Search Publications

TDCOSMO. IX. Systematic comparison between lens modelling software programs: Time-delay prediction for WGD 2038−4008
DOI: 10.1051/0004-6361/202243401 Bibcode: 2022A&A...667A.123S

Frieman, J.; Treu, T.; Palmese, A. +15 more

The importance of alternative methods for measuring the Hubble constant, such as time-delay cosmography, is highlighted by the recent Hubble tension. It is paramount to thoroughly investigate and rule out systematic biases in all measurement methods before we can accept new physics as the source of this tension. In this study, we perform a check f…

2022 Astronomy and Astrophysics
eHST 33
The CGM2 Survey: Circumgalactic O VI from Dwarf to Massive Star-forming Galaxies
DOI: 10.3847/1538-4357/ac450c Bibcode: 2022ApJ...927..147T

Tripp, Todd M.; Prochaska, J. Xavier; Tejos, Nicolas +9 more

We combine 126 new galaxy-O VI absorber pairs from the CGM2 survey with 123 pairs drawn from the literature to examine the simultaneous dependence of the column density of O VI absorbers (N O VI) on galaxy stellar mass, star-formation rate, and impact parameter. The combined sample consists of 249 galaxy-O VI absorber pairs …

2022 The Astrophysical Journal
eHST 33
The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. VI. Insights from Radiative Transfer Modeling
DOI: 10.3847/1538-4357/ac574d Bibcode: 2022ApJ...929...76S

Sheehan, Patrick D.; Megeath, S. Thomas; Looney, Leslie W. +1 more

We present Markov Chain Monte Carlo radiative transfer modeling of a joint ALMA 345 GHz and spectral energy distribution data set for a sample of 97 protostellar disks from the VLA and ALMA Nascent Disk and Multiplicity Survey of Orion Protostars. From this modeling, we derive disk and envelope properties for each protostar, allowing us to examine…

2022 The Astrophysical Journal
Herschel 33
Relentless and complex transits from a planetesimal debris disc
DOI: 10.1093/mnras/stab3475 Bibcode: 2022MNRAS.511.1647F

Mustill, A. J.; Hermes, J. J.; Gänsicke, B. T. +12 more

This article reports quasi-continuous transiting events towards WD 1054-226 at d = 36.2 pc and V = 16.0 mag, based on simultaneous, high-cadence, multiwavelength imaging photometry using ULTRACAM over 18 nights from 2019 to 2020 March. The predominant period is 25.02 h and corresponds to a circular orbit with blackbody Teq = 323 K, wher…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 33
Detection and characterization of instrumental transients in LISA Pathfinder and their projection to LISA
DOI: 10.1103/PhysRevD.105.042002 Bibcode: 2022PhRvD.105d2002B

Baghi, Quentin; Korsakova, Natalia; Slutsky, Jacob +3 more

The LISA Pathfinder (LPF) mission succeeded outstandingly in demonstrating key technological aspects of future space-borne gravitational-wave detectors, such as the Laser Interferometer Space Antenna (LISA). Specifically, LPF demonstrated with unprecedented sensitivity the measurement of the relative acceleration of two free-falling cubic test mas…

2022 Physical Review D
LISAPathfinder 33
High-precision chemical abundances of Galactic building blocks. The distinct chemical abundance sequence of Sequoia
DOI: 10.1051/0004-6361/202142752 Bibcode: 2022A&A...661A.103M

Hattori, Kohei; Helmi, Amina; Ishigaki, Miho N. +5 more

Context. Sequoia is a retrograde kinematic substructure in the nearby Galactic halo, whose properties are a matter of debate. For example, previous studies do not necessarily agree on the chemical abundances of Sequoia stars, which are important for understanding its nature.
Aims: We characterize the chemical properties of a sample of stars f…

2022 Astronomy and Astrophysics
Gaia 33
SALT3-NIR: Taking the Open-source Type Ia Supernova Model to Longer Wavelengths for Next-generation Cosmological Measurements
DOI: 10.3847/1538-4357/ac93f9 Bibcode: 2022ApJ...939...11P

Pérez-Fournon, I.; Fox, O. D.; Poidevin, F. +32 more

A large fraction of Type Ia supernova (SN Ia) observations over the next decade will be in the near-infrared (NIR), at wavelengths beyond the reach of the current standard light-curve model for SN Ia cosmology, SALT3 (~2800-8700 Å central filter wavelength). To harness this new SN Ia sample and reduce future light-curve standardization systematic …

2022 The Astrophysical Journal
eHST 33
Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076
DOI: 10.1051/0004-6361/202243065 Bibcode: 2022A&A...664A.156O

Alonso, R.; Bouchy, F.; Deleuil, M. +93 more

Context. TOI-2076 is a transiting three-planet system of sub-Neptunes orbiting a bright (G = 8.9 mag), young (340 ± 80 Myr) K-type star. Although a validated planetary system, the orbits of the two outer planets were unconstrained as only two non-consecutive transits were seen in TESS photometry. This left 11 and 7 possible period aliases for each…

2022 Astronomy and Astrophysics
CHEOPS Gaia 33
Galactic Kinematics and Observed Flare Rates of a Volume-complete Sample of Mid-to-late M Dwarfs: Constraints on the History of the Stellar Radiation Environment of Planets Orbiting Low-mass Stars
DOI: 10.3847/1538-4357/ac77f9 Bibcode: 2022ApJ...935..104M

Winters, Jennifer G.; Medina, Amber A.; Irwin, Jonathan M. +1 more

We present a study of the relationship between Galactic kinematics, flare rates, chromospheric activity, and rotation periods for a volume-complete, nearly all-sky sample of 219 single stars within 15 pc and with masses between 0.1 and 0.3 M observed during the primary mission of TESS. We find all stars consistent with a common value …

2022 The Astrophysical Journal
Gaia 33
Dwarf AGNs from Optical Variability for the Origins of Seeds (DAVOS): insights from the dark energy survey deep fields
DOI: 10.1093/mnras/stac2262 Bibcode: 2022MNRAS.516.2736B

Bacon, D.; Shen, Yue; Smith, M. +69 more

We present a sample of 706, z < 1.5 active galactic nuclei (AGNs) selected from optical photometric variability in three of the Dark Energy Survey (DES) deep fields (E2, C3, and X3) over an area of 4.64 deg2. We construct light curves using difference imaging aperture photometry for resolved sources and non-difference imaging PSF pho…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 33