Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Briley Lewis"'
Publikováno v:
The Astronomical Journal, Vol 165, Iss 2, p 59 (2023)
We introduce a new framework for point-spread function subtraction based on the spatiotemporal variation of speckle noise in high-contrast imaging data where the sampling timescale is faster than the speckle evolution timescale. One way that space–
Externí odkaz:
https://doaj.org/article/01c5efc99d864faca9478173f827145a
Autor:
Pauline Arriaga, Jesus Salas, Aidan Gibbs, Mason G. MacDougall, Rory O. Bentley, Abhimat K. Gautam, Ronald Lopez, Peter Williams, Briley Lewis
The UCLA Planetarium hosts star shows and lectures on various astronomy topics, educating UCLA and the broader Los Angeles community about science and the wonders of the night sky. It serves over 4...
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::44d2ebc078dc6e4463a198791409ca4c
https://doi.org/10.1002/essoar.10504207.1
https://doi.org/10.1002/essoar.10504207.1
Autor:
Oliver L. White, Bernard Schmitt, Perianne E. Johnson, Kathy E. Mandt, Briley Lewis, Leslie A. Young, John Stansberry, Silvia Protopapa, L. Gabasova
Publikováno v:
Icarus
Icarus, Elsevier, 2019, pp.114070. ⟨10.1016/j.icarus.2020.114070⟩
Icarus, Elsevier, 2019, pp.114070. ⟨10.1016/j.icarus.2020.114070⟩
Pluto has a heterogeneous surface, despite a global haze deposition rate of ~1 micrometer per orbit (Cheng et al., 2017; Grundy et al., 2018). While there could be spatial variation in the deposition rate, this has not yet been rigorously quantified,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bddeaad85d5554659a33627b80c30df0
http://arxiv.org/abs/2008.10716
http://arxiv.org/abs/2008.10716
Autor:
Kieran O'Brien, Briley Lewis, Isabel Lipartito, Neelay Fruitwala, Kristina K. Davis, Benjamin A. Mazin, Rupert Dodkins, Niranjan Thatte, Sumedh Mahashabde
Publikováno v:
Publications of the Astronomical Society of the Pacific, 2020, Vol.132(1016) [Peer Reviewed Journal]
Optical and near-infrared Microwave Kinetic Inductance Detectors, or MKIDs, are low-temperature detectors with inherent spectral resolution that are able to instantly register individual photons with potentially no false counts or readout noise. Thes
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78dbfa16042527d4e96bb28bd2e395ef
http://arxiv.org/abs/2007.15274
http://arxiv.org/abs/2007.15274
Autor:
Eden Molina, Rebecca Lewis, Caroline Nagib, Robert Geil, Kyle Neville, Valerie Rockwell, Zhixian Wang, Jean-Luc Margot, In Yun, Julia Gonzales, Jose Cebreros, Lujia Zhu, Kristy Kwan Lin Fu, Mason G. MacDougall, Armen Tokadjian, Stephen Alexander, Myank Singhal, Grace Li, Christopher Makarem, Sanjana Prabhu Desai, Samar Seth, Rehan Shah, Ryan S. Lynch, Yuri Shimane, Ivan Manan, Alex O. Gonzalez, Briley Lewis, Rishabh M. Jain, Lizvette Villafana, Yoichiro Rokushima, Riley Dunne, Adrian Lam, Carlyn Schmidgall, Pavlo Pinchuk, Shashwat Goel, Sparsh Arora, Connor O’Toole, Griffin Romanek, Benjamin Duclos, Swagata Biswas
Publikováno v:
The Astronomical Journal, vol 161, iss 2
Astronomical Journal, vol 161, iss 2
Astronomical Journal, vol 161, iss 2
We conducted a search for technosignatures in April of 2018 and 2019 with the L-band receiver (1.15-1.73 GHz) of the 100 m diameter Green Bank Telescope. These observations focused on regions surrounding 31 Sun-like stars near the plane of the Galaxy
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d0c0ef74aa69d06419d58492eecdb96f
https://doi.org/10.3847/1538-3881/abcc77
https://doi.org/10.3847/1538-3881/abcc77