The World Space Observatory Ultraviolet (WSO-UV), as a bridge to future UV astronomy
arXiv:1802.06849 · doi:10.1007/s10509-018-3280-7
Abstract
The ultraviolet (UV) astronomy is a very demanded branch of space astronomy. Many dozens of short-term UV-experiments in space, as well as long-term observatories, have brought a very important knowledge on the physics and chemistry of the Universe during the last decades. Unfortunately, no large UV-observatories are planned to be launched by most of space agencies in the coming 10 -- 15 years. Conversely, the large UVOIR observatories of the future will appear not earlier than in 2030s. This paper briefly describes the projects that have been proposed by various groups. We conclude that the World Space Observatory -- Ultraviolet (WSO-UV) will be the only 2-m class UV telescope with capabilities similar to those of the HST for the next decade. The WSO-UV has been described in detail in previous publications, and this paper updates the main characteristics of its instruments and the current state of the whole project. It also addresses the major science topics that have been included in the core program of the WSO-UV, making this core program very relevant to the current state of the UV-astronomy. Finally, we also present here the ground segment architecture that will implement this program.
arXiv commentInternational symposium "Ultraviolet Sky Surveys: the need and the means", 10-14 July 2017, Tel Aviv University, Israel
References in corpus (10)
- The Swift Ultra-Violet/Optical Telescope
- Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation
- The XMM-Newton Optical/UV Monitor Telescope
- The COS-Halos Survey: Physical Conditions and Baryonic Mass in the Low-Redshift Circumgalactic Medium
- In-orbit Performance of UVIT on ASTROSAT
- Strategies for Detecting the Missing Hot Baryons in the Universe
- Finding the UV-Visible Path Forward: Proceedings of the Community Workshop to Plan the Future of UV/Visible Space Astrophysics
- World Space Observatory-Ultraviolet: ISSIS, the imaging instrument
- 18-Months Operation of Lunar-based Ultraviolet Telescope: A Highly Stable Photometric Performance
- Massive stars in advanced evolutionary stages, and the progenitor of GW150914
Cited by in corpus (5)
- Cavity Ring-down UV spectroscopy of the C-X electronic transition of CH
- The EarthASAP mission concept for a Lunar orbiting cubesat
- Spectroscopic Investigation of Nebular Gas (SING): Instrument Design, Assembly and Calibration
- UV astronomy with small satellites
- Influence of radiative pumping on the HD rotational level populations in diffuse molecular clouds of the interstellar medium