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20142026
most cited Pictoris' inner disk in polarized light and new orbital parameters for Pictoris b

131 citations · 1.1k across the 67 of their papers we have counts for

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23 papers · 1 filter

astro-ph.EP2024

The Keck-HGCA Pilot Survey II: Direct Imaging Discovery of HD 63754 B, a ~20 au Massive Companion Near the Hydrogen Burning Limit

Yiting Li, Timothy D. Brandt, Kyle Franson +15

We present the joint astrometric and direct imaging discovery, mass measurement, and orbital analysis of HD 63754 B (HIP 38216 B), a companion near the stellar-substellar boundary…

astro-ph.EP2024

Subaru/CHARIS High-Resolution Mode Spectroscopy of the Brown Dwarf Companion HD 33632 Ab

Aidan Gibbs, Briley Lewis, Michael Fitzgerald +6

Brown dwarfs (BD) are model degenerate in age and mass. High-contrast imaging and spectroscopy of BD companions to host stars where the mass and age can be independently constraine…

astro-ph.EP2023

A Wolf 359 in sheep's clothing: Hunting for substellar companions in the fifth-closest system using combined high-contrast imaging and radial velocity analysis

Rachel Bowens-Rubin, Joseph M. Akana Murphy, Philip M. Hinz +16

Wolf 359 (CN Leo, GJ 406, Gaia DR3 3864972938605115520) is a low-mass star in the fifth-closest neighboring system (2.41 pc). Because of its relative youth and proximity, Wolf 359…

astro-ph.EP2023★ 74 cited

Astrometric Accelerations as Dynamical Beacons: A Giant Planet Imaged Inside the Debris Disk of the Young Star AF Lep

Kyle Franson, Brendan P. Bowler, Yifan Zhou +13

We present the direct imaging discovery of a giant planet orbiting the young star AF Lep, a 1.2 member of the 24 3 Myr Pic moving group. AF Lep was observed a…

astro-ph.EP2022

Battle of the Predictive Wavefront Controls: Comparing Data and Model-Driven Predictive Control for High Contrast Imaging

J. Fowler, Maaike A. M. Van Kooten, Rebecca Jensen-Clem

Ground-based high contrast exoplanet imaging requires state-of-the-art adaptive optics (AO) systems in order to detect extremely faint planets next to their brighter host stars. Fo…

astro-ph.EP2021★ 2 cited

Precise Masses and Orbits for Nine Radial Velocity Exoplanets

Yiting Li, Timothy D. Brandt, G. Mirek Brandt +6

Radial velocity (RV) surveys have discovered hundreds of exoplanetary systems but suffer from a fundamental degeneracy between planet mass and orbital inclination . In thi…

astro-ph.EP2021

The Bright Pyramid Wavefront Sensor

Benjamin L. Gerard, Vincent Chambouleyron, Rebecca Jensen-Clem +1

Extreme adaptive optics (AO) is crucial for enabling the contrasts needed for ground-based high contrast imaging instruments to detect exoplanets. Pushing exoplanet imaging detecti…

astro-ph.EP2021★ 65 cited

A survey of the linear polarization of directly imaged exoplanets and brown dwarf companions with SPHERE-IRDIS. First polarimetric detections revealing disks around DH Tau B and GSC 6214-210 B

R. G. van Holstein, T. Stolker, R. Jensen-Clem +22

Young giant planets and brown dwarf companions emit near-infrared radiation that can be linearly polarized up to several percent. This polarization can reveal the presence of a cir…

astro-ph.EP2020★ 6 cited

Early High-contrast Imaging Results with Keck/NIRC2-PWFS: The SR 21 Disk

Taichi Uyama, Bin Ren, Dimitri Mawet +22

High-contrast imaging of exoplanets and protoplanetary disks depends on wavefront sensing and correction made by adaptive optics instruments. Classically, wavefront sensing has bee…

astro-ph.EP2020★ 84 cited

Keck/NIRC2 '-Band Imaging of Jovian-Mass Accreting Protoplanets around PDS 70

Jason J. Wang, Sivan Ginzburg, Bin Ren +42

We present '-band imaging of the PDS 70 planetary system with Keck/NIRC2 using the new infrared pyramid wavefront sensor. We detected both PDS 70 b and c in our images, as well…

astro-ph.EP2019★ 4 cited

A Hot Saturn Near (but unassociated with) the Open Cluster NGC 1817

Rayna Rampalli, Andrew Vanderburg, Allyson Bieryla +14

We report on the discovery of a hot Saturn-sized planet (9.916 +/- 0.985 R_earth) around a late F star, EPIC 246865365, observed in Campaign 13 of the K2 mission. We began studying…

astro-ph.EP2019★ 11 cited

The Need for Laboratory Measurements and Ab Initio Studies to Aid Understanding of Exoplanetary Atmospheres

Jonathan J. Fortney, Tyler D. Robinson, Shawn Domagal-Goldman +85

We are now on a clear trajectory for improvements in exoplanet observations that will revolutionize our ability to characterize their atmospheric structure, composition, and circul…

astro-ph.EP2019

The Demographics and Atmospheres of Giant Planets with the ELTs

Brendan Bowler, Steph Sallum, Alan Boss +23

Gas giants are the most readily detectable exoplanets but fundamental questions about their system architectures, formation, migration, and atmospheres have been unanswerable with…

astro-ph.EP2018★ 69 cited

Deep exploration of Eridani with Keck Ms-band vortex coronagraphy and radial velocities: mass and orbital parameters of the giant exoplanet

Dimitri Mawet, Lea Hirsch, Eve J. Lee +27

We present the most sensitive direct imaging and radial velocity (RV) exploration of Eridani to date. Eridani is an adolescent planetary system, reminiscent of the early So…

astro-ph.EP2018★ 40 cited

Robo-AO Kepler Survey V: The effect of physically associated stellar companions on planetary systems

Carl Ziegler, Nicholas M. Law, Christoph Baranec +7

The Kepler light curves used to detect thousands of planetary candidates are susceptible to dilution due to blending with previously unknown nearby stars. With the automated laser…

astro-ph.EP2017★ 46 cited

Robo-AO Kepler Survey IV: the effect of nearby stars on 3857 planetary candidate systems

Carl Ziegler, Nicholas M. Law, Christoph Baranec +7

We present the overall statistical results from the Robo-AO Kepler planetary candidate survey, comprising of 3857 high-angular resolution observations of planetary candidate system…

astro-ph.EP2017★ 48 cited

Deep imaging search for planets forming in the TW Hya protoplanetary disk with the Keck/NIRC2 vortex coronagraph

G. Ruane, D. Mawet, J. Kastner +10

Distinct gap features in the nearest protoplanetary disk, TW Hya (distance of 59.50.9 pc), may be signposts of ongoing planet formation. We performed long-exposure thermal inf…

astro-ph.EP2017★ 40 cited

Evidence that the Directly-Imaged Planet HD 131399 Ab is a Background Star

Eric L. Nielsen, Robert J. De Rosa, Julien Rameau +55

We present evidence that the recently discovered, directly-imaged planet HD 131399 Ab is a background star with non-zero proper motion. From new JHK1L' photometry and spectroscopy…

astro-ph.EP2016★ 27 cited

Ultra Short Period Planets in K2 with companions: a double transiting system for EPIC 220674823

Elisabeth R. Adams, Brian Jackson, Michael Endl +10

Two transiting planets have been identified orbiting K2 target EPIC 220674823. One object is an ultra-short-period planet (USP) with a period of just 0.57 days (13.7 hours), while…

astro-ph.EP2016★ 67 cited

Two Small Planets Transiting HD 3167

Andrew Vanderburg, Allyson Bieryla, Dmitry A. Duev +10

We report the discovery of two super-Earth-sized planets transiting the bright (V = 8.94, K = 7.07) nearby late G-dwarf HD 3167, using data collected by the K2 mission. The inner p…

astro-ph.EP2016★ 70 cited

Five Planets Transiting a Ninth Magnitude Star

Andrew Vanderburg, Juliette C. Becker, Martti H. Kristiansen +15

The Kepler mission has revealed a great diversity of planetary systems and architectures, but most of the planets discovered by Kepler orbit faint stars. Using new data from the K2…

astro-ph.EP2016★ 33 cited

Point Source Polarimetry with the Gemini Planet Imager: Sensitivity Characterization with T5.5 Dwarf Companion HD 19467 B

Rebecca Jensen-Clem, Max Millar-Blanchaer, Dimitri Mawet +12

Detecting polarized light from self-luminous exoplanets has the potential to provide key information about rotation, surface gravity, cloud grain size, and cloud coverage. While fi…

astro-ph.EP2015★ 131 cited

Pictoris' inner disk in polarized light and new orbital parameters for Pictoris b

Maxwell A. Millar-Blanchaer, James R. Graham, Laurent Pueyo +54

We present -band observations of Pic with the Gemini Planet Imager's (GPI's) polarimetry mode that reveal the debris disk between ~0.3" (~6 AU) and ~1.7" (~33 AU), while sim…