GRAVITY+: towards faint science, all sky milli arcsecond optical interferometric imaging

S. Gillessen
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引用次数: 1

Abstract

GRAVITY and the VLTI have transformed optical interferometry with ground-breaking results on the Galactic Center, Active Galactic Nuclei, and Exoplanets. With modest upgrades to GRAVITY+, the Paranal Observatory will open up the extragalactic sky for milli-arcsec resolution interferometric imaging, and give access to galactic targets as faint as 22 mag. GRAVITY+ will measure the black hole masses of active galactic nuclei across cosmic times, establish whether globular clusters harbor intermediate-mass black holes, and obtain high-quality exoplanet spectra and orbits. The straightforward upgrade consists of implementing off-axis fringe tracking, an improved throughput, and laser-guide star adaptive optics for all 8m telescopes and can be divided up into several phases. Most of the upgrades will be beneficial to all VLTI instruments. Here we present a few selected science cases and outline the project, which could be implemented within a few years.
GRAVITY+:面向微弱科学,全天空毫角秒光学干涉成像
重力和VLTI已经改变了光学干涉测量法,在银河系中心、活动星系核和系外行星上取得了突破性的结果。通过对GRAVITY+的适度升级,帕拉纳天文台将打开银河系外的天空,进行毫弧分辨率的干涉成像,并获得微弱到22等的星系目标。GRAVITY+将测量跨宇宙时间活动星系核的黑洞质量,确定球状星团是否有中等质量的黑洞,并获得高质量的系外行星光谱和轨道。直接升级包括实现离轴条纹跟踪,提高吞吐量,以及所有8米望远镜的激光导星自适应光学系统,可以分为几个阶段。大多数升级将有利于所有VLTI仪器。在这里,我们提出了一些精选的科学案例,并概述了该项目,该项目可能在几年内实施。
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