Search Publications

Observation of the radiation environment and solar energetic particle events in Mars orbit in May 2018- June 2022
DOI: 10.1016/j.lssr.2023.03.006 Bibcode: 2023LSSR...39..106S

Gopalswamy, Nat; Semkova, Jordanka; Koleva, Rositza +19 more

The dosimeter Liulin-MO for measuring the radiation environment onboard the ExoMars Trace Gas Orbiter (TGO) is a module of the Fine Resolution Epithermal Neutron Detector (FREND). Here we present results from measurements of the charged particle fluxes, dose rates and estimation of dose equivalent rates at ExoMars TGO Mars science orbit, provided …

2023 Life Sciences in Space Research
ExoMars-16 SOHO 6
Constraining dark matter interactions mediated by a light scalar with white dwarfs
DOI: 10.1103/PhysRevD.107.083022 Bibcode: 2023PhRvD.107h3022R

Ramirez-Quezada, Maura E.

Observations of white dwarfs in dark matter-rich environments can provide strong limits on the strength of dark matter interactions. Here we apply the recently improved formalism of the dark matter capture rate in white dwarfs to a general model in which dark matter interacts with the white dwarf ion components via a light scalar mediator. We comp…

2023 Physical Review D
eHST 6
Metallicity-PAH Relation of MIR-selected Star-forming Galaxies in AKARI North Ecliptic Pole-wide Survey
DOI: 10.3847/1538-3881/aca09c Bibcode: 2023AJ....165...31S

Hashimoto, Tetsuya; Jeong, Woong-Seob; Hwang, Ho Seong +9 more

We investigate the variation in the mid-infrared spectral energy distributions of 373 low-redshift (z < 0.4) star-forming galaxies, which reflects a variety of polycyclic aromatic hydrocarbon (PAH) emission features. The relative strength of PAH emission is parameterized as q PAH, which is defined as the mass fraction of PAH particle…

2023 The Astronomical Journal
AKARI Herschel 6
Unveiling the gravitationally unstable disc of a massive star-forming galaxy using NOEMA and MUSE
DOI: 10.1093/mnras/stad1820 Bibcode: 2023MNRAS.524.3913P

Cannon, John M.; Hayes, Matthew; Östlin, Göran +7 more

Using new high-resolution data of CO (2-1), H$\alpha$ and H$\beta$ obtained with the Northern Extended Millimeter Array (NOEMA) and the Multi-Unit Spectroscopic Explorer (MUSE) at the Very Large Telescope, we have performed a Toomre Q disc stability analysis and studied star formation, gas depletion times and other environmental parameters on sub-…

2023 Monthly Notices of the Royal Astronomical Society
eHST 6
Classification of Chandra X-Ray Sources in Cygnus OB2
DOI: 10.3847/1538-4365/acdd68 Bibcode: 2023ApJS..269...10K

Naylor, Tim; Drake, Jeremy J.; Wright, Nicholas J. +11 more

We have devised a predominantly Naive Bayes-based method to classify X-ray sources detected by Chandra in the Cygnus OB2 association into members, foreground objects, and background objects. We employ a variety of X-ray, optical, and infrared characteristics to construct likelihoods using training sets defined by well-measured sources. Combination…

2023 The Astrophysical Journal Supplement Series
Gaia 6
The age, kinematics, and metallicity of nearby Sun-like stars and the history of the Milky Way disc
DOI: 10.1051/0004-6361/202346828 Bibcode: 2023A&A...678A..39G

Gondoin, P.

Contact. Investigating how the Milky Way formed and has evolved is an important topic in astrophysics that requires the determination of precise ages for large samples of stars over long periods.
Aims: The present study addresses the formation history of nearby Sun-like stars using the emission reversal in the cores of their Ca II H&K Fra…

2023 Astronomy and Astrophysics
Gaia 6
The Direct-method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High Noon
DOI: 10.3847/1538-4357/acb153 Bibcode: 2023ApJ...948..108G

Richard, Johan; Siana, Brian; Freeman, William R. +5 more

We present a Keck/MOSFIRE rest-optical composite spectrum of 16 typical gravitationally lensed star-forming dwarf galaxies at 1.7 ≲ z ≲ 2.6 (z mean = 2.30), all chosen independent of emission-line strength. These galaxies have a median stellar mass of $\mathrm{log}{({M}_{* }/{M}_{\odot })}_{\mathrm{med}}={8.29}_{-0.43}^{+0.51}$ and a me…

2023 The Astrophysical Journal
eHST 6
Varstrometry for Off-nucleus and Dual Sub-kiloparsec Active Galactic Nuclei (VODKA): Very Long Baseline Array Searches for Dual or Off-nucleus Quasars and Small-scale Jets
DOI: 10.3847/1538-4357/ad00b3 Bibcode: 2023ApJ...958...29C

Shen, Yue; Zakamska, Nadia L.; Lazio, Joseph +5 more

Dual and off-nucleus active supermassive black holes are expected to be common in the hierarchical structure formation paradigm, but their identification at parsec scales remains a challenge due to strict angular resolution requirements. We conducted a systematic study using the Very Long Baseline Array (VLBA) to examine 23 radio-bright candidate …

2023 The Astrophysical Journal
Gaia 6
Dynamical masses and ages of Sirius-like systems
DOI: 10.1093/mnras/stad1849 Bibcode: 2023MNRAS.524..695Z

Kiman, Rocio; Brandt, Timothy D.; Li, Yiting +4 more

We measure precise orbits and dynamical masses and derive age constraints for six confirmed and one candidate Sirius-like systems, including the Hyades member HD 27483. Our orbital analysis incorporates radial velocities, relative astrometry, and Hipparcos-Gaia astrometric accelerations. We constrain the main-sequence lifetime of a white dwarf's p…

2023 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos eHST 6
Evolution of the Radial Size and Expansion of Coronal Mass Ejections Investigated by Combining Remote and In Situ Observations
DOI: 10.3847/1538-4357/acd847 Bibcode: 2023ApJ...952....7Z

Lugaz, Noé; Zhuang, Bin; Scolini, Camilla +4 more

A fundamental property of coronal mass ejections (CMEs) is their radial expansion, which determines the increase in the CME radial size and the decrease in the CME magnetic field strength as the CME propagates. CME radial expansion can be investigated either by using remote observations or by in situ measurements based on multiple spacecraft in ra…

2023 The Astrophysical Journal
SOHO 6