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Follow up of the IceCube alerts with the Baikal-GVD telescope

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Follow up of the IceCube alerts with the Baikal-GVD telescope

Viktoriya Dik

on behalf of the Baikal-GVD collaboration Supervisors:

Shaybonov B. A., Suvorova O. V.

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Content of the work

Baikal-GVD monitors online alerts from IceCube since August 2020.

The aim of this work is the search for correlation in direction and time of the signal in IceCube notifications with events

reconstructed from Baikal-GVD data for muon and cascade

modes.

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Baikal Gigaton Volume Detector

Effective volume for Baikal-GVD in 2021

— 0.4 kм3 for ν with E>100 TeV.

One cluster's volume is 0.05 km3.

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Data transfer and processing scheme

See also B. Shaybonov talk

Time delays:

1. Few minutes from shore

2. Few hours in data processing ~ lake noises

Telescope

DAQ Storage

Processing Online

Analysis User

analysis

Quasi online Analysis

Deep

underwater Shore station Computing Center at Dubna

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Muon track and cascade reconstruction

The distribution of the

mismatch angles between MC neutrinos with an energy spectrum of E-2 and reconstructed muon trajectories.

Selection muon neutrino cuts reject events with Zen < 120º.

The distribution of events by angle between the simulated and reconstructed shower directions for one cluster.

For cascade reconstruction algorithm and cuts see also M. Shelepov talk

median angle ~ 1.27°

median angle ~ 4.5°

For muon reconstruction

algorithm see talks of D. Zaborov and G. Safronov

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Sky locations of IceCube events in +/- 12 h from alert time

Seven start points of events with 92º<Zen<124º -> Muon

reconstruction is low efficient for one cluster mode

Source below horizonSource above horizon

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Three IC events tracks with the same visibility

The cascade ★ event rate is within

background estimate

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Example: search for neutrinos around IC201120A Bronze by cascades

Cuts for cascades on χ2, LLH, OM’s probability hit/

non hit, Nhit>7.

Cone ψ < 5º between the direction of the event and the alert IC201120A.

weight = 1/ψ

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GVD cascade events with cone ψ< 5º in ±30 days around IC alerts in Aug 2020-Sep 2020

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GVD cascade events with cone ψ< 5º in ±30 days around IC alerts in Oct 2020

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GVD cascade events with cone ψ< 5º in ±30 days around IC alerts in Nov 2020

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GVD cascade events with cone ψ< 5º in ±30 days around IC alerts in Dec 2020 and Feb 2021

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Example: upper limit on fluence for IC201014A

For all clusters 2020 with cuts Data

Back

Track of IC201014A

Nbg = 0.44, Nobs = 1,

P-value =0.36, n90% = 4.36 Expos = 1787 TeV-1 cm2

E-2F = n90%/Expos = 2.44 . 10-3 Tev cm-2

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Results by GVD cascade events

Publ. In A. D. Avrorin et al. HIGH ENERGY NEUTRINO FOLLOW UP WITH BAIKAL-GVD, Astronomy Letters 2021-02-01

For IC200926B, IC200929A, IC201014A Nobs= 1 in +/- 12 h.

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Summary

The Baikal-GVD neutrino telescope has been monitoring alerts from IceCube neutrino telescope in quasi online regime.

In cascade mode reconstruction the search of the concidences was done in cone 5° and ±12 h.

For energy range 1TeV - 10PeV and assumption of E-2 spectrum in the source and equal fluence in all flavors the upper limits on neutrino fluence were found:

1÷2 GeV/cm2. The results were obtained for cascades and single clusters.

Latest IC alerts in May were also tested.

Referencias

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