Search Publications

ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies Selected by Herschel: Discovery of Spatially Extended SMGs and Implications
DOI: 10.3847/1538-4357/abd6e4 Bibcode: 2021ApJ...908..192S

Pérez-González, Pablo G.; Richard, Johan; Smail, Ian +19 more

We present an ALMA 1.3 mm (Band 6) continuum survey of lensed submillimeter galaxies (SMGs) at z = 1.0 to ∼3.2 with an angular resolution of ∼0"2. These galaxies were uncovered by the Herschel Lensing Survey and feature exceptionally bright far-infrared continuum emission (Speak ≳ 90 mJy) owing to their lensing magnification. We detect …

2021 The Astrophysical Journal
Gaia Herschel eHST 18
Forward modelling of Kepler-band variability due to faculae and spots
DOI: 10.1093/mnras/stab1190 Bibcode: 2021MNRAS.504.4751J

Solanki, Sami K.; Shapiro, Alexander I.; Krivova, Natalie +4 more

Variability observed in photometric light curves of late-type stars (on time-scales longer than a day) is a dominant noise source in exoplanet surveys and results predominantly from surface manifestations of stellar magnetic activity, namely faculae and spots. The implementation of faculae in light-curve models is an open problem, with scaling typ…

2021 Monthly Notices of the Royal Astronomical Society
SOHO 18
Discovery of O stars in the tidal Magellanic Bridge. Stellar parameters, abundances, and feedback of the nearest metal-poor massive stars and their implication for the Magellanic System ecology
DOI: 10.1051/0004-6361/202039486 Bibcode: 2021A&A...646A..16R

Hamann, W. -R.; Oskinova, L. M.; Ramachandran, V.

The Magellanic Bridge, stretching between the Small and the Large Magellanic Cloud (SMC and LMC), is the nearest tidally stripped intergalactic environment. The Bridge has a significantly low average metallicity of Z ≲ 0.1 Z. Here we report the first discovery of O-type stars in the Magellanic Bridge. Three massive O stars were identif…

2021 Astronomy and Astrophysics
Gaia 18
Galactic extinction laws - II. Hidden in plain sight, a new interstellar absorption band at 7700 Å broader than any known DIB
DOI: 10.1093/mnras/staa2371 Bibcode: 2021MNRAS.501.2487M

Caballero, J. A.; Bohlin, R. C.; Maíz Apellániz, J. +2 more

We have detected a broad interstellar absorption band centred close to 7700 Å and with a full width at half-maximum (FWHM) of 176.6 ± 3.9 Å. This is the first such absorption band detected in the optical range and is significantly wider than the numerous diffuse interstellar bands (DIBs). It remained undiscovered until now because it is partially …

2021 Monthly Notices of the Royal Astronomical Society
eHST 18
A search for variable subdwarf B stars in TESS Full Frame Images - II. Variable objects in the northern ecliptic hemisphere
DOI: 10.1093/mnras/stab668 Bibcode: 2021MNRAS.503.3828B

Sahoo, S. K.; Baran, A. S.; Ostrowski, J. +1 more

We report the results of our search for pulsating subdwarf B stars in Full Frame Images collected during Year 2 of the TESS mission and covering the northern ecliptic hemisphere. This is a continuation of our effort we presented in Paper I. We found 13 likely new pulsating subdwarf B stars, 10 pulsating candidates that are identified as other hot …

2021 Monthly Notices of the Royal Astronomical Society
Gaia 18
Cosmological constraints on Hořava gravity revised in light of GW170817 and GRB170817A and the degeneracy with massive neutrinos
DOI: 10.1103/PhysRevD.103.104060 Bibcode: 2021PhRvD.103j4060F

Frusciante, Noemi; Benetti, Micol

We revise the cosmological bounds on Hořava gravity, taking into account the stringent constraint on the speed of propagation of gravitational waves from GW170817 and GRB170817A. In light of this, we also investigate the degeneracy between massive neutrinos and Hořava gravity. We show that a luminal propagation of gravitational waves suppresses th…

2021 Physical Review D
eHST 18
Magnetic and Rotational Evolution of ρ CrB from Asteroseismology with TESS
DOI: 10.3847/1538-4357/ac1f19 Bibcode: 2021ApJ...921..122M

Kochukhov, Oleg; Drake, Jeremy J.; Stassun, Keivan G. +15 more

During the first half of main-sequence lifetimes, the evolution of rotation and magnetic activity in solar-type stars appears to be strongly coupled. Recent observations suggest that rotation rates evolve much more slowly beyond middle age, while stellar activity continues to decline. We aim to characterize this midlife transition by combining arc…

2021 The Astrophysical Journal
Gaia 18
Deciphering Solar Magnetic Activity: 140 Years of the `Extended Solar Cycle' - Mapping the Hale Cycle
DOI: 10.1007/s11207-021-01938-7 Bibcode: 2021SoPh..296..189M

Velli, Marco; McIntosh, Scott W.; Srivastava, Abhishek K. +6 more

We investigate the occurrence of the "extended solar cycle" (ESC) as it occurs in a host of observational data spanning 140 years. Investigating coronal, chromospheric, photospheric, and interior diagnostics, we develop a consistent picture of solar activity migration linked to the 22-year Hale (magnetic) cycle using superposed epoch analysis (SEA…

2021 Solar Physics
SOHO 18
Sinuous ridges in Chukhung crater, Tempe Terra, Mars: Implications for fluvial, glacial, and glaciofluvial activity
DOI: 10.1016/j.icarus.2020.114131 Bibcode: 2021Icar..35714131B

Conway, Susan J.; Balme, Matthew R.; Lewis, Stephen R. +6 more

We present a geomorphic map of Chukhung crater (38.47°N, 72.42°W) in central Tempe Terra, Mars. Chukhung crater formed ~3.6-2.1 Ga, between the early Hesperian and early Amazonian periods of Mars' geologic history. It hosts dendritic networks of crater wall valleys, broad crater floor valleys, mid- to late-Amazonian-aged debris-covered glaciers, m…

2021 Icarus
MEx 18
Benchmarking Dust Emission Models in M101
DOI: 10.3847/1538-4357/abe942 Bibcode: 2021ApJ...912..103C

Gordon, Karl D.; Leroy, Adam K.; Koch, Eric W. +7 more

We present a comparative study of four physical dust models and two single-temperature modified blackbody models by fitting them to the resolved WISE, Spitzer, and Herschel photometry of M101 (NGC 5457). Using identical data and a grid-based fitting technique, we compare the resulting dust and radiation field properties derived from the models. We…

2021 The Astrophysical Journal
Herschel 18