Search Publications

On the degree of dynamical packing in the Kepler multiplanet systems
DOI: 10.1093/mnras/stad1921 Bibcode: 2023MNRAS.526.2118O

Tamayo, Daniel; Obertas, Alysa; Murray, Norm

Current planet formation theories rely on initially compact orbital configurations undergoing a (possibly extended) phase of giant impacts following the dispersal of the dissipative protoplanetary disc. The orbital architectures of observed mature exoplanet systems have likely been strongly sculpted by chaotic dynamics, instabilities, and giant im…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 9
Lyα Scattering Models Trace Accretion and Outflow Kinematics in T Tauri Systems
DOI: 10.3847/1538-4357/acaf70 Bibcode: 2023ApJ...944..185A

Herczeg, Gregory J.; France, Kevin; Ábrahám, Péter +18 more

T Tauri stars produce broad Lyα emission lines that contribute ~88% of the total UV flux incident on the inner circumstellar disks. Lyα photons are generated at the accretion shocks and in the protostellar chromospheres and must travel through accretion flows, winds, and jets, the protoplanetary disks, and the interstellar medium before reaching t…

2023 The Astrophysical Journal
Herschel eHST 9
New Generation Stellar Spectral Libraries in the Optical and Near-infrared. I. The Recalibrated UVES-POP Library for Stellar Population Synthesis
DOI: 10.3847/1538-4365/acc321 Bibcode: 2023ApJS..266...11B

Afanasiev, Anton V.; Chilingarian, Igor V.; Melo, Claudio +8 more

We present reprocessed flux-calibrated spectra of 406 stars from the UVES-POP stellar library in the wavelength range 320-1025 nm, which can be used for stellar population synthesis. The spectra are provided in the two versions having spectral resolving power R = 20,000 and R = 80,000. Raw spectra from the ESO data archive were re-reduced using th…

2023 The Astrophysical Journal Supplement Series
Gaia 9
Star cluster classification using deep transfer learning with PHANGS-HST
DOI: 10.1093/mnras/stad2238 Bibcode: 2023MNRAS.526.2991H

Mobasher, Bahram; Kruijssen, J. M. Diederik; Chevance, Mélanie +17 more

Currently available star cluster catalogues from the Hubble Space Telescope (HST) imaging of nearby galaxies heavily rely on visual inspection and classification of candidate clusters. The time-consuming nature of this process has limited the production of reliable catalogues and thus also post-observation analysis. To address this problem, deep t…

2023 Monthly Notices of the Royal Astronomical Society
eHST 9
Pixelated Reconstruction of Foreground Density and Background Surface Brightness in Gravitational Lensing Systems Using Recurrent Inference Machines
DOI: 10.3847/1538-4357/accf84 Bibcode: 2023ApJ...951....6A

Hezaveh, Yashar; Adam, Alexandre; Perreault-Levasseur, Laurence +1 more

Modeling strong gravitational lenses in order to quantify distortions in the images of background sources and to reconstruct the mass density in foreground lenses has been a difficult computational challenge. As the quality of gravitational lens images increases, the task of fully exploiting the information they contain becomes computationally and…

2023 The Astrophysical Journal
eHST 9
Saturn's atmospheric response to the large influx of ring material inferred from Cassini INMS measurements
DOI: 10.1016/j.icarus.2022.115328 Bibcode: 2023Icar..39115328M

Fletcher, Leigh N.; Guerlet, Sandrine; Moses, Julianne I. +12 more

During the Grand Finale stage of the Cassini mission, organic-rich ring material was discovered to be flowing into Saturn's equatorial upper atmosphere at a surprisingly large rate. Through a series of photochemical models, we have examined the consequences of this ring material on the chemistry of Saturn's neutral and ionized atmosphere. We find …

2023 Icarus
Cassini 9
A Large-scale Kinematic Study of Molecular Gas in High-z Cluster Galaxies: Evidence for High Levels of Kinematic Asymmetry
DOI: 10.3847/1538-4357/acae96 Bibcode: 2023ApJ...944..213C

Cooper, M. C.; Clements, D. L.; van Kampen, E. +14 more

We investigate the resolved kinematics of the molecular gas, as traced by the Atacama Large Millimeter/submillimeter Array in CO (2-1), of 25 cluster member galaxies across three different clusters at a redshift of z ~ 1.6. This is the first large-scale analysis of the molecular gas kinematics of cluster galaxies at this redshift. By separately es…

2023 The Astrophysical Journal
eHST 9
SN 2021fxy: mid-ultraviolet flux suppression is a common feature of Type Ia supernovae
DOI: 10.1093/mnras/stad1171 Bibcode: 2023MNRAS.522.3481D

Lundqvist, P.; Suntzeff, N. B.; Wang, L. +26 more

We present ultraviolet (UV) to near-infrared (NIR) observations and analysis of the nearby Type Ia supernova SN 2021fxy. Our observations include UV photometry from Swift/UVOT, UV spectroscopy from HST/STIS, and high-cadence optical photometry with the Swope 1-m telescope capturing intranight rises during the early light curve. Early B - V colours…

2023 Monthly Notices of the Royal Astronomical Society
eHST 9
Tilt-to-length coupling in LISA Pathfinder: A data analysis
DOI: 10.1103/PhysRevD.108.102003 Bibcode: 2023PhRvD.108j2003A

Mendes, L.; Russano, G.; Sanjuan, J. +76 more

We present a study of the tilt-to-length coupling noise during the LISA Pathfinder mission and how it depended on the system's alignment. Tilt-to-length coupling noise is the unwanted coupling of angular and lateral spacecraft or test mass motion into the primary interferometric displacement readout. It was one of the major noise sources in the LI…

2023 Physical Review D
LISAPathfinder 9
Stability and Detectability of Exomoons Orbiting HIP 41378 f, a Temperate Jovian Planet with an Anomalously Low Apparent Density
DOI: 10.3847/1538-3881/ad011c Bibcode: 2023AJ....166..208H

Vanderburg, Andrew; Kirk, James; López-Morales, Mercedes +21 more

Moons orbiting exoplanets ("exomoons") may hold clues about planet formation, migration, and habitability. In this work, we investigate the plausibility of exomoons orbiting the temperate (T eq = 294 K) giant (R = 9.2 R ) planet HIP 41378 f, which has been shown to have a low apparent bulk density of 0.09 g cm-3 a…

2023 The Astronomical Journal
eHST 9