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2018年SPIE天文望远镜和仪器仪表会议（SPIE Astronomical Telescopes + Instrumentation）
2018年 SPIE 天文望远镜和仪器仪表 会议
2017/11/27
SPIE conference papers are published in the Proceedings of SPIE and available via the SPIE Digital Library, the world’s largest collection of optics and photonics research. The Proceedings are indexed...
2018年SPIE空间望远镜和仪器：紫外线到伽马射线会议（SPIE Space Telescopes and Instrumentation 2018:Ultraviolet to Gamma Ray）
2018年 SPIE 空间望远镜和仪器：紫外线到伽马射线 会议
2017/11/27
Observation of the hot universe, from 105 K upward, has a vital impact on some of the most fundamental questions in astrophysics today. Hot plasmas, from the sun and stellar coronae to the cores of ga...
2018年SPIE地面和机载望远镜会议（SPIE Ground-based and Airborne Telescopes VII）
2018年 SPIE 地面和机载望远镜 会议
2017/11/27
This conference is the latest in the series on Ground Based and Airborne Telescopes, where progress in the field continues at an exciting pace. The next generation of extremely large telescopes is und...
2018年SPIE望远镜和仪器光学与机械技术进展会议（SPIE Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation）
2018年 SPIE 望远镜和仪器光学与机械技术进展 会议
2017/11/27
Following the success of the SPIE Modern Technologies in Space- and Ground-based Telescopes and Instrumentation conferences in previous years, this conference will continue to provide an opportunity a...
High-energy astrophysics is a relatively young scientific field, made possible by space-borne telescopes. During the half-century history of x-ray astronomy, the sensitivity of focusing x-ray telescop...
A Statistical Comparison of the Optical/UV and X-ray Afterglows of Gamma-Ray Bursts using the Swift Ultra-violet Optical and X-ray Telescopes
Statistical Comparison the Optical/UV X-ray
2010/11/30
We present the systematic analysis of the UVOT and XRT light curves for a sample of 26 Swift Gamma-Ray Bursts (GRBs). By comparing the optical/UV and X-ray light curves, we found that they are remarka...
Pulsar timing arrays as imaging gravitational wave telescopes: angular resolution and source (de)confusion
Pulsar timing arrays imaging gravitational wave telescopes
2010/10/30
Pulsar timing arrays (PTAs) will be sensitive to a finite number of gravitational wave (GW) "point" sources (e.g. supermassive black hole binaries). N quiet pulsars with accurately known distances d_{...
Present and future of the TeV astronomy with Cherenkov telescopes
High Energy Astrophysical Phenomena (astro-ph.HE)
2010/10/11
Cherenkov telescopes play a major role in the growth of the TeV Astronomy which, in 20 years, has reached the status of an important branch of Astrophysics, because of the observations of the violent,...
Observations of the Blazar 3C 66A with the MAGIC Telescopes in Stereoscopic Mode
High Energy Astrophysical Phenomena (astro-ph.HE)
2010/10/4
We report new observations of the intermediate-frequency peaked BL Lacertae object 3C 66A with the MAGIC telescopes. The data sample we use were taken in 2009 December and 2010 January, and comprises ...
El Observatorio de San Pedro Mártir：A World-Class Site for Large Telescopes
San Pedro Mártir Large Telescopes World-Class Site
2009/7/1
El Observatorio de San Pedro Mártir：A World-Class Site for Large Telescopes。
Observations of AGN with large telescopes。
The Diffuse Ionized Gas in the large telescopes era
Diffuse Ionized Gas large telescopes era
2009/6/25
The Diffuse Ionized Gas in the large telescopes era。
Faint C and O recombination lines in H II regions and large telescopes：The case of S311
recombination lines H II regions Faint C
2009/6/25
Faint C and O recombination lines in H II regions and large telescopes：The case of S311。
Near Ground Wind Simulations by a Meso-Scale Atmospherical Model for the Extremely Large Telescopes Site Selection
Wind Simulations Telescopes Site Selection Meso-Scale Atmospherical
2009/6/16
Near Ground Wind Simulations by a Meso-Scale Atmospherical Model for the Extremely Large Telescopes Site Selection。
The meteorological stations of the 1.5 and 0.84 m telescopes of the OAN：description and results
telescopes meteorological stations OAN
2009/6/9
The meteorological stations of the 1.5 and 0.84 m telescopes of the OAN: description and results。