The Weizmann Fast Astronomical Survey Telescope (W-FAST): System Overview

Guy Nir, Eran O Ofek, Sagi Ben-Ami, Noam Segev, David Polishook, Ofir Hershko, Oz Diner, Ilan Manulis, Barak Zackay, Avishay Gal-Yam, Ofer Yaron

Research output: Contribution to journalArticlepeer-review

10 Citations (Scopus)
34 Downloads (Pure)

Abstract

A relatively unexplored phase space of transients and stellar variability is that of second and sub-second timescales. We describe a new optical observatory operating in the Negev desert in Israel, with a 55 cm aperture, a field of view of 2fdg6 × 2fdg6 (≈7 deg2) equipped with a high frame rate, low read noise, CMOS camera. The system can observe at a frame rate of up to 90 HZ (full frame), while nominally observations are conducted at 10–25 Hz. The data, generated at a rate of over 6 Gbits s−1 at a frame rate of 25 Hz, are analyzed in real time. The observatory is fully robotic and capable of autonomously collecting data on a few thousand stars in each field each night. We present the system overview, performance metrics, science objectives, and some first results, e.g., the detection of a high rate of glints from geosynchronous satellites, reported in Nir et al. 2020.
Original languageEnglish
Article number075002
Number of pages14
JournalPublications of the Astronomical Society of the Pacific
Volume133
Issue number1025
DOIs
Publication statusPublished - 7 May 2021

Fingerprint

Dive into the research topics of 'The Weizmann Fast Astronomical Survey Telescope (W-FAST): System Overview'. Together they form a unique fingerprint.

Cite this