2021A&A...655A..16M


Query : 2021A&A...655A..16M

2021A&A...655A..16M - Astronomy and Astrophysics, volume 655A, 16-16 (2021/11-1)

First results from the REAL-time Transient Acquisition backend (REALTA) at the Irish LOFAR station.

MURPHY P.C., CALLANAN P., McCAULEY J., McKENNA D.J., FIONNAGAIN D.O., LOUIS C.K., REDMAN M.P., CANIZARES L.A., CARLEY E.P., MALONEY S.A., COGHLAN B., DALY M., SCULLY J., DOOLEY J., GAJJAR V., GIESE C., BRENNAN A., KEANE E.F., MAGUIRE C.A., QUINN J., MOONEY S., RYAN A.M., WALSH J., JACKMAN C.M., GOLDEN A., RAY T.P., DOYLE J.G., RIGNEY J., BURTON M. and GALLAGHER P.T.

Abstract (from CDS):

Modern radio interferometers such as the LOw Frequency ARray (LOFAR) are capable of producing data at hundreds of gigabits to terabits per second. This high data rate makes the analysis of radio data cumbersome and computationally expensive. While high performance computing facilities exist for large national and international facilities, that may not be the case for instruments operated by a single institution or a small consortium. Data rates for next generation radio telescopes are set to eclipse those currently in operation, hence local processing of data will become all the more important. Here, we introduce the REAL-time Transient Acquisition backend (REALTA), a computing backend at the Irish LOFAR station (I-LOFAR) which facilitates the recording of data in near real-time and post-processing. We also present first searches and scientific results of a number of radio phenomena observed by I-LOFAR and REALTA, including pulsars, fast radio bursts, rotating radio transients, the search for extraterrestrial intelligence, Jupiter, and the Sun.

Abstract Copyright: © ESO 2021

Journal keyword(s): instrumentation: miscellaneous - methods: data analysis - telescopes

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 FRB 20180916B rB 01 58 00.750 +65 43 00.30           ~ 313 0
2 M 1 SNR 05 34 30.9 +22 00 53           ~ 6192 1
3 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5259 0
4 PSR B1919+21 Psr 19 21 44.815 +21 53 02.25           ~ 384 0
5 PSR B2217+47 Psr 22 19 48.139 +47 54 53.93           ~ 219 0

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