Search Publications

Ytterbium atom interferometry for dark matter searches
DOI: 10.1103/PhysRevA.110.033313 Bibcode: 2024PhRvA.110c3313Z

Zhou, Yifan; Ranson, Rowan; Panagiotou, Michalis +1 more

We analyze the projected sensitivity of a laboratory-scale ytterbium atom interferometer to scalar, vector, and pseudoscalar dark matter signals. A frequency ratio measurement between two transitions in Yb171 enables a sea…

2024 Physical Review A
MICROSCOPE 2
Cosmic-ray diffusion in two local filamentary clouds
DOI: 10.1051/0004-6361/202348299 Bibcode: 2024A&A...685A.102K

Grenier, I. A.; Kamal Youssef, F. R.

Context. Hadronic interactions between cosmic rays (CRs) and interstellar gas have been probed in γ rays across the Galaxy. A fairly uniform CR distribution is observed up to a few hundred parsecs from the Sun, except in the Eridu cloud, which shows an unexplained 30-50% deficit in GeV to TeV CR flux.
Aims: To explore the origin of this defic…

2024 Astronomy and Astrophysics
Gaia 2
Study on Test-Mass Charging for Taiji Gravitational Wave Observatory
DOI: 10.1029/2023SW003724 Bibcode: 2024SpWea..2203724H

Han, Ruilong; Cai, Minghui; Yang, Tao +8 more

Taiji is proposed as a space-based gravitational wave (GW) observatory consisting of three spacecraft in a heliocentric orbit meanwhile with the distance of 3 million kilometers ahead of the Earth at about 20°. Free-falling test masses (TMs) are a key component of the interferometer for space-based GW detection in the 0.1mHz-1 Hz frequency range. …

2024 Space Weather
Ulysses 2
Calibrating the metallicity of M dwarfs in wide physical binaries with F-, G-, and K-primaries - II: carbon, oxygen, and odd-Z iron-peak abundances of the primary stars
DOI: 10.1093/mnras/stae076 Bibcode: 2024MNRAS.528.3028D

Caballero, J. A.; Montes, D.; Duque-Arribas, C. +1 more

Detailed chemical composition of stars is of prime interest for a range of topics in modern stellar astrophysics, such as the chemical evolution of the Galaxy or the formation, composition, and structure of exoplanets. In this work, we derive the C and O abundances and update Sc, V, Mn, and Co abundances considering hyperfine structure effects and…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
Exploration of Halo Substructures in Integrals-of-motion Space with Gaia Data Release 3
DOI: 10.3847/1538-4357/ad8352 Bibcode: 2024ApJ...976..161L

Ye, Dashuang; Du, Cuihua; Deng, Mingji +2 more

Using kinematic data from the Gaia Data Release 3 catalog, along with metallicity estimates robustly derived from Gaia BP/RP spectra, we have explored the Galactic stellar halo in search of both known and potentially new substructures. By applying the Hierarchical Density-Based Spatial Clustering of Applications with Noise clustering algorithm in …

2024 The Astrophysical Journal
Gaia 2
The MIRI/MRS Library. I. Empirically correcting detector charge migration in unresolved sources
DOI: 10.1051/0004-6361/202450241 Bibcode: 2024A&A...688A.226G

Gordon, Karl D.; Law, David R.; Patapis, Polychronis +7 more

Context. The James Webb Space Telescope (JWST) has been collecting scientific data for over two years now. The Medium Resolution Spectrometer (MRS) of the Mid-InfraRed Instrument (MIRI) has been one of the telescope's most popular modes, and has already produced ground-breaking results. Scientists are now looking deeper into the data for new excit…

2024 Astronomy and Astrophysics
JWST 2
The merger of hard binaries in globular clusters as the primary channel for the formation of second-generation stars
DOI: 10.1093/mnras/stad3611 Bibcode: 2024MNRAS.527.7005K

Kravtsov, Valery; Calderón, Francisco A.; Dib, Sami

We have recently presented observational evidence which suggests that the origin of the second-generation (G2) stars in globular clusters (GCs) is due to the binary-mediated collision of primordial (G1) low-mass main-sequence (MS) stars. This mechanism avoids both the mass budget problem and the need of external gas for dilution. Here, we report o…

2024 Monthly Notices of the Royal Astronomical Society
eHST 2
NGC 5474 X-1: A neutron star ultraluminous X-ray source in an old stellar cluster?
DOI: 10.1093/mnras/stad3719 Bibcode: 2024MNRAS.52710185A

Fabrika, Sergei; Atapin, Kirill; Vinokurov, Alexander +4 more

We present an optical and X-ray study of the ultraluminous X-ray source (ULX) NGC 5474 X-1. The X-ray spectrum taken during the bright state of the source (LX ~ 2 × 1040 erg s-1) shows signatures of a broad absorption line at ≃ 8 keV, which may be a cyclotron resonant scattering feature. This implies that this syst…

2024 Monthly Notices of the Royal Astronomical Society
eHST 2
La Silla-QUEST RR Lyrae star survey II: the Crater II tidal streams
DOI: 10.1093/mnras/stae488 Bibcode: 2024MNRAS.535..443C

Girard, T.; Baltay, C.; Howard, R. +5 more

We describe photometry improvements in the La Silla-Quest RR Lyrae star (RRLS) survey that enable it to reach distances from the Sun (d) ~140 kpc. We report the results of surveying ~300 deg2 of sky around the large, low-surface-brightness Crater II dwarf spheroidal galaxy. At d >80 kpc, we find a large overde…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
A CIGALE module tailored (not only) for low-luminosity active galactic nuclei
DOI: 10.1051/0004-6361/202450510 Bibcode: 2024A&A...692A.209L

Alexander, D. M.; Lapi, A.; Comastri, A. +17 more

The spectral energy distribution (SED) of low-luminosity active galactic nuclei (LLAGN) presents unique challenges as the emission from these objects is comparable to the radiation from their host galaxy and the accretion physics involved is particularly complex. This study introduces a novel CIGALE module specifically designed to address these ch…

2024 Astronomy and Astrophysics
Herschel XMM-Newton 2