activity
20092026
most citedFormation of Organic Molecules and Water in Warm Disk Atmospheres

90 citations · 417 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2026

Qualification pathways for Photonic Integrated Circuits in Astrophotonic Space Missions

Kalaga Madhav, Aashia Rahman, Máté Ádámkovics

Photonic integrated circuits (PICs) promise order-of-magnitude reductions in the size, weight and power (SWaP) of optical subsystems for astronomy, planetary and Earth-observation…

astro-ph.EP2021★ 14 cited

High Spatial and Spectral Resolution Observations of the Forbidden 1.707 micron Rovibronic SO Emissions on Io: Evidence for Widespread Stealth Volcanism

Imke de Pater, Katherine de Kleer, Mate Adamkovics

We present observations obtained with the 10-m Keck telescopes of the forbidden SO rovibronic transition at 1.707 micron on Io while in eclipse. We show its spatial distribution at…

astro-ph.EP2020★ 8 cited

Modeling transmission windows in Titan's lower troposphere: Implications for infrared spectrometers aboard future aerial and surface missions

Paul Corlies, George D. McDonald, Alexander G. Hayes +10

From orbit, the visibility of Titan's surface is limited to a handful of narrow spectral windows in the near-infrared (near-IR), primarily from the absorption of methane gas. This…

astro-ph.EP2019★ 44 cited

First ALMA Millimeter Wavelength Maps of Jupiter, with a Multi-Wavelength Study of Convection

Imke de Pater, R. J. Sault, Chris Moeckel +15

We obtained the first maps of Jupiter at 1-3 mm wavelength with the Atacama Large Millimeter/Submillimeter Array (ALMA) on 3-5 January 2017, just days after an energetic eruption a…

astro-ph.EP2018★ 40 cited

The Gas Composition and Deep Cloud Structure of Jupiter's Great Red Spot

Gordon L. Bjoraker, Michael H. Wong, Imke de Pater +3

We have obtained high-resolution spectra of Jupiter's Great Red Spot (GRS) between 4.6 and 5.4 microns using telescopes on Mauna Kea in order to derive gas abundances and to constr…

astro-ph.SR2017★ 18 cited

FUV Irradiation and the Heat Signature of Accretion in Protoplanetary Disk Atmospheres

Joan R. Najita, Mate Adamkovics

Although stars accrete mass throughout the first few Myr of their lives, the physical mechanism that drives disk accretion in the T Tauri phase is uncertain, and diagnostics that p…

astro-ph.EP2017★ 21 cited

Retrieving Neptune's aerosol properties from Keck OSIRIS observations. I. Dark regions

S. H. Luszcz-Cook, K. de Kleer, I. de Pater +2

We present and analyze three-dimensional data cubes of Neptune from the OSIRIS integral-field spectrograph on the 10-m Keck telescope, from July 2009. These data have a spatial res…

astro-ph.EP2016★ 42 cited

The near-surface methane humidity on Titan

Juan M. Lora, Mate Adamkovics

We retrieve vertical and meridional variations of methane mole fraction in Titan's lower troposphere by re-analyzing near-infrared ground-based observations from 17 July 2014 UT (A…

astro-ph.IM2016★ 8 cited

The InfraRed Imaging Spectrograph (IRIS) for TMT: latest science cases and simulations

Shelley A. Wright, Gregory Walth, Tuan Do +36

The Thirty Meter Telescope (TMT) first light instrument IRIS (Infrared Imaging Spectrograph) will complete its preliminary design phase in 2016. The IRIS instrument design includes…

astro-ph.EP2015★ 31 cited

Titan Science with the James Webb Space Telescope (JWST)

Conor A. Nixon, Richard K. Achterberg, Mate Adamkovics +12

The James Webb Space Telescope (JWST), scheduled for launch in 2018, is the successor to the Hubble Space Telescope (HST) but with a significantly larger aperture (6.5 m) and advan…

astro-ph.IM2014★ 7 cited

The InfraRed Imaging Spectrograph (IRIS) for TMT: Overview of innovative science programs

Shelley A. Wright, James E. Larkin, Anna M. Moore +22

IRIS (InfraRed Imaging Spectrograph) is a first light near-infrared diffraction limited imager and integral field spectrograph being designed for the future Thirty Meter Telescope…

astro-ph.EP2012

The changing rotational excitation of C_3 in comet 9P/Tempel 1 during Deep Impact

Máté Ádámkovics, Imke de Pater, Hy Spinrad

The 4050Å band of C was observed with Keck/HIRES echelle spectrometer during the {\em Deep Impact} encounter. We perform a 2-dimensional analysis of the exposures in order to s…

astro-ph.SR2011★ 90 cited

Formation of Organic Molecules and Water in Warm Disk Atmospheres

Joan R. Najita, Mate Adamkovics, Alfred E. Glassgold

Observations from Spitzer and ground-based infrared spectroscopy reveal significant diversity in the molecular emission from the inner few AU of T Tauri disks. We explore theoretic…

astro-ph.SR2010★ 47 cited

Dust, Ice and Gas in Time (DIGIT) Herschel program first results: A full PACS-SED scan of the gas line emission in protostar DK Cha

T. A. van Kempen, J. D. Green, N. J. Evans +42

DK Cha is an intermediate-mass star in transition from an embedded configuration to a star plus disk stage. We aim to study the composition and energetics of the circumstellar mate…

astro-ph.EP2009★ 27 cited

Discovery of fog at the south pole of Titan

M. E. Brown, A. L. Smith, C. Chen +1

While Saturn's moon Titan appears to support an active methane hydrological cycle, no direct evidence for surface-atmosphere exchange has yet appeared. It is possible that the iden…

astro-ph.EP2009★ 20 cited

Component-resolved Near-infrared Spectra of the (22) Kalliope System

Conor Laver, Imke de Pater, Franck Marchis +2

We observed (22) Kalliope and its companion Linus with the integral-field spectrograph OSIRIS, which is coupled to the adaptive optics system at the W.M. Keck II telescope on March…