trial signals have been found.

Source: en.wikipedia.org/wiki/SERENDIP

ugh data to prove that they belong to extraterrestrial intelligence. In September–October 2004 the media wrote about Radio source SHGb02+14a and its artificial origin, but scrutiny has not been able to confirm its connection with an extraterrestrial civilization. Currently no confirmed extraterres -

DIP VI was deployed in 2014 at both Arecibo and the Green Bank Telescope. SERENDIP VI will also look for fast radio bursts, in collaboration with scientists from University of Oxford and West Virginia University. •Findings: The program has found around 400 suspicious signals, but there is not eno -

led at the Arecibo Observatory in June 2009. The digital back-end instrument was an FPGA-based 128 million-channel digital spectrometer covering 200 MHz of bandwidth. It took data commensally with the seven-beam Arecibo L-band Feed Array (ALFA). The next generation of SERENDIP experiments, SEREN -

Bank Observatory and the Arecibo 305m telescope. SERENDIP observations have been conducted at frequencies between 400 MHz and 5 GHz, with most observations near the so-called Cosmic Water Hole (1.42 GHz (21 cm) neutral hydrogen and 1.66 GHz hydroxyl transitions). •Projects: SERENDIP V was instal -

channel analog radio spectrometer covering 100 kHz of bandwidth. Subsequent instruments have been significantly more capable, with the number of channels doubling roughly every year. These instruments have been deployed at a large number of telescopes including the NRAO 90m telescope at the Green -

stream" radio telescope observations as a "piggy-back" or "commensal" program. Rather than having its own observation program, SERENDIP analyzes deep space radio telescope data that it obtains while other astronomers are using the telescope. •Background: The initial SERENDIP instrument was a 100 -

SERENDIP (Search for Extraterrestrial Radio Emissions from Nearby Developed Intelligent Populations) is a Search for Extra-Terrestrial Intelligence (SETI) program originated by the Berkeley SETI Research Center at the University of California, Berkeley. SERENDIP takes advantage of ongoing "main -

dings, 1985.

Source: seti.berkeley.edu/SERENDIP.html

al. SERENDIP IV Data Acquisition Reduction and Analysis Paper. - Dan Werthimer et al. "The BERKELEY SETI Program, SERENDIP III and IV Instrumentation" Progress in the Search for Extraterrestrial Life, ASP Conference Series 1995. -Dan Werthimer et al. "The SERENDIP II Design" IAU Conference Procee -

lescope in West Virginia. •Additional information on SERENDIP and SERENDIP V.v: -Planetary Society's excellent article on SETI@home and SERENDIP V.v. -CASPER's technical description of the SERENDIP V.v instrument system. -Jeff Cobb et al. 1996 SIREN Conference Paper on SERENDIP IV. -Jeff Cobb et -

tential signatures of ETI. Although SERENDIP does not analyze data to the same level of detail as the computing power of SETI@home allows, it scans a broader range of frequencies. The data used in SERENDIP are currently taken using the Arecibo radio telescope in Puerto Rico, and the Green Bank Te -