2023MNRAS.523.2219A


Query : 2023MNRAS.523.2219A

2023MNRAS.523.2219A - Mon. Not. R. Astron. Soc., 523, 2219-2235 (2023/August-1)

Bursts from Space: MeerKAT - the first citizen science project dedicated to commensal radio transients.

ANDERSSON A., LINTOTT C., FENDER R., BRIGHT J., CAROTENUTO F., DRIESSEN L., ESPINASSE M., GASEALAHWE K., HEYWOOD I., VAN DER HORST A.J., MOTTA S., RHODES L., TREMOU E., WILLIAMS D.R.A., WOUDT P., ZHANG X., BLOEMEN S., GROOT P., VREESWIJK P., GIARRATANA S., SAIKIA P., ANDERSSON J., ARROYO L.R., BAERT L., BAUMANN M., DOMAINKO W., ESCHWEILER T., FORSYTHE T., GAUDENZI S., GRENIER R.A., IANNONE D., LAHOZ K., MELVILLE K.J., NASCIMENTO M.D.S., NAVARRO L., PARTHASARATHI S., PIILONEN, RAHMAN N., SMITH J., STEWART B., TEMOKE N., TWOREK C. and WHITTLE I.

Abstract (from CDS):

The newest generation of radio telescopes is able to survey large areas with high sensitivity and cadence, producing data volumes that require new methods to better understand the transient sky. Here, we describe the results from the first citizen science project dedicated to commensal radio transients, using data from the MeerKAT telescope with weekly cadence. Bursts from Space: MeerKAT was launched late in 2021 and received ∼89 000 classifications from over 1000 volunteers in 3 months. Our volunteers discovered 142 new variable sources which, along with the known transients in our fields, allowed us to estimate that at least 2.1 per cent of radio sources are varying at 1.28 GHz at the sampled cadence and sensitivity, in line with previous work. We provide the full catalogue of these sources, the largest of candidate radio variables to date. Transient sources found with archival counterparts include a pulsar (B1845-01) and an OH maser star (OH 30.1-0.7), in addition to the recovery of known stellar flares and X-ray binary jets in our observations. Data from the MeerLICHT optical telescope, along with estimates of long time-scale variability induced by scintillation, imply that the majority of the new variables are active galactic nuclei. This tells us that citizen scientists can discover phenomena varying on time-scales from weeks to several years. The success both in terms of volunteer engagement and scientific merit warrants the continued development of the project, while we use the classifications from volunteers to develop machine learning techniques for finding transients.

Abstract Copyright: © The Author(s) 2023. Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): surveys - radio continuum: galaxies - radio continuum: general - radio continuum: transients

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR.

Simbad objects: 23

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Number of rows : 23
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SDSS J094103.80+344334.1 G 09 41 03.80160 +34 43 34.1148           ~ 100 0
2 IC 2497 rG 09 41 04.1049384864 +34 43 58.172413980           ~ 90 1
3 MAXI J1348-630 HX? 13 48 12.7388336424 -63 16 29.709083208           ~ 201 0
4 V* IL Lup HXB 15 47 08.2768672752 -47 40 10.284587760         15.624 ~ 532 1
5 V* V821 Ara LXB 17 02 49.3876391280 -48 47 23.087954544         15.322 ~ 2237 0
6 PSR J1703-4902 Psr 17 03 54.54100 -48 52 01.0400           ~ 42 0
7 TYC 8332-2529-1 SB* 17 04 56.2556998776 -48 21 00.578413800   12.06 11.15     ~ 8 0
8 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
9 NAME XTE J17464-3213 LXB 17 46 15.59637 -32 14 00.8600           ~ 805 0
10 SCR J1746-3214 PM* 17 46 40.6585966320 -32 14 04.504387560   17.94   15.89 12.71 M5.5 17 0
11 MAXI J1803-298 BH? 18 03 41.0 -29 48 14           ~ 69 0
12 SAX J1808.4-3658 LXB 18 08 27.58 -36 58 43.9           ~ 1051 0
13 NVSS J181752+064638 rG 18 17 52.63491120 +06 46 38.1510840           ~ 6 1
14 NVSS J181849+062843 Rad 18 18 49.22 +06 28 43.1           ~ 2 0
15 VLASS1QLCIR J181955.28+074418.7 cm 18 19 55.28676 +07 44 18.7317           ~ 1 0
16 MAXI J1820+070 LXB 18 20 21.9423816480 +07 11 07.284859440           ~ 511 0
17 NVSS J182029+063419 Rad 18 20 29.94 +06 34 19.0           ~ 2 0
18 PSR B1845-01 Psr 18 48 23.59600 -01 23 58.4800           ~ 154 0
19 OH 030.1-00.7 OH* 18 48 41.98728 -02 50 29.5080           O-rich 107 0
20 AX J1848.8-0129 X 18 48 48 -01 29.2           ~ 27 0
21 EXO 1846-031 LXB 18 49 17.1 -03 03 44           ~ 114 0
22 SWIFT J1858.6-0814 XB* 18 58 34.91 -08 14 14.8           ~ 76 0
23 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2810 0

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