Detection of a 0.1802-day periodic signal in TESS photometry of slow-rising nova PGIR22akgylf interpreted as orbital modulation from binary distortion of the envelope during common-envelope interaction.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Modeling indicates arrays of small seeing-limited telescopes are more cost-effective than single large seeing-limited ones for single-object observations, with single diffraction-limited telescopes preferred only below 20-28 magnitudes depending on architecture.
citing papers explorer
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TESS detection of periodic brightness variations during the rise of classical nova PGIR22akgylf
Detection of a 0.1802-day periodic signal in TESS photometry of slow-rising nova PGIR22akgylf interpreted as orbital modulation from binary distortion of the envelope during common-envelope interaction.
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Single object observations: Large telescopes vs. multiple small telescopes
Modeling indicates arrays of small seeing-limited telescopes are more cost-effective than single large seeing-limited ones for single-object observations, with single diffraction-limited telescopes preferred only below 20-28 magnitudes depending on architecture.