Search Results - "Theissen, Christopher"
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Parallaxes of Cool Objects with WISE: Filling in for Gaia
Published in The Astrophysical journal (01-08-2018)“…This paper uses the multi-epoch astrometry from the Wide-field Infrared Survey Explorer (WISE) to demonstrate a method to measure proper motions and…”
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Early Time Spectropolarimetry of the Aspherical Type II Supernova SN 2023ixf
Published in Astrophysical journal. Letters (01-10-2023)“…Abstract We present six epochs of optical spectropolarimetry of the Type II supernova (SN) 2023ixf ranging from ∼2 to 15 days after the explosion. Polarimetry…”
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Discovery of the Exceptionally Short Period Ultracool Dwarf Binary LP 413-53AB
Published in Astrophysical journal. Letters (01-03-2023)“…Abstract We report the detection of large-amplitude, rapid radial velocity (RV) variations and line-splitting in high-resolution Keck/NIRSPEC spectra of the M9…”
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Assessing the C/O Ratio Formation Diagnostic: A Potential Trend with Companion Mass
Published in The Astronomical journal (01-09-2023)“…Abstract The carbon-to-oxygen (C/O) ratio in an exoplanet atmosphere has been suggested as a potential diagnostic of planet formation. Now that a number of…”
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The 3D Kinematics of the Orion Nebula Cluster: NIRSPEC-AO Radial Velocities of the Core Population
Published in The Astrophysical journal (01-02-2022)“…Abstract The kinematics and dynamics of stellar and substellar populations within young, still-forming clusters provide valuable information for constraining…”
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The 3D Kinematics of the Orion Nebula Cluster. II. Mass-dependent Kinematics of the Inner Cluster
Published in The Astrophysical journal (01-02-2024)“…Abstract We present the kinematic analysis of 246 stars within 4 ′ from the center of Orion Nebula Cluster (ONC), the closest massive star cluster with active…”
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WARM DUST AROUND COOL STARS: FIELD M DWARFS WITH WISE 12 OR 22 μm EXCESS EMISSION
Published in The Astrophysical journal (20-10-2014)“…Using the Sloan Digital Sky Survey Data Release 7 (SDSS DR7) spectroscopic catalog, we searched the WISE AllWISE catalog to investigate the occurrence of warm…”
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Astrometric Accelerations as Dynamical Beacons: A Giant Planet Imaged inside the Debris Disk of the Young Star AF Lep
Published in Astrophysical journal. Letters (01-06-2023)“…Abstract We present the direct-imaging discovery of a giant planet orbiting the young star AF Lep, a 1.2 M ⊙ member of the 24 ± 3 Myr β Pic moving group. AF…”
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The Ultracool SpeXtroscopic Survey. I. Volume-limited Spectroscopic Sample and Luminosity Function of M7−L5 Ultracool Dwarfs
Published in The Astrophysical journal (01-10-2019)“…We present a volume-limited, spectroscopically verified sample of M7−L5 ultracool dwarfs (UCDs) within 25 pc. The sample contains 410 sources, of which 93%…”
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The Brown Dwarf Kinematics Project (BDKP). VI. Ultracool Dwarf Radial and Rotational Velocities from SDSS/APOGEE High-resolution Spectroscopy
Published in The Astrophysical journal. Supplement series (01-10-2024)“…Abstract We present precise measurements of radial (RV) and projected rotational ( v sin i ) velocities of a sample of 258 M6 to L2 dwarfs with multiepoch,…”
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Moderate-resolution K-band Spectroscopy of the Substellar Companion VHS 1256 b
Published in The Astronomical journal (01-10-2022)“…Abstract We present moderate-resolution ( R ∼ 4000) K -band spectra of the planetary-mass companion VHS 1256 b. The data were taken with the OSIRIS integral…”
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JWST-TST High Contrast: Spectroscopic Characterization of the Benchmark Brown Dwarf HD 19467 B with the NIRSpec Integral Field Spectrograph
Published in The Astronomical journal (01-10-2024)“…Abstract We present the atmospheric characterization of the substellar companion HD 19467 B as part of the pioneering James Webb Space Telescope Guaranteed…”
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Multiple Patchy Cloud Layers in the Planetary-mass Object SIMP 0136+0933
Published in The Astrophysical journal (01-04-2024)“…Abstract Multiwavelength photometry of brown dwarfs and planetary-mass objects provides insight into their atmospheres and cloud layers. We present…”
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Beyond the Local Volume. I. Surface Densities of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
Published in The Astrophysical journal (01-01-2022)“…Abstract Ultracool dwarf stars and brown dwarfs provide a unique probe of large-scale Galactic structure and evolution; however, until recently spectroscopic…”
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89 New Ultracool Dwarf Comoving Companions Identified with the Backyard Worlds: Planet 9 Citizen Science Project
Published in The Astronomical journal (01-06-2024)“…Abstract We report the identification of 89 new systems containing ultracool dwarf companions to main-sequence stars and white dwarfs, using the citizen…”
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Beyond the Local Volume. II. Population Scaleheights and Ages of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
Published in The Astrophysical journal (01-07-2022)“…Abstract Ultracool dwarfs (UCDs) represent a significant proportion of stars in the Milky Way, and deep samples of these sources have the potential to…”
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Discovery of a Hypervelocity L Subdwarf at the Star/Brown Dwarf Mass Limit
Published in Astrophysical journal. Letters (01-08-2024)“…Abstract We report the discovery of a high-velocity, very low-mass star or brown dwarf whose kinematics suggest it is unbound to the Milky Way. CWISE…”
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RUNAWAY M DWARF CANDIDATES FROM THE SLOAN DIGITAL SKY SURVEY
Published in The Astrophysical journal (01-11-2015)“…ABSTRACT We present a sample of 20 runaway M dwarf candidates (RdMs) within 1 kpc of the Sun whose Galactocentric (GC) velocities exceed 400 km s−1. The…”
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A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9
Published in The Astrophysical journal (01-12-2021)“…Abstract Through the Backyard Worlds: Planet 9 citizen science project we discovered a late-type L dwarf co-moving with the young K0 star BD+60 1417 at a…”
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2MASS J11151597+1937266: A Young, Dusty, Isolated, Planetary-mass Object with a Potential Wide Stellar Companion
Published in The Astrophysical journal (20-01-2018)“…We present 2MASS J11151597+1937266, a recently identified low-surface-gravity L dwarf, classified as an L2γ based on Sloan Digital Sky Survey optical…”
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