TESS detection of periodic brightness variations during the rise of classical nova PGIR22akgylf
Kirill V. Sokolovsky, Elias Aydi, Konstantin Malanchev, Koji Mukai, Jennifer L. Sokoloski, Laura Chomiuk, Peter Allen Craig, Rebekah A. Hounsell, Justin D. Linford, Isabella Molina, Montana N. Williams, Kishalay De, Mansi M. Kasliwal, Nicholas Earley, David J. Lane, Filipp D. Romanov, Richard Schmidt
astro-ph.SR
Submitted: 2026-06-10
Comments: 21 page, 11 figures, 3 tables; submitted to PASP; comments welcome
Code: https://github.com/kirxkirx/PGIR22akgylf_lightkurve
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The Pan-STARRS1 Surveys
- The orbital period of the nova V1674 Her as observed with TESS
- A very rapidly rotating white dwarf in nova YZ Reticuli
- The Place of Recurrent Novae among the Symbiotic Stars
- TESS Input Catalog versions 8.1 and 8.2: Phantoms in the 8.0 Catalog and How to Handle Them
- Pre-maximum and maximum of Novae: The spectroscopic observations of Nova ASASSN-17hx
- Insights from Pulsating Nova Envelopes
- TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections?
- Atlas of photometric and spectroscopic daily monitoring of the very slow Nova Cas 2021 (=V1405 Cas) during the first 660 days of its outburst
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