JCMT spectra of Venus at 266.94 GHz, June 2017: photo
The discovery data: single-dish spectra from the RxA3 receiver and ACSIS correlator around the phosphine 1–0 line, in which the claimed absorption is a few parts in ten thousand of the continuum.
ESO, 2017. CC BY 4.0
Copies 5
DatasetEast Asian Observatory · cadc-ccda.hia-iha.nrc-cnrc.gc.ca · 2017-06 · JCMT/EAO data policy: public after the proprietary periodPrimary source: JCMT project S16BP007: Venus at 266.94 GHz (RxA3/ACSIS), June 20171 step from the original
DocumentGreaves and colleagues · doi.org · 2020-09-14 · publisherPrimary source: Phosphine gas in the cloud decks of Venus2 steps from the original
DocumentGreaves and colleagues · arxiv.org · 2020-09-14 · arXiv-nonexclusivePrimary source: Phosphine gas in the cloud decks of Venus2 steps from the original
PhotoESO · eso.org · 2020-09-14 · CC BY 4.03 steps from the original
PictureALMA, Greaves et al. & JCMT · eso.org · CC BY 4.03 steps from the original
Where it was made
James Clerk Maxwell Telescope, Maunakea, Hawaii · Submillimetre telescope
Sources 2
Cite it
Mysteries Department. (2026). JCMT spectra of Venus at 266.94 GHz, June 2017 [Artifact ART0CQY25YY25G0]. https://mysteriesdept.com/r/ART0CQY25YY25G0
@misc{mysteriesdept_art0cqy25yy25g0,
title = {JCMT spectra of Venus at 266.94 GHz, June 2017},
author = {{Mysteries Department}},
year = {2026},
note = {Artifact, catalog key ART0CQY25YY25G0},
url = {https://mysteriesdept.com/r/ART0CQY25YY25G0}
}