Search Publications

Broken into Pieces: ATLAS and Aliqa Uma as One Single Stream
DOI: 10.3847/1538-4357/abeb18 Bibcode: 2021ApJ...911..149L

Lewis, Geraint F.; Hattori, Kohei; Erkal, Denis +18 more

We present the first spectroscopic measurements of the ATLAS and Aliqa Uma streams from the Southern Stellar Stream Spectroscopic Survey (S5), in combination with the photometric data from the Dark Energy Survey and astrometric data from Gaia. From the coherence of spectroscopic members in radial velocity and proper motion, we find that…

2021 The Astrophysical Journal
Gaia 59
Convolutional neural network identification of galaxy post-mergers in UNIONS using IllustrisTNG
DOI: 10.1093/mnras/stab806 Bibcode: 2021MNRAS.504..372B

Ellison, Sara L.; Gwyn, Stephen; Hudson, Michael J. +6 more

The Canada-France Imaging Survey (CFIS) will consist of deep, high-resolution r-band imaging over ~5000 deg2 of the sky, representing a first-rate opportunity to identify recently merged galaxies. Because of the large number of galaxies in CFIS, we investigate the use of a convolutional neural network (CNN) for automated merger classifi…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 59
Spiral Arms and a Massive Dust Disk with Non-Keplerian Kinematics: Possible Evidence for Gravitational Instability in the Disk of Elias 2-27
DOI: 10.3847/1538-4357/abf243 Bibcode: 2021ApJ...914...88P

Lodato, G.; Pinte, C.; Testi, L. +16 more

To determine the origin of the spiral structure observed in the dust continuum emission of Elias 2-27 we analyze multiwavelength continuum ALMA data with a resolution of ~0"2 (~23 au) at 0.89, 1.3, and 3.3 mm. We also study the kinematics of the disk with 13CO and C18O ALMA observations in the J = 3-2 transition. The spiral a…

2021 The Astrophysical Journal
Gaia 59
A "Quick Look" at All-sky Galactic Archeology with TESS: 158,000 Oscillating Red Giants from the MIT Quick-look Pipeline
DOI: 10.3847/1538-4357/ac14b1 Bibcode: 2021ApJ...919..131H

Huber, Daniel; Sharma, Sanjib; Stello, Dennis +6 more

We present the first near all-sky yield of oscillating red giants from the prime mission data of NASA's Transiting Exoplanet Survey Satellite (TESS). We apply machine learning toward long-cadence TESS photometry from the first data release by the MIT Quick-look Pipeline to automatically detect the presence of red giant oscillations in frequency po…

2021 The Astrophysical Journal
Gaia 59
3D simulations of photochemical hazes in the atmosphere of hot Jupiter HD 189733b
DOI: 10.1093/mnras/stab1053 Bibcode: 2021MNRAS.504.2783S

Showman, Adam P.; Zhang, Xi; Tan, Xianyu +3 more

Photochemical hazes have been suggested as candidate for the high-altitude aerosols observed in the transmission spectra of many hot Jupiters. We present 3D simulations of the hot Jupiter HD 189733b to study how photochemical hazes are transported by atmospheric circulation. The model includes spherical, constant-size haze particles that gravitati…

2021 Monthly Notices of the Royal Astronomical Society
eHST 59
Multiwavelength continuum sizes of protoplanetary discs: scaling relations and implications for grain growth and radial drift
DOI: 10.1093/mnras/stab1808 Bibcode: 2021MNRAS.506.2804T

Testi, L.; Tazzari, M.; Natta, A. +5 more

We analyse spatially resolved ALMA observations at 0.9, 1.3, and 3.1 mm for the 26 brightest protoplanetary discs in the Lupus star-forming region. We characterize the discs multiwavelength brightness profiles by fitting the interferometric visibilities in a homogeneous way, obtaining effective disc sizes at the three wavelengths, spectral index p…

2021 Monthly Notices of the Royal Astronomical Society
Gaia 59
INTEGRAL x-ray constraints on sub-GeV dark matter
DOI: 10.1103/PhysRevD.103.063022 Bibcode: 2021PhRvD.103f3022C

Pinetti, Elena; Fornengo, Nicolao; Cirelli, Marco +1 more

Light dark matter (DM), defined here as having a mass between 1 MeV and about 1 GeV, is an interesting possibility both theoretically and phenomenologically, at one of the frontiers of current progress in the field of DM searches. Its indirect detection via gamma rays is challenged by the scarcity of experiments in the MeV-GeV region. We look ther…

2021 Physical Review D
INTEGRAL 59
Star formation and nuclear activity in luminous infrared galaxies: an infrared through radio review
DOI: 10.1007/s00159-020-00128-x Bibcode: 2021A&ARv..29....2P

Aalto, Susanne; Alonso-Herrero, Almudena; Mattila, Seppo +2 more

Nearby galaxies offer unique laboratories allowing multi-wavelength spatially resolved studies of the interstellar medium, star formation and nuclear activity across a broad range of physical conditions. In particular, detailed studies of individual local luminous infrared galaxies (LIRGs) are crucial for gaining a better understanding of these pr…

2021 Astronomy and Astrophysics Review
Herschel eHST 59
Milky Way Mid-Infrared Spitzer Spectroscopic Extinction Curves: Continuum and Silicate Features
DOI: 10.3847/1538-4357/ac00b7 Bibcode: 2021ApJ...916...33G

Gordon, Karl D.; Hines, Dean C.; Bouwman, Jeroen +7 more

We measured the mid-infrared (MIR) extinction using Spitzer photometry and spectroscopy (3.6-37 µm) for a sample of Milky Way sight lines (mostly) having measured ultraviolet extinction curves. We used the pair method to determine the MIR extinction that we then fit with a power law for the continuum and modified Drude profiles for the silic…

2021 The Astrophysical Journal
IUE eHST 59
TESS Observations of the WASP-121 b Phase Curve
DOI: 10.3847/1538-3881/abd8d2 Bibcode: 2021AJ....161..131D

Mikal-Evans, Thomas; Sing, David K.; Kane, Stephen R. +23 more

We study the red-optical photometry of the ultrahot Jupiter WASP-121 b as observed by the Transiting Exoplanet Survey Satellite (TESS) and model its atmosphere through a radiative transfer simulation. Given its short orbital period of ∼1.275 days, inflated state, and bright host star, WASP-121 b is exceptionally favorable for detailed atmospheric …

2021 The Astronomical Journal
eHST 58