Conférences - Astronomie, astrophysique et cosmologie - Chine

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1
The 3rd PANDA Symposium on Time Domain Astronomy and first results from Insight-HXMT
18 jui 2018 - 22 jui 2018 • Chengdu, Chine
Résumé:
The Hard X-ray Modulation Telescope (HXMT), also known as Insight, is China’s first space X-ray astronomy satellite, designed to observe X-ray emission from compact objects, such as black holes, neutron stars and Gamma Ray Bursts (GRBs). This satellite was successfully launched on June 15, 2017, and has already produced multiple interesting results during its in-orbit test. In particular, the Insight-HXMT participated in a global joint observation in search of the electromagnetic counterparts of GW170817, providing a stringent constraint for the properties of the electromagnetic radiation from this binary neutron star merger. We plan to unveil the first results from the Insight-HXMT at the anniversary of its launch, during the 3rd PANDA Symposium. We will also take this opportunity to discuss some hot topics in high-energy astrophysics and introduce the mission to the younger Pacific/Asiatic as well as the international community.
Contact:
Email.: yinqq@ihep.ac.cn
Sujets:
First Results from Insight-HXMT, Gravitational Waves and Their Electromagnetic Counterparts, Extreme Accretion Events on Supermassive Black Holes, Neutron Stars
Identifiant de l'évènement:
1025665
2
2018 Colloquium on QTT Science and Technology
10 jul 2018 • Urumqi, Chine
Résumé:
The Steerable 110-m Aperture Radio Telescope (SmART) is a key project at state level jointly promoted by the Chinese Academy of Sciences, Xinjiang Autonomous Region, and the astronomical community in China. The general goal of the project is to build the world’s largest aperture fully steerable radio telescope in Qitai County, Xinjiang. The telescope is also known as the Qitai Radio Telescope (QTT for short).
Identifiant de l'évènement:
1037456
3
2018 Colloquium on QTT Science and Technology
10 jul 2018 - 14 jul 2018 • Urumqi, Chine
Résumé:
The Steerable 110-m Aperture Radio Telescope (SmART) is a key project at state level jointly promoted by the Chinese Academy of Sciences, Xinjiang Autonomous Region, and the astronomical community in China. The general goal of the project is to build the world’s largest aperture fully steerable radio telescope in Qitai County, Xinjiang. The telescope is also known as the Qitai Radio Telescope (QTT for short). The design of the QTT and associated systems is well advanced and we expect construction to commence soon. We are planning this Colloquium to provide an overview of building and operating large-aperture radio telescopes around the world, with a focus on QTT scientific goals, frontier technologies, QTT construction and project management, etc. We expect the Colloquium to provide valuable suggestions to further the development of radio astronomy and technology in China. We cordially invite domestic and foreign experts in radio astronomy to join the Colloquium.
Sujets:
Steerable 110-m Aperture Radio Telescope Science and Technology
Identifiant de l'évènement:
1036716
4
The 2nd APSCO & ISSI-BJ Space Science School with EISCAT on "Study Space Weather Effects From the Sun to the Ground"
10 oct 2018 • China Remote Sensing Satellite Ground Station, San, Chine
Identifiant de l'évènement:
1070380
5
The Life And Times Of The Milky Way: The Symbiosis Between Gaia And Ground-Based Spectroscopic Surveys
12 nov 2018 • Shanghai, Chine
Identifiant de l'évènement:
1033400
6
IAU Symposium: Galactic Dynamics in the Era of Large Surveys
23 jui 2019 • Shanghai, Chine
Identifiant de l'évènement:
1070363
7
IAU Symposium: Galactic Dynamics in the Era of Large Surveys
23 jui 2019 - 28 jui 2019 • Shanghai, Chine
Résumé:
Galaxy dynamics is key to our understanding of the assembly history and current structure of galaxies. Surveys of the Milky Way, Local Group, and nearby and distant galaxies, are mapping their kinematics and chemistry in unprecedented detail. The deluge of data is helping to clarify the role of interactions, gas cycle, star formation, nuclear activity, dynamical and secular evolution in shaping galaxies, and is also raising new questions. The conference will review our current knowledge and address the major challenges to our understanding of galaxy structure and evolution.
Identifiant de l'évènement:
1059774

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Dernière mise jour: 25 Mai 2018