7.1k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Chinese Academy of SciencesCN5.9k papers
- University of Chinese Academy of SciencesCN2.2k papers
- Peking UniversityCN1.2k papers
- Centre National de la Recherche ScientifiqueFR759 papers
- Yunnan ObservatoriesCN679 papers
- Shanghai Astronomical ObservatoryCN633 papers
- Beijing Normal UniversityCN629 papers
- Purple Mountain ObservatoryCN616 papers
- Tsinghua UniversityCN578 papers
- Kavli Institute for Theoretical SciencesCN552 papers
- Nanjing UniversityCN462 papers
- Center for Astrophysics Harvard & SmithsonianUS455 papers
28 papers · 2 filters
The Five-hundred-meter Aperture Spherical Radio Telescope (FAST) Project
Di Li, Zhichen Pan
The Five-hundred-meter Aperture Spherical radio Telescope (FAST) is a Chinese mega-science project funded by the National Development and Reform Commission (NDRC) of the People's R…
LAMOST Spectrograph Response Curves: Stability and Application to flux calibration
Bing Du, A-Li Luo, Zhong-Rui Bai +14
The task of flux calibration for LAMOST (Large sky Area Multi-Object Spectroscopic Telescope) spectra is difficult due to many factors. For example, the lack of standard stars, fla…
WES - Weihai Echelle Spectrograph
Dong-Yang Gao, Hang-Xin Ji, Chen Cao +7
The Weihai Echelle Spectrograph (WES) is the first fiber-fed echelle spectrograph for astronomical observation in China. It is primarily used for chemical abundance and asteroseism…
The Deep and Transient Universe in the SVOM Era: New Challenges and Opportunities - Scientific prospects of the SVOM mission
J. Wei, B. Cordier, S. Antier +77
To take advantage of the astrophysical potential of Gamma-Ray Bursts (GRBs), Chinese and French astrophysicists have engaged the SVOM mission (Space-based multi-band astronomical V…
Calibration of Herschel SPIRE FTS observations at different spectral resolutions
N. Marchili, R. Hopwood, T. Fulton +11
The SPIRE Fourier Transform Spectrometer on board the Herschel Space Observatory had two standard spectral resolution modes for science observations: high resolution (HR) and low r…
Optical Sky Brightness and Transparency During the Winter Season at Dome A Antarctica From the Gattini-Allsky Camera
Yi Yang, Anna M. Moore, Kevin Krisciunas +21
The summit of the Antarctic plateau, Dome A, is proving to be an excellent site for optical, NIR, and THz astronomical observations. GATTINI was a wide-field camera installed on th…
Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
Gaia Collaboration, A. G. A. Brown, A. Vallenari +5
At about 1000 days after the launch of Gaia we present the first Gaia data release, Gaia DR1, consisting of astrometry and photometry for over 1 billion sources brighter than magni…
The Gaia mission
Gaia Collaboration
Gaia is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006, following a study in which the original…
Astronomical Data Fusion Tool Based on PostgreSQL
Bo Han, Yanxia Zhang, Shoubo Zhong +1
With the application of advanced astronomical technologies, equipments and methods all over the world, astronomy covers from radio, infrared, visible light, ultraviolet, X-ray and…
Phase Quantization Study of Spatial Light Modulator for Extreme High contrast Imaging
Jiangpei Dou, Deqing Ren
Direct imaging of exoplanets by reflected starlight is extremely challenging due to the large luminosity ratio to the primary star. Wave-front control is a critical technique to at…
The Night Sky Spectrum of Xinglong Observatory: Changes from 2004 to 2015
Ji-Cheng Zhang, Zhou Fan, Jing-Zhi Yan +4
We present spectroscopic measurements on the night sky of Xinglong Observatory for a period of 12 years from 2004 to 2015. The spectra were obtained on moonless clear nights using…
The Infrared Imaging Spectrograph (IRIS) for TMT: Instrument Overview
James E. Larkin, Anna M. Moore, Shelley A. Wright +14
IRIS is a near-infrared (0.84 to 2.4 microns) integral field spectrograph and wide-field imager being developed for first light with the Thirty Meter (TMT). It mounts to the advanc…
The InfraRed Imaging Spectrograph (IRIS) for TMT: latest science cases and simulations
Shelley A. Wright, Gregory Walth, Tuan Do +36
The Thirty Meter Telescope (TMT) first light instrument IRIS (Infrared Imaging Spectrograph) will complete its preliminary design phase in 2016. The IRIS instrument design includes…
A Non-parametric Approach to Constrain the Transfer Function in Reverberation Mapping
Yan-Rong Li, Jian-Min Wang, Jin-Ming Bai
Broad emission lines of active galactic nuclei stem from a spatially extended region (broad-line region, BLR) that is composed of discrete clouds and photoionized by the central io…
eXTP -- enhanced X-ray Timing and Polarimetry Mission
S. N. Zhang, M. Feroci, A. Santangelo +181
eXTP is a science mission designed to study the state of matter under extreme conditions of density, gravity and magnetism. Primary targets include isolated and binary neutron star…
A Monte-Carlo Method for Making SDSS -Band Magnitude more accurate
Jiayin Gu, Cuihua Du, Wenbo Zuo +4
We develop a new Monte-Carlo-based method to convert the SDSS (Sloan Digital Sky Survey) -band magnitude to the SCUSS (South Galactic Cap of -band Sky Survey) -band magnit…
NUV Star Catalogue from the Lunar-based Ultraviolet Telescope Survey. First Release
Xian-Min Meng, Xu-Hui Han, Jian-Yan Wei +7
We present a star catalogue extracted from the Lunar-based Ultraviolet Telescope (LUT) survey program. LUT's observable sky area is a circular belt around the Moon's north pole, an…
Sky reconstruction for the Tianlai cylinder array
Jiao Zhang, Shifan Zuo, Reza Ansari +5
In this paper, we apply our sky map reconstruction method for transit type interferometers to the Tianlai cylinder array. The method is based on the spherical harmonic decompositio…
Sky reconstruction from transit visibilities: PAON-4 and Tianlai Dish Array
Jiao Zhang, Reza Ansari, Xuelei Chen +3
The spherical harmonics -mode decomposition is a powerful sky map reconstruction method suitable for radio interferometers operating in transit mode. It can be applied to variou…
The Xinglong 2.16-m Telescope: Current Instruments and Scientific Projects
Zhou Fan, Huijuan Wang, Xiaojun Jiang +9
The Xinglong 2.16-m reflector is the first 2-meter class astronomical telescope in China. It was jointly designed and built by the Nanjing Astronomical Instruments Factory (NAIF),…
A Sodium laser guide star coupling efficiency measurement method
Feng Lu, Zhi-Xia Shen, Suijian Xue +8
Large telescope's adaptive optics (AO) system requires one or several bright artificial laser guide stars to improve its sky coverage. The recent advent of high power sodium laser…
Detecting super-Nyquist-frequency gravitational waves using a pulsar timing array
S. -X Yi, S. -N. Zhang
The maximum frequency of gravitational waves (GWs) detectable with traditional pulsar timing methods is set by the Nyquist frequency () of the observation. Beyond this…
The data processing pipeline for the Herschel SPIRE Fourier Transform Spectrometer
T. Fulton, D. A. Naylor, E. T. Polehampton +13
We present the data processing pipeline to generate calibrated data products from the Spectral and Photometric Imaging Receiver (SPIRE) imaging Fourier Transform Spectrometer on th…
The radio environment of the 21 Centimeter Array: RFI detection and mitigation
Yan Huang, Xiang-Ping Wu, Qian Zheng +2
Detection and mitigation of radio frequency interference (RFI) is the first and also the key step for data processing in radio observations, especially for ongoing low frequency ra…