Issue |
A&A
Volume 640, August 2020
|
|
---|---|---|
Article Number | L4 | |
Number of page(s) | 9 | |
Section | Letters to the Editor | |
DOI | https://doi.org/10.1051/0004-6361/202038423 | |
Published online | 30 July 2020 |
Letter to the Editor
3HSP J095507.9+355101: A flaring extreme blazar coincident in space and time with IceCube-200107A
1
Institute for Advanced Study, Technische Universität München, Lichtenbergstrasse 2a, 85748 Garching bei München, Germany
e-mail: giommipaolo@gmail.com
2
Associated to Agenzia Spaziale Italiana, ASI, Via del Politecnico s.n.c., 00133 Roma, Italy
3
ICRANet, Piazzale della Repubblica 10, 65122 Pescara, Italy
4
European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany
5
Associated to INAF – Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monteporzio Catone, Italy
6
Technische Universität München, Physik-Department, James-Frank-Str. 1, 85748 Garching bei München, Germany
7
Institutt for fysikk, NTNU, Trondheim, Norway
8
INAF – Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monteporzio Catone, Italy
9
INAF – IASF Milano, Via Corti 12, 20133 Milano, Italy
Received:
15
May
2020
Accepted:
5
July
2020
The uncertainty region of the highly energetic neutrino IceCube200107A includes 3HSP J095507.9+355101 (z = 0.557), an extreme blazar, which was detected in a high, very hard, and variable X-ray state shortly after the neutrino arrival. Following a detailed multiwavelength investigation, we confirm that the source is a genuine BL Lac. This new detection differs from TXS 0506+056, which is thus far the first source associated with IceCube neutrinos, and is considered a “masquerading” BL Lac. As in the case of TXS 0506+056, 3HSP J095507.9+355101 is also way off the so-called blazar sequence. We consider 3HSP J095507.9+355101 a possible counterpart to the IceCube neutrino. Finally, we discuss some theoretical implications in terms of neutrino production.
Key words: neutrinos / radiation mechanisms: non-thermal / galaxies: active / gamma rays: galaxies / BL Lacertae objects: general
© ESO 2020
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.