Add to ORKGWe present the results of a deep high-contrast imaging search for planets around Vega. Vega is an ideal target for high-contrast imaging because it is bright, nearby, and young with a face-on two-belt debris disk that may be shaped by unseen planets. We obtained J- and H-band data on Vega with the coronagraphic integral-field spectrograph Project 1640 (P1640) at Palomar Observatory. Two nights of data were obtained in 2016, in poor seeing conditions, and two additional nights in more favorable conditions in 2017. In total, we obtained 5.5 hours of integration time on Vega in moderate to good seeing conditions (<1farcs5). We did not detect any low-mass companions in this system. Our data present the most sensitive contrast limits around Vega...
Vega excess stars are main sequence stars which are surrounded by a cool dust disk, left as a remna...
Vega and Fomalhaut are similar in terms of mass, ages, and global debris disk properties; therefore,...
We present new observations of the Vega system with the Plateau de Bure Interferometer. The debris d...
We present the results of a deep high-contrast imaging search for planets around Vega. Vega is an id...
From adaptive optics observations with the Palomar 5 m telescope we place upper limits on the masses...
We report on high contrast near-infrared (~2.2 μm) observations of Vega obtained with the Palomar Fi...
Using the FLUOR near-infrared beam combiner installed at the CHARA Array (Mt Wilson, CA), we have ob...
Context. Gaps in circumstellar disks can signal the existence of planetary perturbers, making such s...
Context: Only a handful of debris disks have been imaged up to now. Due to the need for high dynamic...
Stars with debris disks are intriguing targets for direct-imaging exoplanet searches, owing both to ...
Using the FLUOR beam-combiner installed at the CHARA Array (Mt. Wilson, CA), we have obtained highpr...
We have conducted deep mid-infrared imaging of a relatively nearby sample of candidate Vega-like sta...
We report on high contrast near infrared ( ∼ 2.2 µm) observations of Vega ob-tained with the Palomar...
Vega may have a massive companion in a wide orbit, as evidenced by structure in its cold dust debris...
We report on infrared interferometric observations of Vega obtained in May and June 2005 with the FL...
Vega excess stars are main sequence stars which are surrounded by a cool dust disk, left as a remna...
Vega and Fomalhaut are similar in terms of mass, ages, and global debris disk properties; therefore,...
We present new observations of the Vega system with the Plateau de Bure Interferometer. The debris d...
We present the results of a deep high-contrast imaging search for planets around Vega. Vega is an id...
From adaptive optics observations with the Palomar 5 m telescope we place upper limits on the masses...
We report on high contrast near-infrared (~2.2 μm) observations of Vega obtained with the Palomar Fi...
Using the FLUOR near-infrared beam combiner installed at the CHARA Array (Mt Wilson, CA), we have ob...
Context. Gaps in circumstellar disks can signal the existence of planetary perturbers, making such s...
Context: Only a handful of debris disks have been imaged up to now. Due to the need for high dynamic...
Stars with debris disks are intriguing targets for direct-imaging exoplanet searches, owing both to ...
Using the FLUOR beam-combiner installed at the CHARA Array (Mt. Wilson, CA), we have obtained highpr...
We have conducted deep mid-infrared imaging of a relatively nearby sample of candidate Vega-like sta...
We report on high contrast near infrared ( ∼ 2.2 µm) observations of Vega ob-tained with the Palomar...
Vega may have a massive companion in a wide orbit, as evidenced by structure in its cold dust debris...
We report on infrared interferometric observations of Vega obtained in May and June 2005 with the FL...
Vega excess stars are main sequence stars which are surrounded by a cool dust disk, left as a remna...
Vega and Fomalhaut are similar in terms of mass, ages, and global debris disk properties; therefore,...
We present new observations of the Vega system with the Plateau de Bure Interferometer. The debris d...