Search Publications

Obliquity Constraints on an Extrasolar Planetary-mass Companion
DOI: 10.3847/1538-3881/ab76c6 Bibcode: 2020AJ....159..181B

Knutson, Heather A.; Morley, Caroline V.; Bowler, Brendan P. +8 more

We place the first constraints on the obliquity of a planetary-mass companion outside of the solar system. Our target is the directly imaged system 2MASS J01225093-2439505 (2M0122), which consists of a 120 Myr 0.4 M star hosting a 12-27 MJ companion at 50 au. We constrain all three of the system's angular-momentum vectors: h…

2020 The Astronomical Journal
Gaia eHST 52
Spectral Variability of VHS J1256-1257b from 1 to 5 µm
DOI: 10.3847/1538-3881/ab9e04 Bibcode: 2020AJ....160...77Z

Kataria, Tiffany; Apai, Dániel; Zhou, Yifan +4 more

Multiwavelength time-resolved observations of rotationally modulated variability from brown dwarfs and giant exoplanets are the most effective method for constraining their heterogeneous atmospheric structures. In a companion paper, we reported the discovery of strong near-infrared variability in HST/WFC3/G141 light curves of the very red L-dwarf …

2020 The Astronomical Journal
eHST 51
An Extreme-precision Radial-velocity Pipeline: First Radial Velocities from EXPRES
DOI: 10.3847/1538-3881/ab7e31 Bibcode: 2020AJ....159..187P

Ong, J. M. Joel; Fischer, Debra A.; Buchhave, Lars A. +13 more

The EXtreme-PREcision Spectrograph (EXPRES) is an environmentally stabilized, fiber-fed, R = 137,500, optical spectrograph. It was recently commissioned at the 4.3 m Lowell Discovery Telescope near Flagstaff, Arizona. The spectrograph was designed with a target radial-velocity (RV) precision of 30 cm s-1. In addition to instrumental inn…

2020 The Astronomical Journal
Gaia 50
Two Views of the Radius Gap and the Role of Light Curve Fitting
DOI: 10.3847/1538-3881/ab9fff Bibcode: 2020AJ....160...89P

Petigura, Erik A.

Recently, several groups have resolved a gap that bifurcates planets between the size of Earth and Neptune into two populations. The location and depth of this feature is an important signature of the physical processes that form and sculpt planets. In particular, planets residing in the radius gap are valuable probes of these processes as they ma…

2020 The Astronomical Journal
Gaia 50
Performance Verification of the EXtreme PREcision Spectrograph
DOI: 10.3847/1538-3881/ab811d Bibcode: 2020AJ....159..238B

Ong, J. M. Joel; Fischer, Debra A.; Buchhave, Lars A. +22 more

The EXtreme PREcision Spectrograph (EXPRES) is a new Doppler spectrograph designed to reach a radial-velocity measurement precision sufficient to detect Earth-like exoplanets orbiting nearby, bright stars. We report on extensive laboratory testing and on-sky observations to quantitatively assess the instrumental radial-velocity measurement precisi…

2020 The Astronomical Journal
Gaia 49
Revisiting MOA 2013-BLG-220L: A Solar-type Star with a Cold Super-Jupiter Companion
DOI: 10.3847/1538-3881/aba2d3 Bibcode: 2020AJ....160..121V

Cole, Andrew A.; Beaulieu, Jean-Philippe; Bond, Ian A. +7 more

We present the analysis of high-resolution images of MOA-2013-BLG-220, taken with the Keck adaptive optics system six years after the initial observation, identifying the lens as a solar-type star hosting a super-Jupiter-mass planet. The masses of planets and host stars discovered by microlensing are often not determined from light-curve data, whi…

2020 The Astronomical Journal
Gaia 47
Exploring the Evolution of Stellar Rotation Using Galactic Kinematics
DOI: 10.3847/1538-3881/ab91b2 Bibcode: 2020AJ....160...90A

Angus, Ruth; Foreman-Mackey, Daniel; van Saders, Jennifer +9 more

The rotational evolution of cool dwarfs is poorly constrained after ∼1-2 Gyr due to a lack of precise ages and rotation periods for old main-sequence stars. In this work, we use velocity dispersion as an age proxy to reveal the temperature-dependent rotational evolution of low-mass Kepler dwarfs and demonstrate that kinematic ages could be a usefu…

2020 The Astronomical Journal
Gaia 46
Into the UV: A Precise Transmission Spectrum of HAT-P-41b Using Hubble's WFC3/UVIS G280 Grism
DOI: 10.3847/1538-3881/ab7b78 Bibcode: 2020AJ....159..204W

Wakeford, H. R.; Sing, D. K.; Nikolov, N. +8 more

The ultraviolet-visible wavelength range holds critical spectral diagnostics for the chemistry and physics at work in planetary atmospheres. To date, time-series studies of exoplanets to characterize their atmospheres have relied on several combinations of modes on the Hubble Space Telescope's STIS/COS instruments to access this wavelength regime.…

2020 The Astronomical Journal
eHST 45
The First Habitable-zone Earth-sized Planet from TESS. II. Spitzer Confirms TOI-700 d
DOI: 10.3847/1538-3881/aba4b3 Bibcode: 2020AJ....160..117R

Barclay, Thomas; Vanderburg, Andrew; Latham, David W. +43 more

We present Spitzer 4.5 µm observations of the transit of TOI-700 d, a habitable-zone Earth-sized planet in a multiplanet system transiting a nearby M-dwarf star (TIC 150428135, 2MASS J06282325-6534456). TOI-700 d has a radius of ${1.144}_{-0.061}^{+0.062}{R}_{\oplus }$ and orbits within its host star's conservative habitable zone with a peri…

2020 The Astronomical Journal
Gaia 45
The Dynamics of Interstellar Asteroids and Comets within the Galaxy: An Assessment of Local Candidate Source Regions for 1I/'Oumuamua and 2I/Borisov
DOI: 10.3847/1538-3881/ab7336 Bibcode: 2020AJ....159..147H

Hallatt, Tim; Wiegert, Paul

The low velocity of interstellar asteroid 1I/'Oumuamua with respect to our galaxy's local standard of rest implies that it is young. Adopting the young age hypothesis, we assess possible origin systems for this interstellar asteroid and for 2I/Borisov, though the latter's higher speed means it is unlikely to be young. First, their past trajectorie…

2020 The Astronomical Journal
Gaia 45