, André, Weld, David M.
Periodic driving can tune the quasistatic properties of quantum matter. A well-known example is the dynamical modification of tunneling by an oscillating electric field. Here we show experimentally that driving the phasonic degree of freedom of a col
Externí odkaz:
http://arxiv.org/abs/2312.00976
Autor:
Sun, Lei, Wang, Xin, Teplitz, Harry I., Mehta, Vihang, Alavi, Anahita, Rafelski, Marc, Windhorst, Rogier A., Scarlata, Claudia, Gardner, Jonathan P., Smith, Brent M., Sunnquist, Ben, Prichard, Laura, Cheng, Yingjie, Grogin, Norman, Hathi, Nimish P., Hayes, Matthew, Koekemoer, Anton M., Mobasher, Bahram, Nedkova, Kalina V., O'Connell, Robert, Robertson, Brant, Taamoli, Sina, Yung, L. Y. Aaron, Brammer, Gabriel, Colbert, James, Conselice, Christopher, Gawiser, Eric, Guo, Yicheng, Jansen, Rolf A., Ji, Zhiyuan, Lucas, Ray A., Rutkowski, Michael, Siana, Brian, Vanzella, Eros, Ashcraft, Teresa, Bagley, Micaela, Baronchelli, Ivano, Barro, Guillermo, Blanche, Alex, Broussard, Adam, Carleton, Timothy, Chartab, Nima, Codoreanu, Alex, Cohen, Seth, Dai, Y. Sophia, Darvish, Behnam, Davé, Romeel, DeGroot, Laura, De Mello, Duilia, Dickinson, Mark, Emami, Najmeh, Ferguson, Henry, Ferreira, Leonardo, Finkelstein, Keely, Finkelstein, Steven, Gburek, Timothy, Giavalisco, Mauro, Grazian, Andrea, Gronwall, Caryl, Hemmati, Shoubaneh, Howell, Justin, Iyer, Kartheik, Kaviraj, Sugata, Kurczynski, Peter, Lazar, Ilin, MacKenty, John, Mantha, Kameswara Bharadwaj, Martin, Alec, Martin, Garreth, McCabe, Tyler, Olsen, Charlotte, Otteson, Lillian, Ravindranath, Swara, Redshaw, Caleb, Sattari, Zahra, Soto, Emmaris, Zabelle, Bonnabelle, team, the UVCANDELS
UVCANDELS is a HST Cycle-26 Treasury Program awarded 164 orbits of primary ultraviolet (UV) F275W imaging and coordinated parallel optical F435W imaging in four CANDELS fields: GOODS-N, GOODS-S, EGS, and COSMOS, covering a total area of $\sim426$ arc
Externí odkaz:
http://arxiv.org/abs/2311.15664
Autor:
Ronayne, Kaila, Papovich, Casey, Yang, Guang, Shen, Lu, Dickinson, Mark, Kennicutt, Robert, Alavi, Anahita, Haro, Pablo Arrabal, Bagley, Micaela, Burgarella, Denis, Bail, Aurélien Le, Bell, Eric, Cleri, Nikko, Cole, Justin, Costantin, Luca, de la Vega, Alexander, Daddi, Emanuele, Elbaz, David, Finkelstein, Steven, Grogin, Norman, Holwerda, Benne, Kartaltepe, Jeyhan, Kirkpatrick, Allison, Koekemoer, Anton, Lucas, Ray, Magnelli, Benjamin, Mobasher, Bahram, Perez-Gonzalez, Pablo, Prichard, Laura, Rafelski, Marc, Rodighiero, Giulia, Sunnquist, Ben, Teplitz, Harry, Wang, Xin, Windhorst, Rogier, Yung, L. Y. Aaron
We test the relationship between UV-derived star formation rates (SFRs) and the 7.7 ${\mu}$m polycyclic aromatic hydrocarbon (PAH) luminosities from the integrated emission of galaxies at z ~ 0 - 2. We utilize multi-band photometry covering 0.2 - 160
Externí odkaz:
http://arxiv.org/abs/2310.07766
Autor:
Prichard, Max L., Spar, Benjamin M., Morera, Ivan, Demler, Eugene, Yan, Zoe Z., Bakr, Waseem S.
The emergence of quasiparticles in quantum many-body systems underlies the rich phenomenology in many strongly interacting materials. In the context of doped Mott insulators, magnetic polarons are quasiparticles that usually arise from an interplay b
Externí odkaz:
http://arxiv.org/abs/2308.12951