A SETI Survey of the Vela Region using the Murchison Widefield Array: Orders of Magnitude Expansion in Search Space. (arXiv:2009.03267v1 [astro-ph.IM])
<a href="http://arxiv.org/find/astro-ph/1/au:+Tremblay_C/0/1/0/all/0/1">Chenoa D. Tremblay</a>, <a href="http://arxiv.org/find/astro-ph/1/au:+Tingay_S/0/1/0/all/0/1">Steven J. Tingay</a>
Following the results of our previous low frequency searches for
extraterrestrial intelligence (SETI) using the Murchison Widefield Array (MWA),
directed toward the Galactic Centre and the Orion Molecular Cloud (Galactic
Anticentre), we report a new large-scale survey toward the Vela region with the
lowest upper limits thus far obtained with the MWA. Using the MWA in the
frequency range 98-128 MHz over a 17 hour period, a $sim$400 deg$^2$ field
centred on the Vela Supernova Remnant was observed with a frequency resolution
of 10 kHz. Within this field there are six known exoplanets. At the positions
of these exoplanets, we searched for narrow band signals consistent with radio
transmissions from intelligent civilizations. No unknown signals were found
with a 5sigma detection threshold. In total, across this work plus our two
previous surveys, we have now examined 75 known exoplanets at low frequencies.
In addition to the known exoplanets, we have included in our analysis the
calculation of the Effective Isotropic Radiated Power (EIRP) upper limits
toward over 10 million stellar sources in the Vela field with known distances
from Gaia (assuming a 10 kHz transmission bandwidth).
Following the results of our previous low frequency searches for
extraterrestrial intelligence (SETI) using the Murchison Widefield Array (MWA),
directed toward the Galactic Centre and the Orion Molecular Cloud (Galactic
Anticentre), we report a new large-scale survey toward the Vela region with the
lowest upper limits thus far obtained with the MWA. Using the MWA in the
frequency range 98-128 MHz over a 17 hour period, a $sim$400 deg$^2$ field
centred on the Vela Supernova Remnant was observed with a frequency resolution
of 10 kHz. Within this field there are six known exoplanets. At the positions
of these exoplanets, we searched for narrow band signals consistent with radio
transmissions from intelligent civilizations. No unknown signals were found
with a 5sigma detection threshold. In total, across this work plus our two
previous surveys, we have now examined 75 known exoplanets at low frequencies.
In addition to the known exoplanets, we have included in our analysis the
calculation of the Effective Isotropic Radiated Power (EIRP) upper limits
toward over 10 million stellar sources in the Vela field with known distances
from Gaia (assuming a 10 kHz transmission bandwidth).
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