Zobrazeno 1 - 10
of 15 498
pro vyhledávání: '"Marrone A"'
We present the first combined analysis of quark and lepton observables in flavour models based on modular invariance. The analysis is performed within a specific model with modular $2O$ symmetry. Unlike previous studies, which analyzed observables in
Externí odkaz:
http://arxiv.org/abs/2409.15823
Autor:
Farah, Joseph, Galison, Peter, Akiyama, Kazunori, Bouman, Katherine L., Bower, Geoffrey C., Chael, Andrew, Fuentes, Antonio, Gómez, José L., Honma, Mareki, Johnson, Michael D., Kofuji, Yutaro, Marrone, Daniel P., Moriyama, Kotaro, Narayan, Ramesh, Pesce, Dominic W., Tiede, Paul, Wielgus, Maciek, Zhao, Guang-Yao, Collaboration, The Event Horizon Telescope
Publikováno v:
ApJL, Volume 930, L18, 2022
Recent developments in very long baseline interferometry (VLBI) have made it possible for the Event Horizon Telescope (EHT) to resolve the innermost accretion flows of the largest supermassive black holes on the sky. The sparse nature of the EHT's $(
Externí odkaz:
http://arxiv.org/abs/2409.08321
The J=1$\rightarrow$0 spectral line of carbon monoxide (CO(1-0)) is the canonical tracer of molecular gas. However, CO(2-1) is frequently used in its place, following the assumption that the higher energy line can be used to infer the CO(1-0) luminos
Externí odkaz:
http://arxiv.org/abs/2409.03963
Autor:
Keenan, Ryan P., Marrone, Daniel P., Keating, Garrett K., Mayer, Evan C., Bays, Kevin, Downey, John, Dunn, Lochlann C., Flores, Joanne C., Folkers, Thomas W., Forbes, David C., Guvenen, Blythe C., Holmstedt, Christian, Moulton, Robert M., Sullivan, Patrick
The CO(1-0) line has been carefully calibrated as a tracer of molecular gas mass. However, recent studies often favor higher J transitions of the CO molecule which are brighter and accessible for redshift ranges where CO(1-0) is not. These lines are
Externí odkaz:
http://arxiv.org/abs/2408.02617
Autor:
Liu, Lun-Jun, Janssen, Reinier M. J., Bumble, Bruce, Kane, Elijah, Foote, Logan M., Bradford, Charles M., Hailey-Dunsheath, Steven, Agrawal, Shubh, Aguirre, James E., Athreya, Hrushi, Bracks, Justin S., Brendal, Brockton S., Corso, Anthony J., Filippini, Jeffrey P., Fu, Jianyang, Groppi, Christopher E., Joralmon, Dylan, Keenan, Ryan P., Kowalik, Mikolaj, Lowe, Ian N., Manduca, Alex, Marrone, Daniel P., Mauskopf, Philip D., Mayer, Evan C., Nie, Rong, Razavimaleki, Vesal, Saeid, Talia, Trumper, Isaac, Vieira, Joaquin D.
We report on the effects of cosmic ray interactions with the Kinetic Inductance Detector (KID) based focal plane array for the Terahertz Intensity Mapper (TIM). TIM is a NASA-funded balloon-borne experiment designed to probe the peak of the star form
Externí odkaz:
http://arxiv.org/abs/2407.17381
Autor:
Sridharan, T. K., Lehmensiek, R., Marrone, D., Cheimets, P., Freeman, M., Galison, P., Houston, J., Johnson, M., Silver, M.
We present the basic design of a large, light weight, spaceborne antenna for the Black Hole Explorer (BHEX) space Very Long Baseline Interferometry (space-VLBI) mission, achieving high efficiency operation at mm/sub-mm wavelengths. An introductory ov
Externí odkaz:
http://arxiv.org/abs/2406.10394
Autor:
Marrone, Daniel P., Houston, Janice, Akiyama, Kazunori, Bilyeu, Bryan, Boroson, Don, Grimes, Paul, Haworth, Kari, Lehmensiek, Robert, Peretz, Eliad, Rana, Hannah, Sinclair, Laura C., Kumara, Sridharan Tirupati, Srinivasan, Ranjani, Tong, Edward, Wang, Jade, Weintroub, Jonathan, Johnson, Michael D.
The Black Hole Explorer (BHEX) is a space very-long-baseline interferometry (VLBI) mission concept that is currently under development. BHEX will study supermassive black holes at unprecedented resolution, isolating the signature of the "photon ring"
Externí odkaz:
http://arxiv.org/abs/2406.10143
Autor:
Srinivasan, Ranjani, Weintroub, Jonathan, Raffanti, Rick, Bilyeu, Bryan, Gauron, Thomas, Test, John, Richards, Elliot, Fernandez, Manuel, Freeman, Mark, Cheimets, Peter, Gendelman, Mauricio, Haworth, Kari, Houston, Janice, Johnson, Michael D., Mamani, Emilia, Marrone, Daniel, Pola, Ariel L., Wang, Jade
This paper describes specification and early design of back end signal processing subsystems for the Black Hole Explorer (BHEX) Very Long Baseline Interferometry (VLBI) space telescope. The "back end" consists of two subsystems. First, the block down
Externí odkaz:
http://arxiv.org/abs/2406.10103
Autor:
Rana, Hannah, Akiyama, Kazunori, Canavan, Edgar, DiPirro, Michael, Freeman, Mark, Galison, Peter, Grimes, Paul, Honma, Mareki, Houston, Janice, Johnson, Michael, Kimball, Mark, Marrone, Daniel, Tong, Edward
The Black Hole Explorer (BHEX) is a space-based very-long baseline interferometry (VLBI) mission aimed at precision black hole measurements, detecting the photon ring around black holes, exploring spacetime, spin, and mass properties, and validating
Externí odkaz:
http://arxiv.org/abs/2406.09975
Autor:
Johnson, Michael D., Akiyama, Kazunori, Baturin, Rebecca, Bilyeu, Bryan, Blackburn, Lindy, Boroson, Don, Cardenas-Avendano, Alejandro, Chael, Andrew, Chan, Chi-kwan, Chang, Dominic, Cheimets, Peter, Chou, Cathy, Doeleman, Sheperd S., Farah, Joseph, Galison, Peter, Gamble, Ronald, Gammie, Charles F., Gelles, Zachary, Gomez, Jose L., Gralla, Samuel E., Grimes, Paul, Gurvits, Leonid I., Hadar, Shahar, Haworth, Kari, Hada, Kazuhiro, Hecht, Michael H., Honma, Mareki, Houston, Janice, Hudson, Ben, Issaoun, Sara, Jia, He, Jorstad, Svetlana, Kauffmann, Jens, Kovalev, Yuri Y., Kurczynski, Peter, Lafon, Robert, Lupsasca, Alexandru, Lehmensiek, Robert, Ma, Chung-Pei, Marrone, Daniel P., Marscher, Alan P., Melnick, Gary J., Narayan, Ramesh, Niinuma, Kotaro, Noble, Scott C., Palmer, Eric J., Palumbo, Daniel C. M., Paritsky, Lenny, Peretz, Eliad, Pesce, Dominic, Plavin, Alexander, Quataert, Eliot, Rana, Hannah, Ricarte, Angelo, Roelofs, Freek, Shtyrkova, Katia, Sinclair, Laura C., Small, Jeffrey, Kumara, Sridharan Tirupati, Srinivasan, Ranjani, Strominger, Andrew, Tiede, Paul, Tong, Edward, Wang, Jade, Weintroub, Jonathan, Wielgus, Maciek, Wong, George, Zhang, Xinyue Alice
We present the Black Hole Explorer (BHEX), a mission that will produce the sharpest images in the history of astronomy by extending submillimeter Very-Long-Baseline Interferometry (VLBI) to space. BHEX will discover and measure the bright and narrow
Externí odkaz:
http://arxiv.org/abs/2406.12917