Search Publications

Near-Earth Sub-Alfvénic Solar Winds: Interplanetary Origins and Geomagnetic Impacts
DOI: 10.3847/1538-4357/ac4471 Bibcode: 2022ApJ...926..135H

Hajra, Rajkumar; Tsurutani, Bruce T.

The near-Earth solar wind is in general super-Alfvénic and supermagnetosonic. Using all available near-Earth solar wind measurements between 1973 and 2020, we identified 30 intervals with sub-Alfvénic solar winds. The majority (83%) of the events occurred within interplanetary coronal mass ejection magnetic clouds (MCs)/driver gases. These MC sub-…

2022 The Astrophysical Journal
SOHO 18
Deep learning-based super-resolution and de-noising for XMM-newton images
DOI: 10.1093/mnras/stac2437 Bibcode: 2022MNRAS.517.4054S

Valtchanov, Ivan; Verdugo, Eva; Lieu, Maggie +6 more

The field of artificial intelligence based image enhancement has been rapidly evolving over the last few years and is able to produce impressive results on non-astronomical images. In this work, we present the first application of Machine Learning based super-resolution (SR) and de-noising (DN) to enhance X-ray images from the European Space Agenc…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 18
Quasi-periodic Accelerations of Energetic Particles during a Solar Flare
DOI: 10.3847/2041-8213/ac6fd2 Bibcode: 2022ApJ...931L..28L

Chen, Wei; Li, Dong

We report the observation of nonstationary quasi-periodic pulsations (QPPs) in high-energy particles during the impulsive phase of an X4.8 flare on 2002 July 23 (SOL2002-07-23T00:35). The X4.8 flare was simultaneously measured by the Reuven Ramaty High Energy Solar Spectroscopic Imager, Nobeyama Radio Polarimeters, and Nobeyama Radioheliograph. Th…

2022 The Astrophysical Journal
SOHO 18
zELDA: fitting Lyman alpha line profiles using deep learning
DOI: 10.1093/mnras/stab3554 Bibcode: 2022MNRAS.510.4525G

Gronke, Max; Saito, Shun; Bonoli, Silvia +2 more

We present zELDA (redshift Estimator for Line profiles of Distant Lyman Alpha emitters), an open source code to fit Lyman α (Ly α) line profiles. The main motivation is to provide the community with an easy to use and fast tool to analyse Ly α line profiles uniformly to improve the understating of Ly α emitting galaxies. zELDA is based on line pro…

2022 Monthly Notices of the Royal Astronomical Society
eHST 18
Future constraints on primordial black holes from XGIS-THESEUS
DOI: 10.1103/PhysRevD.106.023022 Bibcode: 2022PhRvD.106b3022G

Ghosh, Diptimoy; Sachdeva, Divya; Singh, Praniti

Current observations allow primordial black holes (PBHs) in asteroid mass range 1017- 1022 g to constitute the entire dark matter energy density (barring a small mass range constrained by 21-cm observations). In this work, we explore the possibility of probing PBHs with masses 1017- 1019 g via the upcomi…

2022 Physical Review D
INTEGRAL 18
Dark and luminous mass components of Omega Centauri from stellar kinematics
DOI: 10.1093/mnras/stac261 Bibcode: 2022MNRAS.511.4251E

Zivick, Paul; Strigari, Louis E.; Evans, Addy J.

We combine proper motion data from Gaia EDR3 and HST with line-of-sight velocity data to study the stellar kinematics of the ω Cen globular cluster. Using a steady-state, axisymmetric dynamical model, we measure the distribution of both the dark and luminous mass components. Assuming both Gaussian and Navarro-Frenk-White mass profiles, depending o…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 18
Chemodynamical Signatures of Bar Resonances in the Galactic Disk: Current Data and Future Prospects
DOI: 10.3847/1538-4357/ac7da0 Bibcode: 2022ApJ...935...28W

Fragkoudi, Francesca; Wheeler, Adam; Ness, Melissa +2 more

The Galactic disk exhibits complex chemical and dynamical substructure thought to be induced by the bar, spiral arms, and satellites. Here, we explore the chemical signatures of bar resonances in action and velocity space, and characterize the differences between the signatures of corotation (CR) and higher-order resonances using test particle sim…

2022 The Astrophysical Journal
Gaia 18
From ridges to manifolds: 3D characterization of the moving groups in the Milky Way disc
DOI: 10.1051/0004-6361/202244070 Bibcode: 2022A&A...667A.116B

Antoja, T.; Bernet, M.; Monari, G. +4 more

Context. The details of the effect of the bar and spiral arms on the disc dynamics of the Milky Way are still unknown. The stellar velocity distribution in the solar neighbourhood displays kinematic substructures, which are possibly signatures of these processes and of previous accretion events. With the Gaia mission, more details of these signatu…

2022 Astronomy and Astrophysics
Gaia 18
Dynamically Tagged Groups of Metal-poor Stars. II. The Radial Velocity Experiment Data Release 6
DOI: 10.3847/1538-4365/ac680c Bibcode: 2022ApJS..261...19S

Huang, Yang; Beers, Timothy C.; Placco, Vinicius M. +2 more

Orbital characteristics based on Gaia Early Data Release 3 astrometric parameters are analyzed for ~8000 metal-poor stars ([Fe/H] ≤ -0.8) compiled from the Radial Velocity Experiment (RAVE) Data Release 6. Selected as metal-poor candidates based on broadband photometry, RAVE collected moderate-resolution (R ~ 7500) spectra in the region of the Ca …

2022 The Astrophysical Journal Supplement Series
Gaia 18
Quasars with large proper motions: A selection from the LQAC-5 catalogue combined with Gaia EDR3. Focusing on astrometric and photometric properties
DOI: 10.1051/0004-6361/202141915 Bibcode: 2022A&A...660A..16S

Zacharias, N.; Barache, C.; Lambert, S. +5 more

Context. Thanks to the cross-identification between the Gaia EDR3 (E-Data Release 3) catalogue and the quasars' compiled catalogue LQAC-5 (Large Quasar Astrometric Catalogue-5), accurate astrometric parameters as well as photometric measurements were available for a set of 416 113 quasars.
Aims: After analysing the astrometric and photometric…

2022 Astronomy and Astrophysics
Gaia 18