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View article: Basic considerations on spectral coherent combining for high combining performance
Basic considerations on spectral coherent combining for high combining performance Open
View article: Task Scheduling in Geo-Distributed Computing: A Survey
Task Scheduling in Geo-Distributed Computing: A Survey Open
Geo-distributed computing, a paradigm that assigns computational tasks to globally distributed nodes, has emerged as a promising approach in cloud computing, edge computing, cloud-edge computing and supercomputer computing (HPC). It enable…
View article: LEAVES: An Expandable Light-curve Data Set for Automatic Classification of Variable Stars
LEAVES: An Expandable Light-curve Data Set for Automatic Classification of Variable Stars Open
With the increasing amount of astronomical observation data, it is an inevitable trend to use artificial intelligence methods for automatic analysis and identification of light curves for full samples. However, data sets covering all known…
View article: 3DT-CM: A Low-complexity Cross-matching Algorithm for Large Astronomical Catalogues Using 3d-tree Approach
3DT-CM: A Low-complexity Cross-matching Algorithm for Large Astronomical Catalogues Using 3d-tree Approach Open
Location-based cross-matching is a preprocessing step in astronomy that aims to identify records belonging to the same celestial body based on the angular distance formula. The traditional approach involves comparing each record in one cat…
View article: Data release of the AST3-2 automatic survey from Dome A, Antarctica
Data release of the AST3-2 automatic survey from Dome A, Antarctica Open
AST3-2 is the second of the three Antarctic Survey Telescopes, aimed at wide-field time-domain optical astronomy. It is located at Dome A, Antarctica, which is by many measures the best optical astronomy site on the Earth’s surface. Here w…
View article: HLC2: a highly efficient cross-matching framework for large astronomical catalogues on heterogeneous computing environments
HLC2: a highly efficient cross-matching framework for large astronomical catalogues on heterogeneous computing environments Open
Cross-matching operation, which is to find corresponding data for the same celestial object or region from multiple catalogues, is indispensable to astronomical data analysis and research. Due to the large amount of astronomical catalogues…
View article: NBFTP: a dedicated data transfer system for remote astronomical observation at Dome A*
NBFTP: a dedicated data transfer system for remote astronomical observation at Dome A* Open
Dome A, Antarctica, has been thought to be one of the best astronomical sites on the Earth for decades. Since it was first visited by astronomers in 2008, dozens of facilities for astronomical observation and site testing were deployed. Du…
View article: HCGrid: a convolution-based gridding framework for radio astronomy in hybrid computing environments
HCGrid: a convolution-based gridding framework for radio astronomy in hybrid computing environments Open
Gridding operation, which is to map non-uniform data samples on to a uniformly distributed grid, is one of the key steps in radio astronomical data reduction process. One of the main bottlenecks of gridding is the poor computing performanc…
View article: A redistribution tool for long-term archive of astronomical observation data
A redistribution tool for long-term archive of astronomical observation data Open
View article: AstroCatR: a mechanism and tool for efficient time series reconstruction of large-scale astronomical catalogues
AstroCatR: a mechanism and tool for efficient time series reconstruction of large-scale astronomical catalogues Open
Time series data of celestial objects are commonly used to study valuable and unexpected objects such as extrasolar planets and supernova in time domain astronomy. Due to the rapid growth of data volume, traditional manual methods are beco…
View article: Towards an Astronomical Science Platform: Experiences and Lessons Learned from Chinese Virtual Observatory
Towards an Astronomical Science Platform: Experiences and Lessons Learned from Chinese Virtual Observatory Open
In the era of big data astronomy, next generation telescopes and large sky surveys produce data sets at the TB or even PB level. Due to their large data volumes, these astronomical data sets are extremely difficult to transfer and analyze …
View article: Exoplanets in the Antarctic Sky. III. Stellar Flares Found by AST3-II (CHESPA) within the Southern CVZ of TESS
Exoplanets in the Antarctic Sky. III. Stellar Flares Found by AST3-II (CHESPA) within the Southern CVZ of TESS Open
The CHinense Exoplanet Searching Program from Antarctica is a ground-based wide-field photometric survey using the AST3 and CSTAR telescopes located at Dome A, Antarctica. Blessed with the unparalleled observing conditions on the highest p…
View article: Deep residual detection of radio frequency interference for FAST
Deep residual detection of radio frequency interference for FAST Open
Radio frequency interference (RFI) detection and excision are key steps in the data-processing pipeline of the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Because of its high sensitivity and large data rate, FAST requires…
View article: mcatCS: A Highly Efficient Cross-matching Scheme for Multi-band Astronomical Catalogs
mcatCS: A Highly Efficient Cross-matching Scheme for Multi-band Astronomical Catalogs Open
Multi-band astronomical catalog cross-matching has always been, and will continue to be, indispensable to astronomy research. However, the archived data volume in different wavebands is extremely huge, which results in the cross-matching p…
View article: The first release of the AST3-1 Point Source Catalogue from Dome A, Antarctica
The first release of the AST3-1 Point Source Catalogue from Dome A, Antarctica Open
The three Antarctic Survey Telescopes (AST3) aim to carry out time domain imaging survey at Dome A, Antarctica. The first of the three telescopes (AST3-1) was successfully deployed on January 2012. AST3-1 is a 500\,mm aperture modified Sch…
View article: CMSA: a heterogeneous CPU/GPU computing system for multiple similar RNA/DNA sequence alignment
CMSA: a heterogeneous CPU/GPU computing system for multiple similar RNA/DNA sequence alignment Open
CMSA focuses on the multiple similar RNA/DNA sequence alignment and proposes a novel bitmap based algorithm to improve the center star strategy. We can conclude that harvesting the high performance of modern GPU is a promising approach to …
View article: AstroCloud: A Distributed Cloud Computing and Application Platform for Astronomy
AstroCloud: A Distributed Cloud Computing and Application Platform for Astronomy Open
Virtual Observatory (VO) is a data-intensively online astronomical research and education environment, which takes advantages of advanced information technologies to achieve seamless and global access to astronomical information. AstroClou…
View article: An Improved Platform for Multi-Agent Based Stock Market Simulation in Distributed Environment
An Improved Platform for Multi-Agent Based Stock Market Simulation in Distributed Environment Open
Multi-agent based simulation has been widely used in behavior finance, and several single-processed simulation platforms with Agent-Based Modeling (ABM) have been proposed. However, traditional simulations of stock markets on single proces…