Uploaded August 2020 | Updated September 2026, 1 hour ago
The Zwicky Transient Facility high-cadence Galactic Plane survey and its implications for LISA
Thomas Kupfer
The Zwicky Transient Facility (ZTF) started science operation in March 2018. 40% of ZTF observing time is dedicated to two public surveys: one covering the entire Northern sky every three nights in g and r passbands and one visiting the Galactic Plane every night in g and r. In addition to the public Galactic Plane survey, ZTF has conducted a dedicated high-cadence survey of selected Galactic Plane fields to find and study ultracompact Galactic binaries. So far we have covered about 4900 sqd. In this talk, I will present an overview of the ZTF Galactic Plane observations and present some science highlights from the first two years, including a new class of ultracompact He-star binaries which are detectable for LISA.
The Zwicky Transient Facility high-cadence Galactic Plane survey and its implications for LISA
Thomas Kupfer
The Zwicky Transient Facility (ZTF) started science operation in March 2018. 40% of ZTF observing time is dedicated to two public surveys: one covering the entire Northern sky every three nights in g and r passbands and one visiting the Galactic Plane every night in g and r. In addition to the public Galactic Plane survey, ZTF has conducted a dedicated high-cadence survey of selected Galactic Plane fields to find and study ultracompact Galactic binaries. So far we have covered about 4900 sqd. In this talk, I will present an overview of the ZTF Galactic Plane observations and present some science highlights from the first two years, including a new class of ultracompact He-star binaries which are detectable for LISA.
