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Validations and Corrections of the SFD and Planck Reddening Maps Based on LAMOST and Gaia Data
DOI: 10.3847/1538-4365/ac642f Bibcode: 2022ApJS..260...17S

Chen, Bingqiu; Yuan, Haibo; Sun, Yang

Precise correction of dust reddening is fundamental to obtain the intrinsic parameters of celestial objects. The Schlegel et al. (SFD) and the Planck 2D extinction maps are widely used for reddening correction. In this work, using accurate reddening determinations of about 2 million stars from the Large Sky Area Multi-Object Fiber Spectroscopic Te…

2022 The Astrophysical Journal Supplement Series
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
Radio-loud Quasars above Redshift 4: Very Long Baseline Interferometry (VLBI) Imaging of an Extended Sample
DOI: 10.3847/1538-4365/ac63b8 Bibcode: 2022ApJS..260...49K

Paragi, Zsolt; Krezinger, Máté; Frey, Sándor +7 more

High-redshift radio sources provide plentiful opportunities for studying the formation and evolution of early galaxies and supermassive black holes. However, the number of known radio-loud active galactic nuclei (AGN) above redshift 4 is rather limited. At high redshifts, it appears that blazars, with relativistically beamed jets pointing toward t…

2022 The Astrophysical Journal Supplement Series
Gaia XMM-Newton 18
Stellar Atmospheric Parameters of M-type Stars from LAMOST DR8
DOI: 10.3847/1538-4365/ac6754 Bibcode: 2022ApJS..260...45D

Gao, Qi; Wu, Yue; Yan, Hong-Liang +9 more

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Low Resolution Spectroscopic Survey (LRS) provides massive spectroscopic data on M-type stars, and the derived stellar parameters could bring vital help to various studies. We adopt the ULySS package to perform χ 2 minimization with model spectra generated from the M…

2022 The Astrophysical Journal Supplement Series
Gaia 18
A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit
DOI: 10.3847/1538-4365/ac75bd Bibcode: 2022ApJS..262...12K

Kobulnicky, Henry A.; Cook, Evan M.; Molnar, Lawrence A. +1 more

Contact binary star systems represent the long-lived penultimate phase of binary evolution. Population statistics of their physical parameters inform an understanding of binary evolutionary pathways and end products. We use light curves and new optical spectroscopy to conduct a pilot study of ten (near) contact systems in the long-period (P > 0…

2022 The Astrophysical Journal Supplement Series
Gaia 17
Universal Scaling Laws for Solar and Stellar Atmospheric Heating: Catalog of Power-law Index between Solar Activity Proxies and Various Spectral Irradiances
DOI: 10.3847/1538-4365/ac8b15 Bibcode: 2022ApJS..262...46T

Notsu, Yuta; Namekata, Kosuke; Toriumi, Shin +1 more

The formation of extremely hot outer atmospheres is one of the most prominent manifestations of magnetic activity common to late-type dwarf stars, including the Sun. It is widely believed that these atmospheric layers, the corona, transition region, and chromosphere, are heated by the dissipation of energy transported upwards from the stellar surf…

2022 The Astrophysical Journal Supplement Series
Hinode 17
Finding Quasars behind the Galactic Plane. II. Spectroscopic Identifications of 204 Quasars at ∣b∣ < 20°
DOI: 10.3847/1538-4365/ac7f3e Bibcode: 2022ApJS..261...32F

Zheng, Jie; Jiang, Linhua; Feng, Xiaotong +21 more

Quasars behind the Galactic plane (GPQs) are important astrometric references and valuable probes of Galactic gas, yet the search for GPQs is difficult due to severe extinction and source crowding in the Galactic plane. In this paper, we present a sample of 204 spectroscopically confirmed GPQs at ∣b∣ < 20°, 191 of which are new discoveries. Thi…

2022 The Astrophysical Journal Supplement Series
Gaia 17
A Catalog of Early-type Hα Emission-line Stars and 62 Newly Confirmed Herbig Ae/Be Stars from LAMOST Data Release 7
DOI: 10.3847/1538-4365/ac4964 Bibcode: 2022ApJS..259...38Z

Qin, Li; Luo, A. -Li; Hou, Wen +6 more

We derive a catalog of early-type emission-line stars including 30,023 spectra of 25,867 stars from LAMOST Data Release 7, in which 4189 have Simbad records. The spectra are classified into three morphological types (10 subtypes) based on Hα emission-line profiles. Some spectra contaminated by nebula emission lines such as from H II regions are fl…

2022 The Astrophysical Journal Supplement Series
Gaia 17
BASS. XXIII. A New Mid-infrared Diagnostic for Absorption in Active Galactic Nuclei
DOI: 10.3847/1538-4365/ac5b65 Bibcode: 2022ApJS..261....3P

Ricci, Claudio; Stern, Daniel; Trakhtenbrot, Benny +15 more

In this study, we use the Swift/BAT AGN sample, which has received extensive multiwavelength follow-up analysis as a result of the BAT AGN Spectroscopic Survey, to develop a diagnostic for nuclear obscuration by examining the relationship between the line-of-sight column densities (N H), the 2–10 keV to 12 µm luminosity ratio, and…

2022 The Astrophysical Journal Supplement Series
AKARI XMM-Newton 16
Photometric Recalibration of the SDSS Stripe 82 to a Few Millimagnitude Precision with the Stellar Color Regression Method and Gaia EDR3
DOI: 10.3847/1538-4365/ac470d Bibcode: 2022ApJS..259...26H

Huang, Bowen; Yuan, Haibo

By combining spectroscopic data from the LAMOST DR7, Sloan Digital Sky Survey (SDSS) DR12, and corrected photometric data from the Gaia EDR3, we apply the stellar color regression (SCR) method to recalibrate the SDSS Stripe 82 standard stars catalog of Ivezić et al. With a total number of about 30,000 spectroscopically targeted stars, we have mapp…

2022 The Astrophysical Journal Supplement Series
Gaia 16