activity
20182025
most citedEvolution of Neptune at Near-Infrared Wavelengths from 1994 through 2022

16 citations · 31 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2025

Increasing science yield with a twilight observing program with the SCALES instrument at Keck

Isabel J. Kain, Carlos Alvarez, John M. O'Meara +13

While astronomical twilight closes the observing window for optical astronomers, the infrared sky remains dark even through sunrise, allowing IR astronomers to observe through twil…

astro-ph.EP2023★ 16 cited

Evolution of Neptune at Near-Infrared Wavelengths from 1994 through 2022

Erandi Chavez, Imke de Pater, Erin Redwing +15

Using archival near-infrared observations from the Keck and Lick Observatories and the Hubble Space Telescope, we document the evolution of Neptune's cloud activity from 1994 to 20…

astro-ph.EP2023★ 2 cited

Drift Rates of Major Neptunian Features between 2018 and 2021

Erandi Chavez, Erin Redwing, Imke de Pater +13

Using near-infrared observations of Neptune from the Keck and Lick Observatories, and the Hubble Space Telescope in combination with amateur datasets, we calculated the drift rates…

astro-ph.EP2022

NaCl & KCl in Io's Atmosphere

Erin Redwing, Imke de Pater, Statia Luszcz-Cook +3

We present the first comprehensive study of NaCl and KCl gases in Io's atmosphere in order to investigate their characteristics, and to infer properties of Io's volcanoes and subsu…

astro-ph.EP2020

ALMA Observations of Io Going into and Coming out of Eclipse

Imke de Pater, Statia Luszcz-Cook, Patricio Rojo +3

We present 1-mm observations constructed from ALMA [Atacama Large (sub)Millimeter Array] data of SO, SO and KCl when Io went from sunlight into eclipse (20 March 2018), and vic…

astro-ph.EP2018★ 13 cited

Small and Nearby NEOs Observed by NEOWISE During the First Three Years of Survey: Physical Properties

Joseph R. Masiero, E. Redwing, A. K. Mainzer +7

Automated asteroid detection routines set requirements on the number of detections, signal-to-noise ratio, and the linearity of the expected motion in order to balance completeness…