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Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. IV. Long-term Doppler Spectroscopy for 11 Stars Thought to Host Cool Giant Exoplanets
DOI: 10.3847/1538-4365/ad18c3 Bibcode: 2024ApJS..271...16D

Mayo, Andrew W.; Rice, Malena; Kane, Stephen R. +29 more

Discovering and characterizing exoplanets at the outer edge of the transit method's sensitivity has proven challenging owing to geometric biases and the practical difficulties associated with acquiring long observational baselines. Nonetheless, a sample of giant exoplanets on orbits longer than 100 days has been identified by transit hunting missi…

2024 The Astrophysical Journal Supplement Series
Gaia 4
A λ 3 mm Line Survey toward the Circumstellar Envelope of the Carbon-rich AGB Star IRC+10216 (CW Leo)
DOI: 10.3847/1538-4365/ad2460 Bibcode: 2024ApJS..271...45T

Zhang, Yong; Zhou, Jianjun; Szczerba, Ryszard +14 more

We present an unbiased λ 3 mm spectral line survey (between 84.5 and 115.8 GHz), conducted by the Purple Mountain Observatory 13.7 m radio telescope, together with updated modeling results, toward the carbon-rich asymptotic giant branch star IRC+10216 (CW Leo). A total of 75 spectral lines (96 transitions) are detected, and identified to arise fro…

2024 The Astrophysical Journal Supplement Series
Herschel 4
Relations of Rotation and Chromospheric Activity to Stellar Age for FGK Dwarfs from Kepler and LAMOST
DOI: 10.3847/1538-4365/ad1eee Bibcode: 2024ApJS..271...19Y

Xiang, Maosheng; Bi, Shaolan; Li, Yaguang +9 more

The empirical relations between rotation period, chromospheric activity, and age can be used to estimate stellar age. To calibrate these relations, we present a catalog, including the masses and ages of 52,321 FGK dwarfs, 47,489 chromospheric activity index $\mathrm{log}{R}_{\mathrm{HK}}^{+}$ , 6077 rotation periods P rot, and variabili…

2024 The Astrophysical Journal Supplement Series
Gaia 4
Projected Rotational Velocities for LAMOST Stars with Effective Temperatures Lower than 9000 K
DOI: 10.3847/1538-4365/ad1eeb Bibcode: 2024ApJS..271....4Z

Luo, A. -Li; Kong, Xiao; Li, Yinbi +5 more

In Data Release 9 of LAMOST, we present measurements of v sin i for a total of 121,698 stars measured using the Medium Resolution Spectrograph (MRS) and 80,108 stars using the Low Resolution Spectrograph (LRS). These values were obtained through a χ 2 minimization process, comparing LAMOST spectra with corresponding grids of synthetical…

2024 The Astrophysical Journal Supplement Series
Gaia 4
He-rich Hot Subdwarf Stars Observed in Gaia DR3 and LAMOST DR7: Carbon and Nitrogen Abundances and Kinematics
DOI: 10.3847/1538-4365/ad1ab2 Bibcode: 2024ApJS..271...21L

Luo, Yangping; Németh, Péter; Wang, Kun +1 more

We conducted an analysis of the abundances of He, C, and N in 210 He-rich hot subdwarfs observed within both the Gaia Data Release 3 (DR3) and LAMOST DR7 data sets. This analysis involved fitting the LAMOST spectra with TLUSTY/SYNSPEC non-LTE synthetic spectra. By examining the Galactic spatial positions, velocity vectors, and orbital parameters o…

2024 The Astrophysical Journal Supplement Series
Gaia 4
Erratum: "Stellar Loci. VII. Photometric Metallicities of 5 Million FGK Stars Based on GALEX GR6+7 AIS and Gaia EDR3" (2024, ApJS, 271, 26)
DOI: 10.3847/1538-4365/ad488b Bibcode: 2024ApJS..272...49L

Huang, Yang; Beers, Timothy C.; Yuan, Haibo +5 more

We combine photometric data from GALEX GR6+7 AIS and Gaia EDR3 with stellar parameters from the SAGA and PASTEL catalogs to construct high-quality training samples for dwarfs ($\rm 0.4< BP-RP<1.6$) and giants ($\rm 0.6< BP-RP <1.6$). We apply careful reddening corrections using empirical temperature- and extinction-dependent extinction…

2024 The Astrophysical Journal Supplement Series
Gaia 3
Magnetic Activity of Millions of G-type Stars Based on the LAMOST DR10 Low-resolution Spectral and TESS Light-curve Surveys and the Future CSST Survey
DOI: 10.3847/1538-4365/ad2de3 Bibcode: 2024ApJS..271...60S

Han, Xianming L.; Misra, Prabhakar; Zhang, Li-yun +5 more

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) data release 10 (DR10) provides over 3 million G-type stellar spectra, which are important for the study of chromospheric activity of solar-like stars. We have used the iSpec program to perform spectral subtraction on the G-type stellar spectra obtained from LAMOST DR10 with a …

2024 The Astrophysical Journal Supplement Series
Gaia 3
Double-lined Spectroscopic Binaries from the LAMOST Low-resolution Survey
DOI: 10.3847/1538-4365/ad856a Bibcode: 2024ApJS..275...40L

Ting, Yuan-Sen; Liu, Junhui; Zhang, Bo +1 more

We report on a data-driven spectral model that we have developed for the identification of double-lined spectroscopic binary stars (SB2s) in the Large Sky Area Multi-Object fiber Spectroscopic Telescope low-resolution survey (R ∼ 1800). Employing simultaneous fitting with both single-star and binary-star models, we detected over 4800 SB2 candidate…

2024 The Astrophysical Journal Supplement Series
Gaia 3
A Deep Redshift Survey of the Perseus Cluster (A426): Spatial Distribution and Kinematics of Galaxies
DOI: 10.3847/1538-4365/ad390d Bibcode: 2024ApJS..272...22K

Park, Byeong-Gon; Hwang, Narae; Hwang, Ho Seong +3 more

We study the global kinematics of the Perseus galaxy cluster (A426) at redshift z = 0.017 using a large sample of galaxies from our new MMT/Hectospec spectroscopic observation for this cluster. The sample includes 1447 galaxies with measured redshifts within 60' from the cluster center (1148 from this MMT/Hectospec program and 299 from the literat…

2024 The Astrophysical Journal Supplement Series
XMM-Newton 3
A Catalog of Early-type Runaway Stars from LAMOST DR8
DOI: 10.3847/1538-4365/ad46f8 Bibcode: 2024ApJS..272...45G

Wang, Luqian; Liu, Chao; Wu, You +3 more

Runaway stars are OB-type stars ejected from their birthplace with large peculiar velocities. The leading hypothesis addressed in their formation includes the supernova ejection mechanism and the dynamic ejection scenario. Identification of runaway populations is the first step to investigating their formation and evolution. Here we present our wo…

2024 The Astrophysical Journal Supplement Series
Gaia 3