Exploring the Breakthrough Listen Investigation for Periodic Spectral Signals (BLIPSS)

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Akshay Suresh, a graduate student at Cornell University, spearheads the Breakthrough Listen Investigation for Periodic Spectral Signals (BLIPSS) — a collaborative project between Cornell University, the SETI Institute, and Breakthrough Listen — to detect repetitive signals from the Milky Way’s core as potential evidence of extraterrestrial life. By focusing on dense star clusters and using a narrow frequency range, BLIPSS amplifies the odds of capturing compelling evidence of extraterrestrial technology.


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Cornell University’s Akshay Suresh is leading the Breakthrough Listen Investigation for Periodic Spectral Signals (BLIPSS), a project focused on detecting repetitive signals from the Milky Way’s core as potential evidence of extraterrestrial life. By focusing on dense star clusters and using a narrow frequency range, BLIPSS aims to detect signals that could be evidence of alien technology.

Akshay Suresh, a graduate student at Cornell University, spearheads an extraordinary scientific endeavor — a groundbreaking mission to uncover periodic signals emanating from the core of the Milky Way called the Breakthrough Listen Investigation for Periodic Spectral Signals (BLIPSS). Such repetitive patterns could be the key to unlocking the mysteries of extraterrestrial intelligence in our galaxy. Suresh and his co-authors detail the project’s results thus far in a paper that was recently published in the Astronomical Journal, "A 4–8 GHz Galactic Center Search for Periodic Technosignatures." .

BLIPSS aims to detect signals between 4-8GHz frequency range

BLIPSS is a collaboration between Cornell University, the SETI Institute, and Breakthrough Listen. By directing their focus towards the central region of the Milky Way, with its dense congregation of stars and possibly habitable exoplanets, the BLIPSS team amplifies the odds of capturing compelling evidence of extraterrestrial technology. If an alien civilization wanted to communicate with other civilizations throughout the Milky Way, the galaxy’s core holds potential as a strategic site for a beacon.

BLIPSS is a collaboration between Cornell University, the SETI Institute, and Breakthrough Listen

"BLIPSS showcases the cutting-edge potential of software as a science multiplier for SETI," said Suresh.

SETI Institute Astronomer Dr. Vishal Gajjar is one of Suresh’s advisors on the project. "Until now, radio SETI has primarily dedicated its efforts to the search for continuous signals," said Gajjar. "Our study sheds light on the remarkable energy efficiency of a train of pulses as a means of interstellar communication across vast distances. Notably, this study marks the first-ever comprehensive endeavor to conduct in-depth searches for these signals." .

BLIPSS uses the Breakthrough Listen instrument on the Green Bank Telescope (GBT)

The team began by testing their algorithm on known pulsars, successfully detecting the expected periodic emissions. Subsequently, they turned their attention to a dataset of scans of the Galactic Center captured by the Breakthrough Listen instrument on the Green Bank Telescope (GBT) in West Virginia. Unlike pulsars, which emit signals across a broad range of radio frequencies, BLIPSS narrowed its search to repeating signals within a narrower frequency range—covering less than a tenth of the width of an average FM radio station.

BLIPSS searches for periodic patterns in the signals, which could signify deliberate technological activities

Dr. Steve Croft, the Breakthrough Listen Project Scientist for GBT and Adjunct Senior Astronomer at the SETI Institute, highlighted the significance of this approach, as it combines narrow bandwidths with periodic patterns that could signify deliberate technological activities by intelligent civilizations. Suresh’s technique presents a novel methodology to sift through this metaphorical haystack, enabling the team to identify tantalizing evidence of advanced extraterrestrial life forms.

The team began by testing their algorithm on known pulsars, and then focused on a dataset of scans of the Galactic Center

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