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Preferred frequency for interstellar communications
It is suggested that the 4829.659-MHz line frequency of the1(11)-to-1(10) rotational transition of formaldehyde is a plausiblefrequency to monitor for the purpose of detecting interstellarcommunications. The formaldehyde line is of interest because, as aresult of the antimaser effect, it exhibits a very low excitationtemperature. The background radiation temperature in the direction ofdark clouds is below the 3 K background temperature; the backgroundnoise temperature, lowered approximately 1 K, is lower than at any otherfrequency band.
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Observation and Astrometry data
| Constellation: | Μυία |
| Right ascension: | 13h04m26.90s |
| Declination: | -64°47'25.4" |
| Apparent magnitude: | 8.537 |
| Distance: | 584.795 parsecs |
| Proper motion RA: | -10.2 |
| Proper motion Dec: | -6.4 |
| B-T magnitude: | 10.586 |
| V-T magnitude: | 8.707 |
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