C. G. Tinney
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View article: HD 222237 b: a long-period super-Jupiter around a nearby star revealed by radial-velocity and <i>Hipparcos–Gaia</i> astrometry
HD 222237 b: a long-period super-Jupiter around a nearby star revealed by radial-velocity and <i>Hipparcos–Gaia</i> astrometry Open
Giant planets on long-period orbits around the nearest stars are among the easiest to directly image. Unfortunately these planets are difficult to fully constrain by indirect methods, e.g. transit and radial velocity (RV). In this study, w…
View article: Revised Architecture and Two New Super-Earths in the HD 134606 Planetary System
Revised Architecture and Two New Super-Earths in the HD 134606 Planetary System Open
Multiplanet systems exhibit a diversity of architectures that diverge from the solar system and contribute to the topic of exoplanet demographics. Radial velocity (RV) surveys form a crucial component of exoplanet surveys, as their long ob…
View article: The role of carbon in red giant spectro-seismology
The role of carbon in red giant spectro-seismology Open
Although red clump stars function as reliable standard candles, their surface characteristics (i.e. Teff, log g, and [Fe/H]) overlap with those of red giant branch stars, which are not standard candles. Recent results have revealed that sp…
View article: 2MASS J09393548-2448279: the coolest and least luminous brown dwarf binary known?
2MASS J09393548-2448279: the coolest and least luminous brown dwarf binary known? Open
Measurement of the luminosity and atmospheric properties of the T8 brown dwarf 2MASS J09393548-2448279 are presented, based on Spitzer IRAC and IRS mid-infrared observations and IRIS2 ground-based astrometry. We determine log{sub 10} L{sub…
View article: Revised Architecture and Two New Super-Earths in the HD 134606 Planetary System
Revised Architecture and Two New Super-Earths in the HD 134606 Planetary System Open
Multi-planet systems exhibit a diversity of architectures that diverge from the solar system and contribute to the topic of exoplanet demographics. Radial velocity (RV) surveys form a crucial component of exoplanet surveys, as their long o…
View article: The role of carbon in red giant spectro-seismology
The role of carbon in red giant spectro-seismology Open
Although red clump stars function as reliable standard candles, their surface characteristics (i.e. $T_\text{eff}$, $\log g$, and [Fe/H]) overlap with those of red giant branch stars, which are not standard candles. Recent results have rev…
View article: SEARCHING for BINARY y DWARFS with the GEMINI MULTI-CONJUGATE ADAPTIVE OPTICS SYSTEM (GeMS)
SEARCHING for BINARY y DWARFS with the GEMINI MULTI-CONJUGATE ADAPTIVE OPTICS SYSTEM (GeMS) Open
The NASA Wide-field Infrared Survey Explorer (WISE) has discovered almost all the known members of the new class of Y-type brown dwarfs. Most of these Y dwarfs have been identified as isolated objects in the field. It is known that binarie…
View article: TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite
TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite Open
We present the discovery of two new 10 day period giant planets from the Transiting Exoplanet Survey Satellite mission, whose masses were precisely determined using a wide diversity of ground-based facilities. TOI-481 b and TOI-892 b have …
View article: Very regular high-frequency pulsation modes in young intermediate-mass stars
Very regular high-frequency pulsation modes in young intermediate-mass stars Open
Asteroseismology probes the internal structures of stars by using their natural pulsation frequencies1. It relies on identifying sequences of pulsation modes that can be compared with theoretical models, which has been done successfully fo…
View article: TOI-677b: A Warm Jupiter (P = 11.2 days) on an Eccentric Orbit Transiting a Late F-type Star
TOI-677b: A Warm Jupiter (P = 11.2 days) on an Eccentric Orbit Transiting a Late F-type Star Open
We report the discovery of TOI-677 b, first identified as a candidate in light curves obtained within Sectors 9 and 10 of the Transiting Exoplanet Survey Satellite (TESS) mission and confirmed with radial velocities. TOI-677 b has a mass o…
View article: KELT-25 b and KELT-26 b: A Hot Jupiter and a Substellar Companion Transiting Young A Stars Observed by TESS
KELT-25 b and KELT-26 b: A Hot Jupiter and a Substellar Companion Transiting Young A Stars Observed by TESS Open
We present the discoveries of KELT-25 b (TIC 65412605, TOI-626.01) and KELT-26 b (TIC 160708862, TOI-1337.01), two transiting companions orbiting relatively bright, early A stars. The transit signals were initially detected by the KELT sur…
View article: 76 T dwarfs from the UKIDSS LAS: Benchmarks, kinematics and an updated space density
76 T dwarfs from the UKIDSS LAS: Benchmarks, kinematics and an updated space density Open
We report the discovery of 76 new T dwarfs from the UKIRT Infrared Deep Sky Survey(UKIDSS) Large Area Survey (LAS). Near-infrared broad-and narrow-band photometry and spectroscopy are presented for the new objects, along withWide-field Inf…
View article: Spinning up a Daze: TESS Uncovers a Hot Jupiter Orbiting the Rapid Rotator TOI-778
Spinning up a Daze: TESS Uncovers a Hot Jupiter Orbiting the Rapid Rotator TOI-778 Open
NASA’s Transiting Exoplanet Survey Satellite (TESS) mission has been uncovering a growing number of exoplanets orbiting nearby, bright stars. Most exoplanets that have been discovered by TESS orbit narrow-line, slow-rotating stars, facilit…
View article: Doppler Constraints on Planetary Companions to Nearby Sun-like Stars: An Archival Radial Velocity Survey of Southern Targets for Proposed NASA Direct Imaging Missions*
Doppler Constraints on Planetary Companions to Nearby Sun-like Stars: An Archival Radial Velocity Survey of Southern Targets for Proposed NASA Direct Imaging Missions* Open
Directly imaging temperate rocky planets orbiting nearby, Sun-like stars with a 6 m class IR/O/UV space telescope, recently dubbed the Habitable Worlds Observatory, is a high-priority goal of the Astro2020 Decadal Survey. To prepare for fu…
View article: A sub-Neptune transiting the young field star HD 18599 at 40 pc
A sub-Neptune transiting the young field star HD 18599 at 40 pc Open
Transiting exoplanets orbiting young nearby stars are ideal laboratories for testing theories of planet formation and evolution. However, to date only a handful of stars with age <1 Gyr have been found to host transiting exoplanets. Her…
View article: Doppler Constraints on Planetary Companions to Nearby Sun-like Stars: An Archival Radial Velocity Survey of Southern Targets for Proposed NASA Direct Imaging Missions
Doppler Constraints on Planetary Companions to Nearby Sun-like Stars: An Archival Radial Velocity Survey of Southern Targets for Proposed NASA Direct Imaging Missions Open
Directly imaging temperate rocky planets orbiting nearby, Sun-like stars with a 6-m-class IR/O/UV space telescope, recently dubbed the Habitable Worlds Observatory, is a high priority goal of the Astro2020 Decadal Survey. To prepare for fu…
View article: TOI 560: Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS, and HIRES RVs
TOI 560: Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS, and HIRES RVs Open
We validate the presence of a two-planet system orbiting the 0.15–1.4 Gyr K4 dwarf TOI 560 (HD 73583). The system consists of an inner moderately eccentric transiting mini-Neptune (TOI 560 b, days, , …
View article: A sub-Neptune transiting the young field star HD 18599 at 40 pc
A sub-Neptune transiting the young field star HD 18599 at 40 pc Open
Transiting exoplanets orbiting young nearby stars are ideal laboratories for testing theories of planet formation and evolution. However, to date only a handful of stars with age <1 Gyr have been found to host transiting exoplanets. Here w…
View article: A dense mini-Neptune orbiting the bright young star HD 18599
A dense mini-Neptune orbiting the bright young star HD 18599 Open
Very little is known about the young planet population because the detection of small planets orbiting young stars is obscured by the effects of stellar activity and fast rotation, which mask planets within radial velocity and transit data…
View article: The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at ≈2 au
The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at ≈2 au Open
Gliese 86 is a nearby K dwarf hosting a giant planet on a ≈16 day orbit and an outer white dwarf companion on a ≈century-long orbit. In this study we combine radial velocity data (including new measurements spanning more than a decade) wit…
View article: 3D Selection of 167 Substellar Companions to Nearby Stars
3D Selection of 167 Substellar Companions to Nearby Stars Open
We analyze 5108 AFGKM stars with at least five high-precision radial velocity points, as well as Gaia and Hipparcos astrometric data, utilizing a novel pipeline developed in previous work. We find 914 radial velocity signals with periods l…
View article: Minerva-Australis. I. Design, Commissioning, and First Photometric Results
Minerva-Australis. I. Design, Commissioning, and First Photometric Results Open
© 2019. The Astronomical Society of the Pacific. All rights reserved. Printed in the U.S.A. The MINERVA-Australis telescope array is a facility dedicated to the follow-up, confirmation, characterization, and mass measurement of planets orb…
View article: FIESTA II. Disentangling Stellar and Instrumental Variability from Exoplanetary Doppler Shifts in the Fourier Domain
FIESTA II. Disentangling Stellar and Instrumental Variability from Exoplanetary Doppler Shifts in the Fourier Domain Open
The radial velocity (RV) detection of exoplanets is challenged by stellar spectroscopic variability that can mimic the presence of planets and by instrumental instability that can further obscure the detection. Both stellar and instrumenta…
View article: The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets
The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets Open
Hot Jupiters—short-period giant planets—were the first extrasolar planets to be discovered, but many questions about their origin remain. NASA’s Transiting Exoplanet Survey Satellite (TESS), an all-sky search for transiting planets, presen…
View article: HD 83443c: A Highly Eccentric Giant Planet on a 22 yr Orbit
HD 83443c: A Highly Eccentric Giant Planet on a 22 yr Orbit Open
We report the discovery of a highly eccentric long-period Jovian planet orbiting the hot-Jupiter host HD 83443. By combining radial velocity data from four instruments (AAT/UCLES, Keck/HIRES, HARPS, Minerva-Australis) spanning more than tw…
View article: HD 83443c: A highly eccentric giant planet on a 22-year orbit
HD 83443c: A highly eccentric giant planet on a 22-year orbit Open
We report the discovery of a highly eccentric long-period Jovian planet orbiting the hot-Jupiter host HD\,83443. By combining radial velocity data from four instruments (AAT/UCLES, Keck/HIRES, HARPS, Minerva-Australis) spanning more than t…
View article: The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at $\approx$2 AU
The Gliese 86 Binary System: A Warm Jupiter Formed in a Disk Truncated at $\approx$2 AU Open
Gliese 86 is a nearby K dwarf hosting a giant planet on a $\approx$16-day orbit and an outer white dwarf companion on a $\approx$century-long orbit. In this study we combine radial velocity data (including new measurements spanning more th…
View article: TESS Asteroseismology of α Mensae: Benchmark Ages for a G7 Dwarf and Its M Dwarf Companion
TESS Asteroseismology of α Mensae: Benchmark Ages for a G7 Dwarf and Its M Dwarf Companion Open
Asteroseismology of bright stars has become increasingly important as a method to determine the fundamental properties (in particular ages) of stars. The Kepler Space Telescope initiated a revolution by detecting oscillations in more than …
View article: Transits of Known Planets Orbiting a Naked-eye Star
Transits of Known Planets Orbiting a Naked-eye Star Open
Some of the most scientifically valuable transiting planets are those that were already known from radial velocity (RV) surveys. This is primarily because their orbits are well characterized and they preferentially orbit bright stars that …
View article: Cluster Difference Imaging Photometric Survey. II. TOI 837: A Young Validated Planet in IC 2602
Cluster Difference Imaging Photometric Survey. II. TOI 837: A Young Validated Planet in IC 2602 Open
© 2020. The American Astronomical Society. All rights reserved. We report the discovery of TOI 837b and its validation as a transiting planet. We characterize the system using data from the NASA Transiting Exoplanet Survey Satellite missio…