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J/PASP/129/E4501  Search for extraterrestrial intelligence     (Isaacson+, 2017)

The Breakthrough Listen search for intelligent life: target selection of nearby stars and galaxies. Isaacson H., Siemion A.P.V., Marcy G.W., Lebofsky M., Price D.C., Macmahon D., Croft S., Deboer D., Hickish J., Werthimer D., Sheikh S., Hellbourg G., Enriquez J.E. <Publ. Astron. Soc. Pac., 129, part no 5, 4501-54501 (2017)> =2017PASP..129e4501I (SIMBAD/NED BibCode)
ADC_Keywords: Stars, nearby Keywords: extraterrestrial intelligence - methods: observational Abstract: We present the target selection for the Breakthrough Listen search for extraterrestrial intelligence during the first year of observations at the Green Bank Telescope, Parkes Telescope, and Automated Planet Finder. On the way to observing 1,000,000 nearby stars in search of technological signals, we present three main sets of objects we plan to observe in addition to a smaller sample of exotica. We chose the 60 nearest stars, all within 5.1pc from the Sun. Such nearby stars offer the potential to observe faint radio signals from transmitters that have a power similar to those on Earth. We add a list of 1649 stars drawn from the Hipparcos catalog that span the Hertzprung-Russell diagram, including all spectral types along the main sequence, subgiants, and giant stars. This sample offers diversity and inclusion of all stellar types, but with thoughtful limits and due attention to main sequence stars. Our targets also include 123 nearby galaxies composed of a "morphological-type-complete" sample of the nearest spirals, ellipticals, dwarf spherioidals, and irregulars. While their great distances hamper the detection of technological electromagnetic radiation, galaxies offer the opportunity to observe billions of stars simultaneously and to sample the bright end of the technological luminosity function. We will also use the Green Bank and Parkes telescopes to survey the plane and central bulge of the Milky Way. Finally, the complete target list includes several classes of exotica, including white dwarfs, brown dwarfs, black holes, neutron stars, and asteroids in our solar system. Description: The stellar sample is defined by two selection criteria. The first is a volume-limited sample of stars within 5pc of the Sun. The second is a spectral class complete sample consisting of stars across the main sequence and some giant branch stars, all within 50pc. We combined the two sub-samples (5pc and 5-50pc) to produce the final set of 1709 target stars that are listed in Table 1. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 68 1709 Stellar Targets
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 9 A9 --- Star Star name 11- 12 I2 h RAh Right ascension (J2000) 14- 15 I2 min RAm Right ascension (J2000) 17- 20 F4.1 s RAs Right ascension (J2000) 23 A1 --- DE- Declination sign (J2000) 24- 25 I2 deg DEd Declination (J2000) 27- 28 I2 arcmin DEm Declination (J2000) 30- 31 I2 arcsec DEs Declination (J2000) 33- 36 I4 yr Ep [2000] Epoch 38- 42 F5.2 mag Vmag V magnitude 44- 50 A7 --- SpType Spectral type 52- 56 F5.2 pc Dist Distance 58- 62 F5.2 arcsec/yr pmRA Proper motion along RA, pmRA*cosDE 64- 68 F5.2 arcsec/yr pmDE Proper motion along DE
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 07-Aug-2017
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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