Identifiers
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name variant
Ricardo Bustos
0.60 · backfill
Papers (33)
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Using the antenna impedance to estimate soil electrical parameters for the MIST global 21-cm experiment
astro-ph.IM · 2025 · author #2
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A Measurement of the Largest-Scale CMB E-mode Polarization with CLASS
astro-ph.CO · 2025 · author #7
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High-Efficiency and Low-Noise Detectors for the Upgraded CLASS 90 GHz Focal Plane
astro-ph.IM · 2024 · author #7
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The Atacama Cosmology Telescope: Quantifying Atmospheric Emission above Cerro Toco
astro-ph.IM · 2024 · author #3
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Sensitivity-Improved Polarization Maps at 40 GHz with CLASS and WMAP data
astro-ph.CO · 2024 · author #4
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Simulating the Detection of the Global 21 cm Signal with MIST for Different Models of the Soil and Beam Directivity
astro-ph.IM · 2023 · author #5
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CLASS Observations of Atmospheric Cloud Polarization at Millimeter Wavelengths
astro-ph.IM · 2023 · author #4
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CLASS Angular Power Spectra and Map-Component Analysis for 40 GHz Observations through 2022
astro-ph.CO · 2023 · author #9
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Cosmology Large Angular Scale Surveyor (CLASS): 90 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
astro-ph.IM · 2023 · author #10
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CLASS Data Pipeline and Maps for 40 GHz Observations through 2022
astro-ph.CO · 2023 · author #9
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Microwave Observations of Venus with CLASS
astro-ph.EP · 2023 · author #6
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On-sky performance of new 90 GHz detectors for the Cosmology Large Angular Scale Surveyor (CLASS)
astro-ph.IM · 2023 · author #7
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Cosmology Large Angular Scale Surveyor (CLASS): Pointing Stability and Beam Measurements at 90, 150, and 220 GHz
astro-ph.IM · 2022 · author #8
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Calibration of Transition-edge Sensor (TES) Bolometer Arrays with Application to CLASS
astro-ph.IM · 2022 · author #4
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The Atacama Cosmology Telescope: Modeling Bulk Atmospheric Motion
astro-ph.IM · 2021 · author #2
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Four-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: On-sky Receiver Performance at 40, 90, 150, and 220 GHz Frequency Bands
astro-ph.IM · 2021 · author #7
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Two decades of km-resolution satellite-based measurements of the precipitable water vapor above the Atacama Desert
astro-ph.IM · 2021 · author #5
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Two Year Cosmology Large Angular Scale Surveyor (CLASS) Observations: Long Timescale Stability Achieved with a Front-End Variable-delay Polarization Modulator at 40 GHz
astro-ph.IM · 2020 · author #8
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Venus Observations at 40 and 90 GHz with CLASS
astro-ph.EP · 2020 · author #6
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Twenty years of PWV measurements in the Chajnantor Area
astro-ph.IM · 2020 · author #4
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Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: 40 GHz Telescope Pointing, Beam Profile, Window Function, and Polarization Performance
astro-ph.IM · 2019 · author #10
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Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A First Detection of Atmospheric Circular Polarization at Q Band
astro-ph.IM · 2019 · author #8
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Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz
astro-ph.CO · 2019 · author #8
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The CCAT-Prime Submillimeter Observatory
astro-ph.IM · 2019 · author #9
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On-sky performance of the CLASS Q-band telescope
astro-ph.IM · 2018 · author #9
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CCAT-prime: a novel telescope for submillimeter astronomy
astro-ph.IM · 2018 · author #9
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The Cosmology Large Angular Scale Surveyor Receiver Design
astro-ph.IM · 2018 · author #9
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Design and characterization of the Cosmology Large Angular Scale Surveyor (CLASS) 93 GHz focal plane
astro-ph.IM · 2018 · author #7
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Variable-delay Polarization Modulators for the CLASS Telescopes
astro-ph.IM · 2018 · author #12
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Prime-Cam: A first-light instrument for the CCAT-prime telescope
astro-ph.IM · 2018 · author #8
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Analysis of the distribution of precipitable water vapor in the Chajnantor area
astro-ph.IM · 2016 · author #3
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Parque Astron\'omico de Atacama: An ideal site for millimeter, submillimeter, and mid-infrared astronomy
astro-ph.IM · 2014 · author #1
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The Cosmic Background Imager 2
astro-ph.CO · 2011 · author #7
Mentions
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2503.19401
#2 · arxiv_oai · confidence 0.70
Ricardo Bustos
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2411.12705
#7 · arxiv_oai · confidence 0.70
Ricardo Bustos
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2501.11904
#7 · arxiv_oai · confidence 0.70
Ricardo Bustos
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2410.13064
#3 · arxiv_oai · confidence 0.70
Ricardo Bustos
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2404.17567
#4 · arxiv_oai · confidence 0.70
Ricardo Bustos
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2308.13309
#10 · arxiv_oai · confidence 0.70
Ricardo Bustos
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2310.07741
#5 · arxiv_oai · confidence 0.70
Ricardo Bustos
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2309.00675
#9 · arxiv_oai · confidence 0.70
Ricardo Bustos
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2305.01045
#9 · arxiv_oai · confidence 0.70
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2309.07221
#4 · arxiv_oai · confidence 0.70
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2304.07367
#6 · arxiv_oai · confidence 0.70
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2301.01417
#7 · arxiv_oai · confidence 0.70
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2205.06901
#4 · arxiv_oai · confidence 0.70
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2101.00034
#8 · arxiv_oai · confidence 0.70
Ricardo Bustos
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2208.05022
#8 · arxiv_oai · confidence 0.70
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2103.03917
#5 · arxiv_oai · confidence 0.70
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2111.01319
#2 · arxiv_oai · confidence 0.70
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2107.08022
#7 · arxiv_oai · confidence 0.70
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2010.12739
#6 · arxiv_oai · confidence 0.70
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2007.04262
#4 · arxiv_oai · confidence 0.70
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1911.04499
#10 · arxiv_oai · confidence 0.70
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1911.00391
#8 · arxiv_oai · confidence 0.70
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1911.01016
#8 · arxiv_oai · confidence 0.70
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1909.02587
#9 · arxiv_oai · confidence 0.70
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1811.08287
#9 · arxiv_oai · confidence 0.70
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1807.00058
#8 · arxiv_oai · confidence 0.70
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1807.04167
#9 · arxiv_oai · confidence 0.70
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1807.06675
#9 · arxiv_oai · confidence 0.70
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1807.03927
#7 · arxiv_oai · confidence 0.70
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1807.03807
#12 · arxiv_oai · confidence 0.70
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1609.01252
#3 · arxiv_oai · confidence 0.70
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1108.3950
#7 · arxiv_oai · confidence 0.70
Ricardo Bustos
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1410.2451
#1 · arxiv_oai · confidence 0.70
Ricardo Bustos
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1410.2451
#1 · backfill · confidence 0.70
Ricardo Bustos
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1108.3950
#7 · backfill · confidence 0.70
Ricardo Bustos