activity
20022025
most citedThe Inner Rings of Beta Pictoris

118 citations · 190 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2025

Studying the Dust Distribution Around Accreting Black Holes with Reverberation Mapping Using PRIMA

Varoujan Gorjian, Michael W. Werner

Variability studies are a powerful tool for studying the structures of unresolved sources. One such type of variability study, called reverberation mapping (RM), established that t…

astro-ph.EP2025★ 8 cited

Low 4.5 μm Dayside Emission Disfavors a Dark Bare-Rock scenario for the Hot Super-Earth TOI-431 b

Christopher Monaghan, Pierre-Alexis Roy, Björn Benneke +13

The full range of conditions under which rocky planets can host atmospheres remains poorly understood, especially in the regime of close-in orbits around late-type stars. One way t…

astro-ph.EP2024

Modeling Spitzer 3.6 and 4.5 m Eclipse Depths for the Inflated Hot Jupiter in the Evolved Binary System HD 202772

Arthur D. Adams, Kimberly Bott, Paul A. Dalba +9

As an inflated Hot Jupiter orbiting an early-type primary star in the evolved binary HD 202772 system, HD 202772 A b's presence invites a study of how such a planet forms and evolv…

astro-ph.HE2013★ 26 cited

Fermi-LAT upper limits on gamma-ray emission from colliding wind binaries

M. Werner, O. Reimer, A. Reimer +1

Context: Colliding wind binaries (CWBs) are thought to give rise to a plethora of physical processes including acceleration and interaction of relativistic particles. Observation o…

astro-ph.HE2012★ 38 cited

Gamma-ray follow-up studies on Eta Carinae

K. Reitberger, O. Reimer, A. Reimer +3

Observations of high energy gamma rays recently revealed a persistent source in spatial coincidence with the binary system Eta Carinae. Since modulation of the observed gamma-ray f…

astro-ph2002★ 118 cited

The Inner Rings of Beta Pictoris

Z. Wahhaj, D. W. Koerner, M. E. Ressler +3

We present Keck images of the dust disk around Beta Pictoris at 17.9 microns that reveal new structure in its morphology. Within 1" (19 AU) of the star, the long axis of the dust e…