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Cited article:

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Constraints on TESS albedos for five hot Jupiters

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TESS Phase Curve of the Hot Jupiter WASP-19b

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3.6 AND 4.5 μm SPITZER PHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b

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Defocused transmission spectroscopy: a potential detection of sodium in the atmosphere of WASP-12b

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K s-band secondary eclipses of WASP-19b and WASP-43b with the Anglo-Australian Telescope★

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Thermal emission at 3.6–8 μm from WASP-19b: a hot Jupiter without a stratosphere orbiting an active star

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The Astrophysical Journal 767 (1) 64 (2013)
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Physical properties, transmission and emission spectra of the WASP-19 planetary system from multi-colour photometry★

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GROUND-BASED TRANSIT SPECTROSCOPY OF THE HOT-JUPITER WASP-19b IN THE NEAR-INFRARED

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The Astrophysical Journal 774 (2) 118 (2013)
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z ′-BAND GROUND-BASED DETECTION OF THE SECONDARY ECLIPSE OF WASP-19b

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IMPROVED SPECTROSCOPIC PARAMETERS FOR TRANSITING PLANET HOSTS

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NEAR-INFRARED THERMAL EMISSION FROM WASP-12b: DETECTIONS OF THE SECONDARY ECLIPSE INKs,H, ANDJ

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Thermal emission at 4.5 and 8 μm of WASP-17b, an extremely large planet in a slightly eccentric orbit

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Thermal emission from WASP-33b, the hottest known planet★

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A CORRELATION BETWEEN STELLAR ACTIVITY AND HOT JUPITER EMISSION SPECTRA

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Lessons from detections of the near-infrared thermal emission of hot Jupiters

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Proceedings of the International Astronomical Union 6 (S276) 154 (2010)
https://doi.org/10.1017/S1743921311020102

High-precision photometry by telescope defocusing - III. The transiting planetary system WASP-2★

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Monthly Notices of the Royal Astronomical Society 408 (3) 1680 (2010)
https://doi.org/10.1111/j.1365-2966.2010.17238.x