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PH3 DataGreaves 2020aEncrenaz 2020Snellen 2020Villanueva 2020Mogul 2020Thompson 2020Greaves 2020bGreaves 2020cTrompet 2020Akins 2021Lincowski 2021Greaves 2021Cordiner 2022Greaves 2022Cordiner 2023
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Greaves 2020aDiscovery paperResponse in Greaves 2022Response in Greaves 2020c (see also Greaves 2021)Response in Greaves 2020b,c (see also Greaves 2021)No response needed; Results consistent with the original detectionResponse in Greaves 2020c (see also Greaves 2021)Response in Greaves 2022Response in Greaves 2021Response in Greaves 2021Response in Greaves 2022
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Encrernaz 2020Response in Greaves 2022Mid-IR observations, upper limit above the cloudsResponse in Greaves 2022Response in Greaves 2022Response in Greaves 2022Response: upper limits can be reconciled by PH3 photolysis, as high/low abundances correspond to Venusian mornings/evenings
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Snellen 2020Response in Greaves 2020c (see also Greaves 2021)Reanalysis of ALMA data, no signal in ALMA dataResponse in Greaves 2020c (see also Greaves 2021)Response: polynomial fitting revisited; different non-subjective method (via FTs) also recovers signalResponse: ALMA signal revisited. JCMT signal revisited; SO2 contamination is minimal.Response in Greaves 2020c (see also Greaves 2021)
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Villanueva 2020Response in Greaves 2020b,c (see also Greaves 2021)Reanalysis of ALMA (no signal) and JCMT data (signal but attribute to SO2)Response: JCMT signal attributed to SO2Response: recovery of ALMA signal using 3 different calibration methods. JCMT revisited; SO2 contamination is minimal.Response: polynomial fitting revisited; different non-subjective method (via FTs) also recovers signalResponse: ALMA signal revisited. JCMT signal revisited; SO2 contamination is minimal.Response in Greaves 2020b,c (see also Greaves 2021)
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Mogul 2020No response needed; Results consistent with the original detectionIndepedent detection of PH3 in the clouds in Pioneer Venus legacy dataNo response needed; Results consistent with the original detectionNo response needed; Results consistent with the original detectionResponse: Reanalyis of the Pioneer Venus legacy data suggestive of in-cloud PH3No response needed; Results consistent with the original detectionNo response needed; Results consistent with the original detection
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Thompson 2020Response in Greaves 2020c (see also Greaves 2021)Response: JCMT signal attributed to SO2Reanalysis of JCMT data, no signal in JCMT dataResponse in Greaves 2020c (see also Greaves 2021)Response: polynomial fitting revisited; different non-subjective method (via FTs) also recovers signalResponse: JCMT signal attributed to SO2Response in Greaves 2020cResponse in Greaves 2020c (see also Greaves 2021)
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Greaves 2020bResponse in Greaves 2022Response in Greaves 2020c Response: recovery of ALMA signal using 3 different calibration methods. JCMT revisited; SO2 contamination is minimal.No response needed; Results consistent with the original detectionResponse in Greaves 2020c (see also Greaves 2021)Recovery of ALMA and JCMT signal, SO2 an unlikely explanation for the signalResponse in Greaves 2022Response in Greaves 2021Response in Greaves 2021Response in Greaves 2022
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Greaves 2020cResponse in Greaves 2022Response: polynomial fitting revisited; different non-subjective method (via FTs) also recovers signalResponse: polynomial fitting revisited; different non-subjective method (via FTs) also recovers signalNo response needed; Results consistent with the original detectionResponse: polynomial fitting revisited; different non-subjective method (via FTs) also recovers signalPolynomial fitting revisited, recovery of the signal with non-subjective method (via FTs)Response in Greaves 2022Response in Greaves 2021Response in Greaves 2021Response in Greaves 2022
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Trompet 2020Response in Greaves 2022Response in Greaves 2022Response in Greaves 2022Mid-IR observations, upper limit above the cloudsResponse in Greaves 2022Response: upper limits can be reconciled by PH3 photolysis, as high/low abundances correspond to Venusian mornings/evenings
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Akins 2021Response in Greaves 2021Response in Greaves 2021Response in Greaves 2021Reanalysis of ALMA data, no signal in ALMA dataResponse: ALMA data revisited with half of the planetary disc. Further assesment on SO2 minimal contamination Response in Greaves 2021
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Lincowski 2021Response in Greaves 2021Response: Reanalysis of the Pioneer Venus legacy data suggestive of in-cloud PH3Response: JCMT signal attributed to SO2Response in Greaves 2021Response in Greaves 2021JCMT signal is consistent with mesospheric (above the clouds) SO2Response: nearly simultaneous SO2 observation from the JCMT archive rule out SO2 as a sourceResponse in Greaves 2021
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Greaves 2021Response in Greaves 2022Response: ALMA signal revisited. JCMT signal revisited; SO2 contamination is minimal.Response: ALMA signal revisited. JCMT signal revisited; SO2 contamination is minimal.No response needed; Results consistent with the original detectionResponse in Greaves 2020cResponse in Greaves 2022Response: ALMA data revisited with half of the planetary disc. Further assesment on SO2 minimal contamination Response: nearly simultaneous SO2 observation from the JCMT archive rule out SO2 as a sourceNearly concurrent measurements of SO2 show that the signal cannot be SO2 Response in Greaves 2022
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Cordiner 2022Response in Greaves 2022Response in Greaves 2022Response in Greaves 2022Response in Greaves 2022SOFIA telescope shows no PH3 in Venus’ atmosphere Response: recovery of Venusian PH3 in SOFIA spectra by reducing contaminating signals; the PH3 abundance is ~3 ppb
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Greaves 2022Response: upper limits can be reconciled by PH3 photolysis, as high/low abundances correspond to Venusian mornings/eveningsResponse in Greaves 2020c (see also Greaves 2021)Response in Greaves 2020b,c (see also Greaves 2021)No response needed; Results consistent with the original detectionResponse in Greaves 2020c (see also Greaves 2021)Response: upper limits can be reconciled by PH3 photolysis, as high/low abundances correspond to Venusian mornings/eveningsResponse in Greaves 2021Response in Greaves 2021Response: recovery of Venusian PH3 in SOFIA spectra by reducing contaminating signals; the PH3 abundance is ~3 ppbRecovery of Venusian PH3 (above the clouds) in SOFIA spectra
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Cordiner 2023SOFIA telescope shows no PH3 in Venus’ atmosphere; Fourier analysis in Greaves 2022 is too "aggressive" likely introducing spectral artifacts
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