Zobrazeno 1 - 10
of 17 386
pro vyhledávání: '"Péter T"'
Autor:
Narola, Harsh, Wouters, Thibeau, Negri, Luca, Lopez, Melissa, Dooney, Tom, Cireddu, Francesco, Wils, Milan, Wong, Isaac C. F., Pang, Peter T. H., Janquart, Justin, Samajdar, Anuradha, Broeck, Chris Van Den, Li, Tjonnie G. F.
Gravitational Wave (GW) detectors routinely encounter transient noise bursts, known as glitches, which are caused by either instrumental or environmental factors. Due to their high occurrence rate, glitches can overlap with GW signals, as in the nota
Externí odkaz:
http://arxiv.org/abs/2411.15506
Autor:
Kunnumkai, Keerthi, Palmese, Antonella, Farah, Amanda M, Bulla, Mattia, Dietrich, Tim, Pang, Peter T H, Anand, Shreya, Andreoni, Igor, Cabrera, Tomas, Connor, Brendan O
With GW170817 being the only multimessenger gravitational wave (GW) event with an associated kilonova (KN) detected so far, there exists a pressing need for realistic estimation of the GW localization uncertainties and rates, as well as optimization
Externí odkaz:
http://arxiv.org/abs/2411.13673
Autor:
Hendrix, Zachary H., Brown, Peter T., Flanagan, Tim, Shepherd, Douglas P., Saurabh, Ayush, Pressé, Steve
Richardson-Lucy deconvolution is widely used to restore images from degradation caused by the broadening effects of a point spread function and corruption by photon shot noise, in order to recover an underlying object. In practice, this is achieved b
Externí odkaz:
http://arxiv.org/abs/2411.00991
Autor:
Jhawar, Sahil, Wouters, Thibeau, Pang, Peter T. H., Bulla, Mattia, Coughlin, Michael W., Dietrich, Tim
Kilonovae, possible electromagnetic counterparts to neutron star mergers, provide important information about high-energy transient phenomena and, in principle, also allow us to obtain information about the source properties responsible for powering
Externí odkaz:
http://arxiv.org/abs/2410.21978
We present an accelerated pipeline, based on high-performance computing techniques and normalizing flows, for joint Bayesian parameter estimation and model selection and demonstrate its efficiency in gravitational wave astrophysics. We integrate the
Externí odkaz:
http://arxiv.org/abs/2410.21076
Autor:
Diamandi, Hilel Hagai, Luo, Yizhi, Mason, David, Kanmaz, Tevfik Bulent, Ghosh, Sayan, Pavlovich, Margaret, Yoon, Taekwan, Behunin, Ryan, Puri, Shruti, Harris, Jack G. E., Rakich, Peter T.
High-fidelity quantum optomechanical control of a mechanical oscillator requires the ability to perform efficient, low-noise operations on long-lived phononic excitations. Microfabricated high-overtone bulk acoustic wave resonators ($\mathrm{\mu}$HBA
Externí odkaz:
http://arxiv.org/abs/2410.18037
Autor:
Cheng, Haotian, Xiang, Chao, Jin, Naijun, Kudelin, Igor, Guo, Joel, Heyrich, Matthew, Liu, Yifan, Peters, Jonathan, Ji, Qing-Xin, Zhou, Yishu, Vahala, Kerry J., Quinlan, Franklyn, Diddams, Scott A., Bowers, John E., Rakich, Peter T.
Compact photonic systems that offer high frequency stability and low noise are of increasing importance to applications in precision metrology, quantum computing, communication, and advanced sensing technologies. However, on-chip resonators comprised
Externí odkaz:
http://arxiv.org/abs/2410.01095
Autor:
Kunnumkai, Keerthi, Palmese, Antonella, Bulla, Mattia, Dietrich, Tim, Farah, Amanda M., Pang, Peter T. H.
The detection of the gravitational-wave event GW230529, presumably a neutron star-black hole (NSBH) merger, by the LIGO-Virgo-KAGRA (LVK) Collaboration is an exciting discovery for multimessenger astronomy. The black hole (BH) has a high probability
Externí odkaz:
http://arxiv.org/abs/2409.10651
Random coalescent processes and branching processes are two fundamental constructs in the field of stochastic processes, each with a rich history and a wide range of applications. Though developed within distinct contexts, in this note we present a n
Externí odkaz:
http://arxiv.org/abs/2409.06910
Autor:
Dahal, Sumit, Ade, Peter A. R., Anderson, Christopher J., Barlis, Alyssa, Barrentine, Emily M., Beeman, Jeffrey W., Bellis, Nicholas, Bolatto, Alberto D., Braianova, Victoria, Breysse, Patrick C., Bulcha, Berhanu T., Cataldo, Giuseppe, Colazo, Felipe A., Chevres-Fernandez, Lee-Roger, Cho, Chullhee, Chmaytelli, Danny S., Connors, Jake A., Costen, Nicholas P., Cursey, Paul W., Ehsan, Negar, Essinger-Hileman, Thomas M., Glenn, Jason, Golec, Joseph E., Hays-Wehle, James P., Hess, Larry A., Jahromi, Amir E., Jenkins, Trevian, Kimball, Mark O., Kogut, Alan J., Kramer, Samuel H., Leung, Nicole, Lowe, Luke N., Mauskopf, Philip D., McMahon, Jeffrey J., Mikula, Vilem, Mirzaei, Mona, Moseley, Samuel H., Mugge-Durum, Jonas W., Nellis, Jacob, Noroozian, Omid, Okun, Kate, Oxholm, Trevor, Parekh, Tatsat, Pen, Ue-Li, Pullen, Anthony R., Rahmani, Maryam, Ramirez, Mathias M., Roberson, Cody, Rodriguez, Samelys, Roselli, Florian, Sapkota, Deepak, Shire, Konrad, Siebert, Gage L., Siddique, Faizah, Sinclair, Adrian K., Somerville, Rachel S., Stephenson, Ryan, Stevenson, Thomas R., Switzer, Eric R., Termini, Jared, Timbie, Peter T., Trenkamp, Justin, Tucker, Carole E., Visbal, Elijah, Volpert, Carolyn G., Watson, Joseph, Weeks, Eric, Wollack, Edward J., Yang, Shengqi, Yung, Aaron
Publikováno v:
Proc. SPIE 13102, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII, 131022I (16 August 2024)
The EXperiment for Cryogenic Large-Aperture Intensity Mapping (EXCLAIM) is a balloon-borne telescope designed to survey star formation over cosmological time scales using intensity mapping in the 420 - 540 GHz frequency range. EXCLAIM uses a fully cr
Externí odkaz:
http://arxiv.org/abs/2409.02847