posted on 2019-08-09, 09:29authored byK. L. Page, A. P. Beardmore, J. P. Osborne
The rapid response capabilities of the Neil Gehrels Swift Observatory, together with the daily planning of its observing schedule, make it an ideal mission for following novae in the X-ray and UV bands, particularly during their early phases of rapid evolution and throughout the supersoft source interval. Many novae, both classical and recurrent, have been extensively monitored by Swift throughout their supersoft phase and later decline. We collect here results from observations of novae with outbursts which occurred between the start of 2006 and the end of 2017.
Funding
These observations would not have been possible without the support of
the Swift PI (Neil Gehrels, and now Brad Cenko), together with the Mission
and Flight Operations Teams. This work is presented on behalf of the Swift
Nova-CV group, co-ordinated by J.P. Osborne, which is open to applications
to join from all interested scientists. The Swift project at the University of
Leicester is funded by the UK Space Agency.
History
Citation
Advances in Space Research, Volume 66, Issue 5, 1 September 2020, Pages 1169-1192
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
AM (Accepted Manuscript)
Published in
Advances in Space Research
Volume
66
Issue
5
Pagination
1169-1192
Publisher
Elsevier for Pergamon, Committee on Space Research (COSPAR)
54 pages, 33 figure panels, 2 tables. To be published in a Special Issue of Advances in Space Research, entitled "Nova Eruptions, Cataclysmic Variables and Related Systems: observational vs theoretical challenges in the 2020 era", following COSPAR 2018;The file associated with this record is under embargo until 12 months after publication, in accordance with the publisher's self-archiving policy. The full text may be available through the publisher links provided above.