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AST3-2 SN Survey Data Release - Image
The data contains 22,576 images, in total of 4.5 TB, covering 565 survey fields with ~ 2000 square
degree
...
Each field has about 30 obs and covers 4.3 square
degree
.
AST3-2 SN Survey Data Release - Catalogue
The data contains 7,702,085 targets, in total of 458MB, covering 565 survey fields with ~ 2000 square
degree
...
Each field has about 30 obs and covers 4.3 square
degree
, and the median limiting magnitude is ~ 17.8mag ...
AST3-2 SN Survey Data Release - Lightcurve
data contains 7,702,611 light curves, in total of 104GB, covering 565 survey fields with ~ 2000 square
degree
...
Each field has about 30 obs and covers 4.3 square
degree
, and the median limiting magnitude is ~ 17.8mag ...
AST3-2 SN Survey Data Release
The data covers 565 survey fields with ~ 2000 square
degree
.
Each field has about 30 obs and covers 4.3 square
degree
.
天文学家利用神经网络方法搜索强引力透镜系统
在此基础上,云南大学中国西南天文研究所的宇宙学团组构建并训练了一个卷积神经网络,并将其应用于欧洲南方天文台2.6米巡天望远镜(VST)千平方度巡天(Kilo-
Degree
Survey—KiDS ...
天文软件大师新年讲座系列
Received a
degree
of Master of Science Electrical Engineering from Georgia Institute of Technology, Atlanta ...
Magnetic Flux and Magnetic Non-potentiality of Active Regions in Eruptive and Confined Solar Flares
Geostationary Operational Environmental Satellite (GOES) class C5.0 and larger that occurred within 45
degree
...
Magnetic Flux and Magnetic Non-potentiality of Active Regions in Eruptive and Confined Solar Flares
Geostationary Operational Environmental Satellite (GOES) class C5.0 and larger that occurred within 45
degree
...
The First Release of the CSTAR
four 14.5cm optical telescopes, each with a different filter (g, r, i and open) and has a 4.5x4.5 sq.
degree
...
Dynamic Property and Magnetic Nonpotentiality of Two Types of Confined Solar Flares
About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21
degree
Mx−1, and about 66% of “Type II ...
” confined events have ΨHFED/ΦAR≥1.0×10−21
degree
Mx−1.
Dynamic Property and Magnetic Nonpotentiality of Two Types of Confined Solar Flares
About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21
degree
Mx−1, and about 66% of “Type II ...
” confined events have ΨHFED/ΦAR≥1.0×10−21
degree
Mx−1.
Dynamic Property and Magnetic Nonpotentiality of Two Types of Confined Solar Flares
About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21
degree
Mx−1, and about 66% of “Type II ...
” confined events have ΨHFED/ΦAR≥1.0×10−21
degree
Mx−1.
Dynamic Property and Magnetic Nonpotentiality of Two Types of Confined Solar Flares
About 73% of “Type I” confined flares have ΨHFED/ΦAR<1.0×10−21
degree
Mx−1, and about 66% of “Type II ...
” confined events have ΨHFED/ΦAR≥1.0×10−21
degree
Mx−1.
Basic Information and Derived Properties of the Final AGN Sample
RA (
degree
): Right ascension (J2000). DEC (
degree
): Declination (J2000). z: Redshift.
Basic Information and Derived Properties of the Final AGN Sample
RA (
degree
): Right ascension (J2000). DEC (
degree
): Declination (J2000). z: Redshift.
Basic Information and Derived Properties of the Final AGN Sample
RA (
degree
): Right ascension (J2000). DEC (
degree
): Declination (J2000). z: Redshift.
Basic Information and Derived Properties of the Final AGN Sample
RA (
degree
): Right ascension (J2000). DEC (
degree
): Declination (J2000). z: Redshift.
Magnetic Helicity Budget of Solar Active Regions Prolific of Eruptive and Confined Flares
Based on nonlinear force-free (NLFF) coronal magnetic field models with a high
degree
of solenoidality ...
Magnetic Helicity Budget of Solar Active Regions Prolific of Eruptive and Confined Flares
Based on nonlinear force-free (NLFF) coronal magnetic field models with a high
degree
of solenoidality ...
First U.S. Naval Observatory CCD Astrograph Catalog(UCAC1)
The UCAC aims at a density (stars per square
degree
) larger than that of the Guide Star Catalog (GSC) ...
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