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Architectures of Coloniality
Published 2023-11-01“… The Owens Valley Paiute, traditional caretakers of the “Land of Flowing Water,” face continued threats to their livelihood due to decades of water extraction from the region by the city of Los Angeles. …”
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Fumarolic Pathways Were Structurally Controlled by a Strike-Slip Fault System Beneath the Bishop Tuff, Bishop, California
Published 2021-10-01“…The Volcanic Tableland, a plateau at the northern end of Owens Valley, CA, is capped by the rhyolitic Bishop Tuff. …”
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Interstellar Bow Shocks around Fast Stars Passing through the Local Interstellar Medium
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Detecting Fast Radio Bursts with Spectral Structure Using the Continuous Forward Algorithm
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Multifrequency Microwave Imaging of Weak Transients from the Quiet Solar Corona
Published 2023-01-01“…Here we use joint radio observations from the Very Large Array (VLA) and the Expanded Owens Valley Solar Array (EOVSA) to detect transient emissions from the quiet solar corona in the microwave (GHz) domain. …”
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C-Band All-Sky Survey: a first look at the Galaxy
Published 2015“… <p style="text-align:justify;"> We present an analysis of the diffuse emission at 5 GHz in the first quadrant of the Galactic plane using two months of preliminary intensity data taken with the C-Band All-Sky Survey (C-BASS) northern instrument at the Owens Valley Radio Observatory, California. Combining C-BASS maps with ancillary data tomake temperature-temperature plots, we find synchrotron spectral indices of β = -2.65 ± 0.05 between 0.408 and 5 GHz and β = -2.72 ± 0.09 between 1.420 and 5 GHz for -10° > |b| > -4°, 20° > l > 40°. …”
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BLAZARS IN THE FERMI ERA: THE OVRO 40 m TELESCOPE MONITORING PROGRAM
Published 2011“…To capitalize on this opportunity, beginning in late 2007, about a year before the start of LAT science operations, we began a large-scale, fast-cadence 15GHz radio monitoring program with the 40 m telescope at the Owens Valley Radio Observatory. This program began with the 1158 northern (δ > -20°) sources from the Candidate Gamma-ray Blazar Survey and now encompasses over 1500 sources, each observed twice per week with about 4mJy (minimum) and 3% (typical) uncertainty. …”
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Synecological response of spring benthic prokaryotes and macroinvertebrates to Paleozoic roof pendant‐derived calcium
Published 2023-05-01“…Here, we surveyed microbial communities (bacteria and archaea) and benthic macroinvertebrate (BMI) communities in springs that recharge through granitoid bedrock in Owens Valley, CA, to determine whether subtle geochemical differences imparted by metamorphosed roof pendant weathering in the source area affect spring ecosystems. …”
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Program and Results of Investigations Rapid Variability of the BL Lac Object 3C 371 in Radio and Optical Ranges
Published 2020-09-01“…BL Lac object 3C 371 is variable in optical and radio range, according to long-term monitoring data, for example AAVSO (American Association of Variable Star Observers) and OVRO (Owens Valley Radio Observatory). In addition, some authors note intra-night variability. …”
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The Solar Origin of an In Situ Type III Radio Burst Event
Published 2023-01-01“…This event was associated with a solar jet that produced an impulsive microwave burst event recorded by the Expanded Owens Valley Solar Array. The type III burst event also coincided with the detection of enhanced in situ energetic electrons recorded by both PSP at 0.37 au and WIND at 1 au, which were located very closely on the Parker spiral longitudinally. …”
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Rapid variations of Si IV spectra in a flare observed by interface region imaging spectrograph at a sub-second cadence
Published 2022-11-01“…Furthermore, peaks of the intensity and the trends of Doppler velocity of the Gaussian fit to the secondary component (averaged in the ribbon) were found to correspond to one of the quasi-periodic pulsations (QPPs) detected during the event in the soft X-ray flux (as measured by the Geostationary Operational Environmental Satellite, GOES) and the microwave radio flux (as measured by the Expanded Owens Valley Solar Array, EOVSA). This result supports a scenario in which the QPPs were driven by repeated magnetic reconnection.…”
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PROPERTY STUDY OF OJ 287 AND BL LAC VARIABILITY IN OPTICALAND RADIO RANGES
Published 2019-12-01“…Design/methodology/approach: The authors used the data of optical observations of OJ 287 in 1978–2018 and of BL Lac in 1970–2018 from the AAVSO (American Association of Variable Star Observers) catalog and from the catalog of a long-term (2008–2018) radio source monitoring at the 40-meter radio telescope, OVRO observatory (Owens Valley Radio Observatory, USA) at 15 GHz, as well as the data from UMRAO observatory (Radio observatory of Michigan University) obtained at 14.5 GHz within 1974–2011. …”
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Temporal and Spectral Properties of the Persistent Radio Source Associated with FRB 20190520B with the VLA
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Spectral Observations and Modeling of a Solar White-light Flare Observed by CHASE
Published 2023-01-01“…The white-light kernels are cospatial with the microwave footpoint sources observed by the Expanded Owens Valley Solar Array and the time profile of the white-light emission matches that of the hard X-ray emission above 30 keV from the Gamma-ray Burst Monitor (GBM) on Fermi. …”
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VERITAS Discovery of Very High Energy Gamma-Ray Emission from S3 1227+25 and Multiwavelength Observations
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Multimessenger Characterization of Markarian 501 during Historically Low X-Ray and γ-Ray Activity
Published 2023-01-01“…We study the broadband emission of Mrk 501 using multiwavelength observations from 2017 to 2020 performed with a multitude of instruments, involving, among others, MAGIC, Fermi's Large Area Telescope (LAT), NuSTAR, Swift, GASP-WEBT, and the Owens Valley Radio Observatory. Mrk 501 showed an extremely low broadband activity, which may help to unravel its baseline emission. …”
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Searches for Neutrinos in the Direction of Radio-bright Blazars with the ANTARES Telescope
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