output
20022026
most citedA Brief Survey of Deep Reinforcement Learning

4.4k citations

Showing 2021 · astro-ph.IMShow all

16 papers · 2 filters

astro-ph.IM2021★ 8 cited

Validation Solutions to the Full-Sky Radio Interferometry Measurement Equation for Diffuse Emission

Adam E. Lanman, Steven G. Murray, Daniel C. Jacobs

Low-frequency radio observatories are reaching unprecedented levels of sensitivity in an effort to detect the 21 cm signal from the Cosmic Dawn. High precision is needed because th…

astro-ph.IM2021

The Correlation Calibration of PAPER-64 data

Tamirat G. Gogo, Yin-Zhe Ma, Piyanat Kittiwisit +21

Observation of redshifted 21-cm signal from the Epoch of Reionization (EoR) is challenging due to contamination from the bright foreground sources that exceed the signal by several…

astro-ph.IM2021★ 1 cited

In-flight gain monitoring of SPIDER's transition-edge sensor arrays

J. P. Filippini, A. E. Gambrel, A. S. Rahlin +67

Experiments deploying large arrays of transition-edge sensors (TESs) often require a robust method to monitor gain variations with minimal loss of observing time. We propose a sens…

astro-ph.IM2021★ 4 cited

Probing the role of magnetic fields in star-forming filaments: NIKA2-Pol commissioning results toward OMC-1

H. Ajeddig, R. Adam, P. Ade +43

Dust polarization observations are a powerful, practical tool to probe the geometry (and to some extent, the strength) of magnetic fields in star-forming regions. In particular, Pl…

astro-ph.IM2021★ 3 cited

Onboard Dynamic Image Exposure Control for the Star-Planet Activity Research CubeSat (SPARCS)

Tahina Ramiaramanantsoa, Judd D. Bowman, Evgenya L. Shkolnik +19

The Star-Planet Activity Research CubeSat (SPARCS) is a 6U CubeSat under development to monitor the flaring and chromospheric activity of M dwarfs at near-ultraviolet (NUV) and far…

astro-ph.IM2021★ 10 cited

Scintillation-limited photometry with the 20-cm NGTS telescopes at Paranal Observatory

Sean M. O'Brien, Daniel Bayliss, James Osborn +17

Ground-based photometry of bright stars is expected to be limited by atmospheric scintillation, although in practice observations are often limited by other sources of systematic n…