Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A
<strong>INTRODUCTION</strong> Neutrinos are tracers of cosmic-ray acceleration: electrically neutral and traveling at nearly the speed of light, they can escape the densest environments and may be traced back to their source of origin. High-energy neutrinos are expected to be produced in...
| Main Authors: | , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Journal article |
| Published: |
American Association for the Advancement of Science
2018
|
| _version_ | 1797103795879018496 |
|---|---|
| author | IceCube Collaboration Fermi-LAT MAGIC AGILE ASAS-SN HAWC H.E.S.S. INTEGRAL Kanata Kiso Kapteyn Liverpool Telescope Subaru Swift/NuSTAR VERITAS VLA/17B-403 teams Sarkar, S |
| author_facet | IceCube Collaboration Fermi-LAT MAGIC AGILE ASAS-SN HAWC H.E.S.S. INTEGRAL Kanata Kiso Kapteyn Liverpool Telescope Subaru Swift/NuSTAR VERITAS VLA/17B-403 teams Sarkar, S |
| author_sort | IceCube Collaboration |
| collection | OXFORD |
| description | <strong>INTRODUCTION</strong> Neutrinos are tracers of cosmic-ray acceleration: electrically neutral and traveling at nearly the speed of light, they can escape the densest environments and may be traced back to their source of origin. High-energy neutrinos are expected to be produced in blazars: intense extragalactic radio, optical, x-ray, and, in some cases, γ-ray sources characterized by relativistic jets of plasma pointing close to our line of sight. Blazars are among the most powerful objects in the Universe and are widely speculated to be sources of high-energy cosmic rays. These cosmic rays generate high-energy neutrinos and γ-rays, which are produced when the cosmic rays accelerated in the jet interact with nearby gas or photons. On 22 September 2017, the cubic-kilometer IceCube Neutrino Observatory detected a ~290-TeV neutrino from a direction consistent with the flaring γ-ray blazar TXS 0506+056. We report the details of this observation and the results of a multiwavelength follow-up campaign. <strong>RATIONALE</strong> Multimessenger astronomy aims for globally coordinated observations of cosmic rays, neutrinos, gravitational waves, and electromagnetic radiation across a broad range of wavelengths. The combination is expected to yield crucial information on the mechanisms energizing the most powerful astrophysical sources. That the production of neutrinos is accompanied by electromagnetic radiation from the source favors the chances of a multiwavelength identification. In particular, a measured association of high-energy neutrinos with a flaring source of γ-rays would elucidate the mechanisms and conditions for acceleration of the highest-energy cosmic rays. The discovery of an extraterrestrial diffuse flux of high-energy neutrinos, announced by IceCube in 2013, has characteristic properties that hint at contributions from extragalactic sources, although the individual sources remain as yet unidentified. Continuously monitoring the entire sky for astrophysical neutrinos, IceCube provides real-time triggers for observatories around the world measuring γ-rays, x-rays, optical, radio, and gravitational waves, allowing for the potential identification of even rapidly fading sources. <strong>RESULTS</strong> A high-energy neutrino-induced muon track was detected on 22 September 2017, automatically generating an alert that was distributed worldwide within 1 min of detection and prompted follow-up searches by telescopes over a broad range of wavelengths. On 28 September 2017, the Fermi Large Area Telescope Collaboration reported that the direction of the neutrino was coincident with a cataloged γ-ray source, 0.1° from the neutrino direction. The source, a blazar known as TXS 0506+056 at a measured redshift of 0.34, was in a flaring state at the time with enhanced γ-ray activity in the GeV range. Follow-up observations by imaging atmospheric Cherenkov telescopes, notably the Major Atmospheric Gamma Imaging Cherenkov (MAGIC) telescopes, revealed periods where the detected γ-ray flux from the blazar reached energies up to 400 GeV. Measurements of the source have also been completed at x-ray, optical, and radio wavelengths. We have investigated models associating neutrino and γ-ray production and find that correlation of the neutrino with the flare of TXS 0506+056 is statistically significant at the level of 3 standard deviations (sigma). On the basis of the redshift of TXS 0506+056, we derive constraints for the muon-neutrino luminosity for this source and find them to be similar to the luminosity observed in γ-rays. <strong>CONCLUSION</strong> The energies of the γ-rays and the neutrino indicate that blazar jets may accelerate cosmic rays to at least several PeV. The observed association of a high-energy neutrino with a blazar during a period of enhanced γ-ray emission suggests that blazars may indeed be one of the long-sought sources of very-high-energy cosmic rays, and hence responsible for a sizable fraction of the cosmic neutrino flux observed by IceCube. |
| first_indexed | 2024-03-07T06:25:02Z |
| format | Journal article |
| id | oxford-uuid:f3fdc8da-3ae3-43ac-a335-6cb31f1f5bc1 |
| institution | University of Oxford |
| last_indexed | 2024-03-07T06:25:02Z |
| publishDate | 2018 |
| publisher | American Association for the Advancement of Science |
| record_format | dspace |
| spelling | oxford-uuid:f3fdc8da-3ae3-43ac-a335-6cb31f1f5bc12022-03-27T12:16:26ZMultimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922AJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:f3fdc8da-3ae3-43ac-a335-6cb31f1f5bc1Symplectic Elements at OxfordAmerican Association for the Advancement of Science2018IceCube CollaborationFermi-LATMAGICAGILEASAS-SNHAWCH.E.S.S.INTEGRALKanataKisoKapteynLiverpool TelescopeSubaruSwift/NuSTARVERITASVLA/17B-403 teamsSarkar, S<strong>INTRODUCTION</strong> Neutrinos are tracers of cosmic-ray acceleration: electrically neutral and traveling at nearly the speed of light, they can escape the densest environments and may be traced back to their source of origin. High-energy neutrinos are expected to be produced in blazars: intense extragalactic radio, optical, x-ray, and, in some cases, γ-ray sources characterized by relativistic jets of plasma pointing close to our line of sight. Blazars are among the most powerful objects in the Universe and are widely speculated to be sources of high-energy cosmic rays. These cosmic rays generate high-energy neutrinos and γ-rays, which are produced when the cosmic rays accelerated in the jet interact with nearby gas or photons. On 22 September 2017, the cubic-kilometer IceCube Neutrino Observatory detected a ~290-TeV neutrino from a direction consistent with the flaring γ-ray blazar TXS 0506+056. We report the details of this observation and the results of a multiwavelength follow-up campaign. <strong>RATIONALE</strong> Multimessenger astronomy aims for globally coordinated observations of cosmic rays, neutrinos, gravitational waves, and electromagnetic radiation across a broad range of wavelengths. The combination is expected to yield crucial information on the mechanisms energizing the most powerful astrophysical sources. That the production of neutrinos is accompanied by electromagnetic radiation from the source favors the chances of a multiwavelength identification. In particular, a measured association of high-energy neutrinos with a flaring source of γ-rays would elucidate the mechanisms and conditions for acceleration of the highest-energy cosmic rays. The discovery of an extraterrestrial diffuse flux of high-energy neutrinos, announced by IceCube in 2013, has characteristic properties that hint at contributions from extragalactic sources, although the individual sources remain as yet unidentified. Continuously monitoring the entire sky for astrophysical neutrinos, IceCube provides real-time triggers for observatories around the world measuring γ-rays, x-rays, optical, radio, and gravitational waves, allowing for the potential identification of even rapidly fading sources. <strong>RESULTS</strong> A high-energy neutrino-induced muon track was detected on 22 September 2017, automatically generating an alert that was distributed worldwide within 1 min of detection and prompted follow-up searches by telescopes over a broad range of wavelengths. On 28 September 2017, the Fermi Large Area Telescope Collaboration reported that the direction of the neutrino was coincident with a cataloged γ-ray source, 0.1° from the neutrino direction. The source, a blazar known as TXS 0506+056 at a measured redshift of 0.34, was in a flaring state at the time with enhanced γ-ray activity in the GeV range. Follow-up observations by imaging atmospheric Cherenkov telescopes, notably the Major Atmospheric Gamma Imaging Cherenkov (MAGIC) telescopes, revealed periods where the detected γ-ray flux from the blazar reached energies up to 400 GeV. Measurements of the source have also been completed at x-ray, optical, and radio wavelengths. We have investigated models associating neutrino and γ-ray production and find that correlation of the neutrino with the flare of TXS 0506+056 is statistically significant at the level of 3 standard deviations (sigma). On the basis of the redshift of TXS 0506+056, we derive constraints for the muon-neutrino luminosity for this source and find them to be similar to the luminosity observed in γ-rays. <strong>CONCLUSION</strong> The energies of the γ-rays and the neutrino indicate that blazar jets may accelerate cosmic rays to at least several PeV. The observed association of a high-energy neutrino with a blazar during a period of enhanced γ-ray emission suggests that blazars may indeed be one of the long-sought sources of very-high-energy cosmic rays, and hence responsible for a sizable fraction of the cosmic neutrino flux observed by IceCube. |
| spellingShingle | IceCube Collaboration Fermi-LAT MAGIC AGILE ASAS-SN HAWC H.E.S.S. INTEGRAL Kanata Kiso Kapteyn Liverpool Telescope Subaru Swift/NuSTAR VERITAS VLA/17B-403 teams Sarkar, S Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A |
| title | Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A |
| title_full | Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A |
| title_fullStr | Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A |
| title_full_unstemmed | Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A |
| title_short | Multimessenger observations of a flaring blazar coincident with high-energy neutrino IceCube-170922A |
| title_sort | multimessenger observations of a flaring blazar coincident with high energy neutrino icecube 170922a |
| work_keys_str_mv | AT icecubecollaboration multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT fermilat multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT magic multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT agile multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT asassn multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT hawc multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT hess multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT integral multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT kanata multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT kiso multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT kapteyn multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT liverpooltelescope multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT subaru multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT swiftnustar multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT veritas multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT vla17b403teams multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a AT sarkars multimessengerobservationsofaflaringblazarcoincidentwithhighenergyneutrinoicecube170922a |