Multibeam Blind Search of Targeted SETI Observations toward 33 Exoplanet Systems with FAST
arXiv:2301.10890 · doi:10.3847/1538-3881/acb706
Abstract
The search for extraterrestrial intelligence (SETI) is to search for technosignatures associated with extraterrestrial life, such as engineered radio signals. In this paper, we apply the multibeam coincidence matching (MBCM) strategy, and propose a new search mode based on the MBCM which we call MBCM blind search mode. In our recent targeted SETI research, 33 exoplanet systems are observed by the Five-hundred-meter Aperture Spherical radio Telescope (FAST). With this blind search mode, we search for narrowband drifting signals across GHz in two orthogonal linear polarization directions separately. There are two special signals, one of which can only be detected by the blind search mode while the other can be found by both blind and targeted search modes. This result reveals huge advantages of the new blind search mode. However, we eliminate the possibility of the special signals being ETI signals based on much evidence, such as the polarization, drift, frequency and beam coverage characteristics. Our observations achieve an unprecedented sensitivity and our work provides a deeper understanding to the polarization analysis of extraterrestrial signals.
arXiv comment15 pages, 1 table, 7 figures. Matches AJ published version. Based on MBCM strategy by Zhen-Zhao Tao et al (2022 AJ 164 160), we propose a new search mode: MBCM blind search mode for FAST SETI observations
References in corpus (32)
- Habitable Zones Around Main-Sequence Stars: New Estimates
- The Five-Hundred-Meter Aperture Spherical Radio Telescope (FAST) Project
- Prevalence of Earth-size planets orbiting Sun-like stars
- The Occurrence Rate of Small Planets around Small Stars
- Biosignatures from Earth-Like Planets Around M Dwarfs
- The Fundamental Performance of FAST with 19-beam Receiver at L Band
- Exploring Exoplanet Populations with NASA's Kepler Mission
- Feasibility Studies for the Detection of in an Earth-like Exoplanet
- The Breakthrough Listen Search for Intelligent Life: 1.1-1.9 GHz observations of 692 Nearby Stars
- The Breakthrough Listen Search for Intelligent Life: Observations of 1327 Nearby Stars over 1.10-3.45 GHz
- The Five-hundred-meter Aperture Spherical Radio Telescope (FAST) Project
- A 1.1 to 1.9 GHz SETI Survey of the Kepler Field: I. A Search for Narrow-band Emission from Select Targets
- Identifying Planetary Biosignature Impostors: Spectral Features of CO and O4 Resulting from Abiotic O2/O3 Production
- The SUrvey for Pulsars and Extragalactic Radio Bursts I: Survey Description and Overview
- The Breakthrough Listen Search for Intelligent Life: A Wideband Data Recorder System for the Robert C. Byrd Green Bank Telescope
- The Breakthrough Listen Search For Intelligent Life Near the Galactic Center I
- SETI Observations of Exoplanets with the Allen Telescope Array
- The Breakthrough Listen Search for Intelligent Life: A 3.95-8.00 GHz Search for Radio Technosignatures in the Restricted Earth Transit Zone
- First SETI Observations with China's Five-hundred-meter Aperture Spherical radio Telescope (FAST)
- A Fast Radio Burst discovered in FAST drift scan survey
- A VLA Search for Radio Signals from M31 and M33
- A Search for Technosignatures Around 31 Sun-like Stars with the Green Bank Telescope at 1.15-1.73 GHz
- A radio technosignature search towards Proxima Centauri resulting in a signal-of-interest
- An Opportunistic Search for ExtraTerrestrial Intelligence (SETI) with the Murchison Widefield Array
- A search for technosignatures from TRAPPIST-1, LHS 1140, and 10 planetary systems in the Kepler field with the Green Bank Telescope at 1.15-1.73 GHz
- The Breakthrough Listen Search for Intelligent Life: Searching for Technosignatures in Observations of TESS Targets of Interest
- Drift Rates of Narrowband Signals in Long-term SETI Observations for Exoplanets
- Sensitive Multi-beam Targeted SETI Observations towards 33 Exoplanet Systems with FAST
- Past, Present and Future Stars that can see Earth as a Transiting Exoplanet
- A search for Extraterrestrial Intelligence (SETI) toward the Galactic Anticenter with the Murchison Widefield Array
- A SETI Survey of the Vela Region using the Murchison Widefield Array: Orders of Magnitude Expansion in Search Space
- The Application of Autocorrelation SETI Search Techniques in an ATA Survey
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- SETI@home: Data Analysis and Findings
- The FAST-SETI Milky Way Globular Cluster Survey I: A Pilot Multibeam On-the-Fly Search of Five Globular Clusters at L-Band
- Theoretical Radio Signals from Radio-Band Gravitational Waves Converted from the Neutron Star Magnetic Field
- Estimating Cosmological Parameters and Reconstructing Hubble Constant with Artificial Neural Networks: A Test with covariance matrix and mock H(z)
- Dual-Backend Multibeam Position Switching Targeted SETI Observations toward Nearby Active Planet-Hosting Systems with FAST
- SETI@home: Data Acquisition and Front-End Processing
- Undetected past contacts with technological species: implications for technosignature science
- An Improved Machine Learning Approach for Radio Frequency Interference Mitigation in FAST-SETI Survey Archival Data