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月基射电天文研讨会 | Radio Astronomy from the Moon
Radio-frequency interference environment Solar and planetary science Synergies with other disciplines (
e
.g ...
Radio-frequency interference environment Solar and planetary science Synergies with other disciplines (
e
.g ...
The Extended Gaia–PS1–SDSS (GPS1+) Proper Motion Catalog
This catalog is divided into two subsamples, i.
e
., the primary and secondary parts.
The Separation Distribution of Ultrawide Binaries across Galactic Populations
contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.
e
.
The Separation Distribution of Ultrawide Binaries across Galactic Populations
contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.
e
.
Magnetic Flux of Active Regions Determining the Eruptive Character of Large Solar Flares
Geostationary Operational Environmental Satellite class M1.0 and larger that occurred during 2010-2019, i.
e
.
Magnetic Flux of Active Regions Determining the Eruptive Character of Large Solar Flares
Geostationary Operational Environmental Satellite class M1.0 and larger that occurred during 2010-2019, i.
e
.
591 High-velocity Stars in the Galactic Halo Selected from LAMOST DR7 and Gaia DR2
investigate the origins of HiVelSCs, we perform orbit integrations and divide them into four types, i.
e
.
591 High-velocity Stars in the Galactic Halo Selected from LAMOST DR7 and Gaia DR2
investigate the origins of HiVelSCs, we perform orbit integrations and divide them into four types, i.
e
.
The Separation Distribution of Ultrawide Binaries across Galactic Populations
contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.
e
.
The Separation Distribution of Ultrawide Binaries across Galactic Populations
contamination rates quickly increase beyond 20,000~AU, until up to 100% at the largest separation bin, i.
e
.
Stellar Loci. V. Photometric Metallicities of 27 Million FGK Stars Based on Gaia Early Data Release 3
Our method is valid for FGK stars with G ≤ 16, [Fe/H] ≥ -2.5, and
E
(B - V) ≤ 0.5.
Stellar Loci. V. Photometric Metallicities of 27 Million FGK Stars Based on Gaia Early Data Release 3
Our method is valid for FGK stars with G ≤ 16, [Fe/H] ≥ -2.5, and
E
(B - V) ≤ 0.5.
A catalog of early-type Hα emission-line stars and 62 newly confirmed Herbig Ae/Bes from LAMOST DR7
forbidden emission lines of [Fe II] and [O I], in which J051425.20+411310.7 is a newly discovered B[
e
] ...
A catalog of early-type Hα emission-line stars and 62 newly confirmed Herbig Ae/Bes from LAMOST DR7
forbidden emission lines of [Fe II] and [O I], in which J051425.20+411310.7 is a newly discovered B[
e
] ...
A New Magnetic Parameter of Active Regions Distinguishing Large Eruptive and Confined Solar Flares
aim of investigating how the magnetic field in solar active regions (ARs) controls flare activity, i.
e
.
A New Magnetic Parameter of Active Regions Distinguishing Large Eruptive and Confined Solar Flares
aim of investigating how the magnetic field in solar active regions (ARs) controls flare activity, i.
e
.
Finding Quasars behind the Galactic Plane. II. Spectroscopic Identifications of 204 Quasars at |b|<20°
FITS files can be viewed with the splot task of IRAF or read with other standard FITS I/O routines (
e
.g ...
FITS files can be viewed with the splot task of IRAF or read with other standard FITS I/O routines (
e
.g ...
Finding Quasars behind the Galactic Plane. II. Spectroscopic Identifications of 204 Quasars at |b| < 20°
FITS files can be viewed with the splot task of IRAF or read with other standard FITS I/O routines (
e
.g ...
FITS files can be viewed with the splot task of IRAF or read with other standard FITS I/O routines (
e
.g ...
S-type stars discovered in Medium-Resolution Spectra of LAMOST DR9
The discovery of these stars is a three-step process, i.
e
., selecting with the ZrO band indices greater ...
S-type stars discovered in Medium-Resolution Spectra of LAMOST DR9
The discovery of these stars is a three-step process, i.
e
., selecting with the ZrO band indices greater ...
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