Two new FRBs discovered by UTMOST

ATel #12124; W. Farah (Swinburne University of Technology "SUT"), M. Bailes (SUT), A. Jameson (SUT), C. Flynn (SUT), V. Gupta (SUT), T. Bateman (The University of Sydney "USyd"), E. D. Barr (Max-Planck-Institut fuer Radioastronomie "MPIfR"), S. Bhandari (CSIRO/ATNF), M. Caleb (University of Manchester), D. Campbell-Wilson (USyd), C. Day (SUT), A. Deller (SUT), A. J. Green (USyd), R. W. Hunstead (USyd), F. Jankowski (SUT), E. F. Keane (Square Kilometer Array Organisation), M. E. Lower (SUT), S. Oslowski (SUT), A. Parthasarathy (SUT), K. Plant (Caltech), D. C. Price (SUT), V. Ravi (Harvard-Smithsonian Center for Astrophysics), R. M. Shannon (SUT), A. Sutherland (USyd), D. Temby (USyd), G. Torr (USyd), G. Urquhart (USyd), V. Venkatraman Krishnan (MPIfR)
on 18 Oct 2018; 09:13 UT
Distributed as an Instant Email Notice Transients
Credential Certification: Wael Farah (wfarah@swin.edu.au)

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At UTC 2018-10-16-04:16:56.3 (2018-10-16.1795823), we found a bright fast radio burst as part of the ongoing search program (UTMOST), at the Molonglo telescope.

A second, unrelated FRB (FRB181017) was found the following day at UTC 2018-10-17-10:24:37.4 (2018-10-17.4337662).

Molonglo is a 1.6 km long East-West array (Bailes et al 2017, PASA, 34, 45) and was operating in drift-scan mode with pointing centred on the meridian at the time of detection. Source localisation is excellent in Right Ascension (5 arcsec at 1-sigma) but poor in Declination (~1.2 deg at 1-sigma) (see Caleb et al 2017 MNRAS 468, 3746).

FRB181016 and FRB181017 were found during a blind FRB search programme in real-time using an automated GPU-accelerated/machine learning based pipeline and the raw voltages were recorded for offline processing.

FRB181016: The optimal dispersion measure (DM) that maximizes the signal-to-noise ratio is: 1984 pc cm^-3. The DM estimate of NE2001 model is ~90 pc cm^-3, and YMW16 model is ~69 pc cm^-3 at this position, resulting in an intergalactic excess of ~1900 pc cm^-3. The upper limit on the DM-inferred redshift is thus z ~ 1.8.

An early estimate (lower limit) of the event's apparent fluence is ~ 70 Jy ms (corrected for attenuation of the primary beam in the RA direction, but not in the Dec direction), width ~ 6.88 ms, with a detection signal-to-noise ratio = 20.

The most likely position is RA = 15:46:20.5, DEC = -25:24:32, J2000, Galactic: Gl = 345.51 deg, Gb = 22.67 deg. The 95% confidence localisation arc is as follows: (RA, DEC) in (hours, deg)

15.769447 -28.263972
15.769986 -27.763111
15.770511 -27.262250
15.771028 -26.761389
15.771531 -26.260500
15.772025 -25.759639
15.772508 -25.258778
15.772983 -24.757917
15.773447 -24.257028
15.773900 -23.756167
15.774344 -23.255306
15.774781 -22.754417
15.775206 -22.253556

A formula describing the localisation arc is:
RA = 15.768768 - 1.106528e-3*(DEC - 25.409019) - 2.038129e-05*(DEC - 25.409019)**2,
where RA is in hours, Dec is in deg, and is valid in the Dec [-29.8,-21.1]

FRB180117: The dispersion measure (DM) that maximizes the signal-to-noise ratio is: 240 pc cm^-3. The DM estimate of NE2001 model is ~38 pc cm^-3, and YMW16 model is ~27 pc cm^-3 at the position of the FRB, resulting in an intergalactic excess of ~205 pc cm^-3. The upper limit on the DM-inferred redshift is thus z ~ 0.2.

An early estimate (lower limit) of the event's apparent fluence is ~ 95 Jy ms (corrected for attenuation of the primary beam in the RA direction, but not in the Dec direction), width ~ 2.6 ms, with a signal-to-noise ratio = 66.

The most likely position is RA =22:05:55 , DEC = -08:50:30, J2000, Galactic: Gl = 50.5 deg, Gb = -47.0 deg. The 95% confidence localisation arc is as follows: (RA, DEC) in (hours, deg)

22.098256 -11.698444
22.098303 -11.197472
22.098350 -10.696472
22.098403 -10.195500
22.098456 -9.694500
22.098511 -9.193528
22.098569 -8.692528
22.098631 -8.191556
22.098692 -7.690556
22.098756 -7.189583
22.098822 -6.688583
22.098892 -6.187611

A formula describing the localisation arc is:
RA = 22.101947 +2.654839e-4*(DEC -8.943028) + 4.195246e-06*(DEC -8.9430278)**2
Where RA is in hours, Dec is in deg, and is valid in the Dec [-13.20,-4.68]

For the dispersion sweep, and the localisation plots, follow this link

Follow-up observations of the FRBs are encouraged.

Two new FRBs discovered by UTMOST