Search Publications

Split Peas in a Pod: Intra-system Uniformity of Super-Earths and Sub-Neptunes
DOI: 10.3847/2041-8213/ac2c77 Bibcode: 2021ApJ...920L..34M

Winn, Joshua N.; Millholland, Sarah C.

The planets within compact multiplanet systems tend to have similar sizes, masses, and orbital period ratios, like "peas in a pod." This pattern was detected when considering planets with radii between 1 and 4 R. However, these same planets show a bimodal radius distribution, with few planets between 1.5 and 2 R. The smalle…

2021 The Astrophysical Journal
Gaia 28
htof: A New Open-source Tool for Analyzing Hipparcos, Gaia, and Future Astrometric Missions
DOI: 10.3847/1538-3881/ac12d0 Bibcode: 2021AJ....162..230B

Dupuy, Trent J.; Brandt, Timothy D.; Li, Yiting +3 more

We present htof, an open-source tool for interpreting and fitting the intermediate astrometric data (IAD) from both the 1997 and 2007 reductions of Hipparcos, the scanning law of Gaia, and future missions such as the Nancy Grace Roman Space Telescope (NGRST). htof solves the astrometric parameters of any system for any arbitrary combination of abs…

2021 The Astronomical Journal
Gaia Hipparcos 28
Warm Jupiters in TESS Full-frame Images: A Catalog and Observed Eccentricity Distribution for Year 1
DOI: 10.3847/1538-4365/abf73c Bibcode: 2021ApJS..255....6D

Hellier, Coel; Triaud, Amaury H. M. J.; Latham, David W. +57 more

Warm Jupiters-defined here as planets larger than 6 Earth radii with orbital periods of 8-200 days-are a key missing piece in our understanding of how planetary systems form and evolve. It is currently debated whether Warm Jupiters form in situ, undergo disk or high-eccentricity tidal migration, or have a mixture of origin channels. These differen…

2021 The Astrophysical Journal Supplement Series
Gaia 28
KIC 5950759: a high-amplitude δ Sct star with amplitude and frequency modulation near the terminal age main sequence
DOI: 10.1093/mnras/stab1124 Bibcode: 2021MNRAS.504.4039B

Bowman, D. M.; Smalley, B.; Tkachenko, A. +5 more

Among the intermediate mass pulsating stars known as δ Sct stars is a subset of high-amplitude and predominantly radial-mode pulsators known as high-amplitude δ Sct (HADS) stars. From more than 2000 δ Sct stars observed by the Kepler space mission, only two HADS stars were detected. We investigate the more perplexing of these two HADS stars, KIC 5…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 28
A New Sample of Warm Extreme Debris Disks from the ALLWISE Catalog
DOI: 10.3847/1538-4357/abdc26 Bibcode: 2021ApJ...910...27M

Henning, Thomas; Pál, András; Kinemuchi, Karen +12 more

Extreme debris disks (EDDs) are rare systems with peculiarly large amounts of warm dust that may stem from recent giant impacts between planetary embryos during the final phases of terrestrial planet growth. Here we report on the identification and characterization of six new EDDs. These disks surround F5-G9 type main-sequence stars with ages >…

2021 The Astrophysical Journal
AKARI Gaia Herschel 28
Faint objects in motion: the new frontier of high precision astrometry
DOI: 10.1007/s10686-021-09781-1 Bibcode: 2021ExA....51..845M

Villaver, Eva; Alves, João; Chemin, Laurent +83 more

Sky survey telescopes and powerful targeted telescopes play complementary roles in astronomy. In order to investigate the nature and characteristics of the motions of very faint objects, a flexibly-pointed instrument capable of high astrometric accuracy is an ideal complement to current astrometric surveys and a unique tool for precision astrophys…

2021 Experimental Astronomy
Gaia eHST 28
Cross-correlation of Planck CMB lensing with DESI-like LRGs
DOI: 10.1093/mnras/staa3927 Bibcode: 2021MNRAS.501.6181K

White, Martin; Kitanidis, Ellie

Cross-correlations between the lensing of the cosmic microwave background (CMB) and other tracers of large-scale structure provide a unique way to reconstruct the growth of dark matter, break degeneracies between cosmology and galaxy physics, and test theories of modified gravity. We detect a cross-correlation between Dark Energy Spectroscopic Ins…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 28
Molecular Line Observations in Two Dusty Star-forming Galaxies at z = 6.9
DOI: 10.3847/1538-4357/ac21db Bibcode: 2021ApJ...921...97J

Greve, Thomas R.; Phadke, Kedar A.; Aravena, Manuel +18 more

SPT0311-58 is the most massive infrared luminous system discovered so far during the Epoch of Reionization (EoR). In this paper, we present a detailed analysis of the molecular interstellar medium at z = 6.9, through high resolution observations of the CO(6-5), CO(7-6), CO(10-9), [C I](2-1), and p-H2O(21,1 -20,2) l…

2021 The Astrophysical Journal
Herschel 28
Molecules with ALMA at Planet-forming Scales (MAPS). XVII. Determining the 2D Thermal Structure of the HD 163296 Disk
DOI: 10.3847/1538-4365/ac143f Bibcode: 2021ApJS..257...17C

Zhang, Ke; Wilner, David J.; Ménard, François +26 more

Understanding the temperature structure of protoplanetary disks is key to interpreting observations, predicting the physical and chemical evolution of the disk, and modeling planet formation processes. In this study, we constrain the two-dimensional thermal structure of the disk around the Herbig Ae star HD 163296. Using the thermochemical code RA…

2021 The Astrophysical Journal Supplement Series
Gaia Herschel 28
Stellar clustering and orbital architecture of planetary systems
DOI: 10.1051/0004-6361/202040201 Bibcode: 2021A&A...649A.111A

Adibekyan, V.; Sousa, S. G.; Barros, S. C. C. +9 more

Context. Revealing the mechanisms shaping the architecture of planetary systems is crucial for our understanding of their formation and evolution. In this context, it has been recently proposed that stellar clustering might be the key in shaping the orbital architecture of exoplanets.
Aims: The main goal of this work is to explore the factors…

2021 Astronomy and Astrophysics
Gaia 28