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originally posted by: bobw927
is it AM , FM , Upper or Lower side Band , FSK, RTTY, Packet , or ASCII and what Frequency Range ???
originally posted by: bobw927
is it AM , FM , Upper or Lower side Band , FSK, RTTY, Packet , or ASCII and what Frequency Range ???
Although unlikely, there is also a possibility that the signals are due to highly peculiar chemical compositions in a small fraction of galactic halo stars.
No known natural sources would produce such a signal. Bell and Hewish began to rule out various sources of human interference, including other radio astronomers, radar reflected off the moon, television signals, orbiting satellites, and even possible effects from a large corrugated metal building near the telescope. None of those could explain the strange signal.
originally posted by: projectvxn
This is my favorite thread of all time here and it deserves far more attention than its getting.
Astronomy Magazine: Be extraordinarily cautious about the newest alien claim
“Apparently several — more than three or four — referees have been disinclined to see this published. I am quite skeptical, in particular of the data processing that can take spectrally sampled data, and infer time variations. So I’d be a little careful.” (Seth Shostak, senior astronomer at the SETI Institute)
“Punch line is that this is interesting but needs to be followed up on other facilities, which we will be doing with Breakthrough Listen” (Andrew Siemion, director of SETI Berkeley)
The SETI protocol holds that researchers should seek confirmation prior to publishing. In this case, it was the other way around. But with the astronomy community now being engaged, I guess we'll soon know more!
The Berkeley SETI Research Center (BSRC) team has added several stars from the Borra and Trottier sample to the Breakthrough Listen observing queue on the 2.4-meter Automated Planet Finder (APF) optical telescope.
The capabilities of the APF spectrograph are well matched to those of the original detection, and these independent follow-up observations will enable us to verify or refute the reported detections. We look forward to consulting with Professor Borra and his team on these observations, as well as additional follow up investigations using other data sources.
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