A Search for Monochromatic Light Toward the Galactic Centre
G. Marcy, N. Tellis, и E. Wishnow. (2022)cite arxiv:2208.13561Comment: Published in Monthly Notices of the Royal Astronomical Society.
Аннотация
A region 140 square degrees toward the Galactic Centre was searched for
monochromatic optical light, both pulses shorter than 1 sec and continuous
emission. A novel instrument was constructed that acquires optical spectra of
every point within 6 square degrees every second, able to distinguish lasers
from astrophysical sources. The system consists of a modified Schmidt
telescope, a wedge prism over the 0.28-meter aperture, and a fast CMOS camera
with 9500 x 6300 pixels. During 2021, a total of 34800 exposures were obtained
and analyzed for monochromatic sources, both sub-second pulses and continuous
in time. No monochromatic light was found. A benchmark laser with a 10-meter
aperture and located 100 light years away would be detected if it had a power
more than ~60 megawatt during 1 sec, and from 1000 light years away, 6000 MW is
required. This non-detection of optical lasers adds to previous optical SETI
non-detections from more than 5000 nearby stars of all masses, from the Solar
gravitational lens focal points of Alpha Centauri, and from all-sky searches
for broadband optical pulses. These non-detections, along with those of
broadband pulses, constitute a growing SETI desert in the optical domain.
Описание
A Search for Monochromatic Light Toward the Galactic Centre
%0 Generic
%1 marcy2022search
%A Marcy, Geoffrey W.
%A Tellis, Nathaniel K.
%A Wishnow, Edward H.
%D 2022
%K tifr
%T A Search for Monochromatic Light Toward the Galactic Centre
%U http://arxiv.org/abs/2208.13561
%X A region 140 square degrees toward the Galactic Centre was searched for
monochromatic optical light, both pulses shorter than 1 sec and continuous
emission. A novel instrument was constructed that acquires optical spectra of
every point within 6 square degrees every second, able to distinguish lasers
from astrophysical sources. The system consists of a modified Schmidt
telescope, a wedge prism over the 0.28-meter aperture, and a fast CMOS camera
with 9500 x 6300 pixels. During 2021, a total of 34800 exposures were obtained
and analyzed for monochromatic sources, both sub-second pulses and continuous
in time. No monochromatic light was found. A benchmark laser with a 10-meter
aperture and located 100 light years away would be detected if it had a power
more than ~60 megawatt during 1 sec, and from 1000 light years away, 6000 MW is
required. This non-detection of optical lasers adds to previous optical SETI
non-detections from more than 5000 nearby stars of all masses, from the Solar
gravitational lens focal points of Alpha Centauri, and from all-sky searches
for broadband optical pulses. These non-detections, along with those of
broadband pulses, constitute a growing SETI desert in the optical domain.
@misc{marcy2022search,
abstract = {A region 140 square degrees toward the Galactic Centre was searched for
monochromatic optical light, both pulses shorter than 1 sec and continuous
emission. A novel instrument was constructed that acquires optical spectra of
every point within 6 square degrees every second, able to distinguish lasers
from astrophysical sources. The system consists of a modified Schmidt
telescope, a wedge prism over the 0.28-meter aperture, and a fast CMOS camera
with 9500 x 6300 pixels. During 2021, a total of 34800 exposures were obtained
and analyzed for monochromatic sources, both sub-second pulses and continuous
in time. No monochromatic light was found. A benchmark laser with a 10-meter
aperture and located 100 light years away would be detected if it had a power
more than ~60 megawatt during 1 sec, and from 1000 light years away, 6000 MW is
required. This non-detection of optical lasers adds to previous optical SETI
non-detections from more than 5000 nearby stars of all masses, from the Solar
gravitational lens focal points of Alpha Centauri, and from all-sky searches
for broadband optical pulses. These non-detections, along with those of
broadband pulses, constitute a growing SETI desert in the optical domain.},
added-at = {2022-08-30T07:43:35.000+0200},
author = {Marcy, Geoffrey W. and Tellis, Nathaniel K. and Wishnow, Edward H.},
biburl = {https://www.bibsonomy.org/bibtex/20466a30cd8c2e1945017018cc8b63c15/citekhatri},
description = {A Search for Monochromatic Light Toward the Galactic Centre},
interhash = {6578b8517a9586890fa13dfe17f858c3},
intrahash = {0466a30cd8c2e1945017018cc8b63c15},
keywords = {tifr},
note = {cite arxiv:2208.13561Comment: Published in Monthly Notices of the Royal Astronomical Society},
timestamp = {2022-08-30T07:43:35.000+0200},
title = {A Search for Monochromatic Light Toward the Galactic Centre},
url = {http://arxiv.org/abs/2208.13561},
year = 2022
}