scholarly journals Ultrahigh-energy neutrino follow-up of gravitational wave events GW150914 and GW151226 with the Pierre Auger Observatory

2016 ◽  
Vol 94 (12) ◽  
Author(s):  
A. Aab ◽  
P. Abreu ◽  
M. Aglietta ◽  
I. Al Samarai ◽  
I. F. M. Albuquerque ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Pierre Auger Observatory ◽  
Ultrahigh Energy ◽  
Energy Neutrino

scholarly journals Search for UHE neutrinos in coincidence with LIGO GW150914 event with the Pierre Auger Observatory

2016 ◽  
Vol 12 (S324) ◽  
pp. 295-298
Author(s):  
Lili Yang ◽  
Keyword(s):  
Energy Range ◽  
Gravitational Wave ◽  
High Energy ◽  
Universal Time ◽  
Pierre Auger Observatory ◽  
Ultra High Energy ◽  
Upper Limit ◽  
Surface Detector ◽  
High Energy Regime

AbstractThe first gravitational wave transient GW150914 was observed by Advanced LIGO on September 14th, 2015 at 09:50:45 Universal Time. In addition to follow-up electromagnetic observations, the detection of neutrinos will probe deeply and more on the nature of astrophysical sources, especially in the ultra-high energy regime. Neutrinos in the EeV energy range were searched in data collected at the surface detector of the Pierre Auger Observatory within ± 500 s and 1 day after the GW150914 event. No neutrino candidates were found. Based on this non-observation, we derive the first and only neutrino fluence upper limit at EeV energies for this event at 90% CL, and report constraints on existence of accretion disk around mergers.

scholarly journals Swift Follow-up Observations of Gravitational-wave and High-energy Neutrino Coincident Signals

2021 ◽  
Vol 909 (2) ◽  
pp. 126
Author(s):  
Azadeh Keivani ◽  
Jamie A. Kennea ◽  
Phil A. Evans ◽  
Aaron Tohuvavohu ◽  
Riki Rapisura ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino

scholarly journals High-energy neutrino follow-up search of gravitational wave event GW150914 with ANTARES and IceCube

2016 ◽  
Vol 93 (12) ◽  
Author(s):  
S. Adrián-Martínez ◽  
A. Albert ◽  
M. André ◽  
M. Anghinolfi ◽  
G. Anton ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino ◽  
Wave Event

scholarly journals Follow-up Search for UHE Photons from Gravitational Wave Sources with the Pierre Auger Observatory

2021 ◽  
Author(s):  
Philip Ruehl ◽  
Pedro Abreu ◽  
Marco Aglietta ◽  
Justin M. Albury ◽  
Ingomar Allekotte ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Pierre Auger Observatory

scholarly journals High-Energy Neutrino follow-up of first gravitational wave event GW150914

2017 ◽  
Vol 888 ◽  
pp. 012045
Author(s):  
Alexis Coleiro ◽  
Bruny Baret ◽  
Thierry Pradier ◽  
Keyword(s):  
Gravitational Wave ◽  
High Energy ◽  
High Energy Neutrino ◽  
Energy Neutrino ◽  
Wave Event

scholarly journals The H.E.S.S. gravitational wave rapid follow-up program

2021 ◽  
Vol 2021 (03) ◽  
pp. 045
Author(s):  
Halim Ashkar ◽  
Francois Brun ◽  
Matthias Füßling ◽  
Clemens Hoischen ◽  
Stefan Ohm ◽  
...  
Keyword(s):  
Gravitational Wave

scholarly journals Processing GOTO data with the Rubin Observatory LSST Science Pipelines I: Production of coadded frames

2021 ◽  
Vol 38 ◽  
Author(s):  
J. R. Mullaney ◽  
L. Makrygianni ◽  
V. Dhillon ◽  
S. Littlefair ◽  
K. Ackley ◽  
...  
Keyword(s):  
Gravitational Wave ◽  
Time Domain ◽  
Wide Area ◽  
Wide Field ◽  
Process Data ◽  
Data Production ◽  
The Time Domain ◽  
Further Development ◽  
High Cadence

Abstract The past few decades have seen the burgeoning of wide-field, high-cadence surveys, the most formidable of which will be the Legacy Survey of Space and Time (LSST) to be conducted by the Vera C. Rubin Observatory. So new is the field of systematic time-domain survey astronomy; however, that major scientific insights will continue to be obtained using smaller, more flexible systems than the LSST. One such example is the Gravitational-wave Optical Transient Observer (GOTO) whose primary science objective is the optical follow-up of gravitational wave events. The amount and rate of data production by GOTO and other wide-area, high-cadence surveys presents a significant challenge to data processing pipelines which need to operate in near-real time to fully exploit the time domain. In this study, we adapt the Rubin Observatory LSST Science Pipelines to process GOTO data, thereby exploring the feasibility of using this ‘off-the-shelf’ pipeline to process data from other wide-area, high-cadence surveys. In this paper, we describe how we use the LSST Science Pipelines to process raw GOTO frames to ultimately produce calibrated coadded images and photometric source catalogues. After comparing the measured astrometry and photometry to those of matched sources from PanSTARRS DR1, we find that measured source positions are typically accurate to subpixel levels, and that measured L-band photometries are accurate to $\sim50$ mmag at $m_L\sim16$ and $\sim200$ mmag at $m_L\sim18$ . These values compare favourably to those obtained using GOTO’s primary, in-house pipeline, gotophoto, in spite of both pipelines having undergone further development and improvement beyond the implementations used in this study. Finally, we release a generic ‘obs package’ that others can build upon, should they wish to use the LSST Science Pipelines to process data from other facilities.

scholarly journals ULTRAHIGH ENERGY NEUTRINOS

2003 ◽  
Vol 18 (22) ◽  
pp. 4085-4096 ◽  
Author(s):  
SHARADA IYER DUTTA ◽  
MARY HALL RENO ◽  
INA SARCEVIC
Keyword(s):  
Black Hole ◽  
Standard Model ◽  
Cross Section ◽  
Neutrino Oscillations ◽  
Ultrahigh Energy ◽  
Nonstandard Model ◽  
Air Shower ◽  
Energy Neutrino ◽  
The Standard Model ◽  
Event Rates

The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino energies up to 1012 GeV, Tests of neutrino oscillations (νμ ↔ ντ) from extragalactic sources of neutrinos are possible with large underground detectors. Measurements of horizontal air shower event rates at neutrino energies above 1010 GeV will be able to constrain nonstandard model contributions to the neutrino-nucleon cross section, e.g., from mini-black hole production.

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