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CHIANTI—An Atomic Database for Emission Lines—Paper. XVIII. Version 11, Advanced Ionization Equilibrium Models: Density and Charge Transfer Effects
DOI: 10.3847/1538-4357/ad6765 Bibcode: 2024ApJ...974...71D

Young, P. R.; Del Zanna, G.; Dere, K. P. +4 more

Version 11 of the CHIANTI database and software package is presented. Advanced ionization equilibrium models have been added for low charge states of seven elements (C, N, O, Ne, Mg, Si, and S), and represent a significant improvement especially when modeling the solar transition region. The models include the effects of higher electron density an…

2024 The Astrophysical Journal
IRIS 7
A first systematic characterization of cataclysmic variables in SRG/eROSITA surveys
DOI: 10.1051/0004-6361/202450537 Bibcode: 2024A&A...690A.243S

Salvato, M.; Stelzer, B.; Schwope, A. D. +4 more

We present an account of known cataclysmic variables (CVs) that were detected as X-ray sources in eROSITA X-ray surveys and have Gaia DR3 counterparts. We address standard CVs with main sequence donors and white dwarfs accreting via Roche-lobe overflow (RLOF) and related objects, the double degenerates (DDs), and the symbiotic stars (SySts). We di…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 7
89 New Ultracool Dwarf Comoving Companions Identified with the Backyard Worlds: Planet 9 Citizen Science Project
DOI: 10.3847/1538-3881/ad324e Bibcode: 2024AJ....167..253R

Meisner, Aaron M.; Cushing, Michael C.; Kirkpatrick, J. Davy +43 more

We report the identification of 89 new systems containing ultracool dwarf companions to main-sequence stars and white dwarfs, using the citizen science project Backyard Worlds: Planet 9 and cross-reference between Gaia and CatWISE2020. 32 of these companions and 33 host stars were followed up with spectroscopic observations, with companion spectra…

2024 The Astronomical Journal
Gaia 7
Wide Binaries with White Dwarf or Neutron Star Companions Discovered from Gaia DR3 and LAMOST
DOI: 10.3847/1538-4357/aced95 Bibcode: 2024ApJ...964..101Z

Liu, Jifeng; Zhang, Haotong; Wang, Song +12 more

The Gaia Data Release 3 (DR3) mission has identified and provided about 440,000 binary systems with orbital solutions, offering a valuable resource for searching binaries including a compact component. By combining the Gaia DR3 data with radial velocities from the LAMOST spectroscopic survey, we identify three wide binaries possibly containing a c…

2024 The Astrophysical Journal
Gaia XMM-Newton 7
X-Ray Winds in Nearby-to-distant Galaxies (X-WING). I. Legacy Surveys of Galaxies with Ultrafast Outflows and Warm Absorbers in z ∼ 0–4
DOI: 10.3847/1538-4365/ad5961 Bibcode: 2024ApJS..274....8Y

Enoto, Teruaki; Ueda, Yoshihiro; Kawamuro, Taiki +10 more

As an inaugural investigation under the X-ray Winds In Nearby-to-distant Galaxies (X-WING) program, we assembled a data set comprising 132 active galactic nuclei (AGNs) spanning redshifts z ∼ 0–4 characterized by blueshifted absorption lines indicative of X-ray winds. Through an exhaustive review of previous research, we compiled the outflow param…

2024 The Astrophysical Journal Supplement Series
XMM-Newton 7
Observation of a propagating slow magnetoacoustic wave in a coronal plasma fan with SDO/AIA and SolO/EUI
DOI: 10.1093/mnras/stad3506 Bibcode: 2024MNRAS.527.5302M

Nakariakov, Valery M.; Kolotkov, Dmitrii Y.; Zhong, Sihui +1 more

Simultaneous observations of a propagating disturbance of EUV intensity, with SDO/AIA at 171 Å and SolO/EUI-HRIEUV at 174 Å, are investigated. The disturbance moves outwards along a plasma fan structure in active region AR 12941 on February 7th 2022, at 12:45-14:15 UT. The spacecraft line-of-sight separation is 19°. The variation of the EUV intens…

2024 Monthly Notices of the Royal Astronomical Society
SolarOrbiter 7
TEMPLATES: A Robust Outlier Rejection Method for JWST/NIRSpec Integral Field Spectroscopy
DOI: 10.1088/1538-3873/ad34fd Bibcode: 2024PASP..136d4503H

Hutchison, Taylor A.; Rigby, Jane R.; Sharon, Keren +14 more

We describe a custom outlier rejection algorithm for JWST/NIRSpec integral field spectroscopy. This method uses a layered sigma clipping approach that adapts clipping thresholds based upon the spatial profile of the science target. We find that this algorithm produces a robust outlier rejection while simultaneously preserving the signal of the sci…

2024 Publications of the Astronomical Society of the Pacific
JWST 7
Using Ly α transits to constrain models of atmospheric escape
DOI: 10.1093/mnras/stae1976 Bibcode: 2024MNRAS.533.3296S

Schreyer, Ethan; Owen, James E.; Loyd, R. O. Parke +1 more

Ly $\alpha$ transits provide an opportunity to test models of atmospheric escape directly. However, translating observations into constraints on the properties of the escaping atmosphere is challenging. The major reason for this is that the observable parts of the o…

2024 Monthly Notices of the Royal Astronomical Society
eHST 7
A Formally Motivated Retrieval Framework Applied to the High-resolution Transmission Spectrum of HD 189733 b
DOI: 10.3847/1538-3881/ad2c8b Bibcode: 2024AJ....167..179B

Blain, Doriann; Sánchez-López, Alejandro; Mollière, Paul

Ground-based high-resolution spectra provide a powerful tool for characterizing exoplanet atmospheres. However, they are greatly hampered by the dominating telluric and stellar lines, which need to be removed prior to any analysis. Such removal techniques ("preparing pipelines") deform the spectrum; hence, a key point is to account for this proces…

2024 The Astronomical Journal
eHST 7
JWST Observations of Young protoStars (JOYS): Overview of gaseous molecular emission and absorption in low-mass protostars
DOI: 10.1051/0004-6361/202451967 Bibcode: 2024A&A...692A.197V

Güdel, M.; Ray, T. P.; Chen, Y. +17 more

Context. The Mid-InfraRed Instrument (MIRI) on board the James Webb Space Telescope (JWST) allows one to probe the molecular gas composition at mid-infrared (mid-IR) wavelengths with unprecedented resolution and sensitivity. It is important to study these features in low-mass embedded protostellar systems, since the formation of planets is thought…

2024 Astronomy and Astrophysics
JWST 7