activity
20072019
most citedFive Debris Disks Newly Revealed in Scattered Light from the HST NICMOS Archive

67 citations · 281 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.EP2019★ 46 cited

An Exo-Kuiper Belt and An Extended Halo around HD 191089 in Scattered Light

Bin Ren, Élodie Choquet, Marshall D. Perrin +70

We have obtained Hubble Space Telescope STIS and NICMOS, and Gemini/GPI scattered light images of the HD 191089 debris disk. We identify two spatial components: a ring resembling K…

astro-ph.SR2016★ 7 cited

Constraints on the presence of SiO gas in the debris disk of HD 172555

T. L. Wilson, R. Nilsson, C. H. Chen +4

We have carried out two sets of observations to quantify the properties of SiO gas in the unusual HD 172555 debris disk: (1) a search for the J=8-7 rotational transition from the v…

astro-ph.SR2014★ 67 cited

Five Debris Disks Newly Revealed in Scattered Light from the HST NICMOS Archive

Rémi Soummer, Marshall D. Perrin, Laurent Pueyo +12

We have spatially resolved five debris disks (HD 30447, HD 35841, HD 141943, HD 191089, and HD 202917) for the first time in near-infrared scattered light by reanalyzing archival H…

astro-ph.SR2013★ 3 cited

Twenty-Five Sub-Arcsecond Binaries Discovered By Lunar Occultations

A. Richichi, O. Fors, F. Cusano +1

We report on 25 sub-arcsecond binaries, detected for the first time by means of lunar occultations in the near-infrared as part of a long-term program using the ISAAC instrument at…

astro-ph.SR2013★ 5 cited

The Curious Case of Glass I: High Ionization and Variability of Different Types

Andrew J. Kruger, Matthew J. Richter, John S. Carr +4

Our Spitzer IRS observation of the infrared companion Glass Ib revealed fine structure emission with high ionization ([NeIII]/[NeII]=2.1 and [SIV]/[SIII]=0.6) that indicates the ga…

astro-ph.SR2013★ 27 cited

An active asteroid belt causing the UX Ori phenomenon in RZ Psc

W. J. de Wit, V. P. Grinin, I. S. Potravnov +3

We report the discovery of mid-infrared excess emission in the young object RZ Psc. The excess constitutes ~8% of its Lbol, and is well fit by a single 500K black-body implying a d…