2013A&A...559A...9A -
Astronomy and Astrophysics, volume 559A, 9-9 (2013/11-1)
Search for muon neutrinos from gamma-ray bursts with the ANTARES neutrino telescope using 2008 to 2011 data.
ADRIAN-MARTINEZ S., ALBERT A., AL SAMARAI I., ANDRE M., ANGHINOLFI M., ANTON G., ANVAR S., ARDID M., ASTRAATMADJA T., AUBERT J.-J., BARET B., BARRIOS-MARTI J., BASA S., BERTIN V., BIAGI S., BIGONGIARI C., BOGAZZI C., BOUHOU B., BOUWHUIS M.C., BRUNNER J., BUSTO J., CAPONE A., CARAMETE L., CARLOGANU C., CARR J., CECCHINI S., CHARIF Z., CHARVIS P., CHIARUSI T., CIRCELLA M., CLASSEN F., CONIGLIONE R., CORE L., COSTANTINI H., COYLE P., CREUSOT A., CURTIL C., DE BONIS G., DEKEYSER I., DESCHAMPS A., DISTEFANO C., DONZAUD C., DORNIC D., DOROSTI Q., DROUHIN D., DUMAS A., EBERL T., EMANUELE U., ENZENHOEFER A., ERNENWEIN J.-P., ESCOFFIER S., FEHN K., FERMANI P., FLAMINIO V., FOLGER F., FRITSCH U., FUSCO L.A., GALATA S., GAY P., GEISSELSOEDER S., GEYER K., GIACOMELLI G., GIORDANO V., GLEIXNER A., GOMEZ-GONZALEZ J.P., GRAF K., GUILLARD G., VAN HAREN H., HEIJBOER A.J., HELLO Y., HERNANDEZ-REY J.J., HEROLD B., HOESSL J., JAMES C.W., DE JONG M., KADLER M., KALEKIN O., KAPPES A., KATZ U., KOOIJMAN P., KOUCHNER A., KREYKENBOHM I., KULIKOVSKIY V., LAHMANN R., LAMBARD E., LAMBARD G., LAROSA G., LEFEVRE D., LEONORA E., LO PRESTI D., LOEHNER H., LOUCATOS S., LOUIS F., MANGANO S., MARCELIN M., MARGIOTTA A., MARTINEZ-MORA J.A., MARTINI S., MICHAEL T., MONTARULI T., MORGANTI M., MUELLER C., NEFF M., NEZRI E., PALIOSELITIS D., PAVALAS G.E., PERRINA C., PIATTELLI P., POPA V., PRADIER T., RACCA C., RICCOBENE G., RICHTER R., RIVIERE C., ROBERT A., ROENSCH K., ROSTOVTSEV A., SAMTLEBEN D.F.E., SANGUINETI M., SCHMID J., SCHNABEL J., SCHULTE S., SCHUESSLER F., SEITZ T., SHANIDZE R., SIEGER C., SIMEONE F., SPIES A., SPURIO M., STEIJGER J.J.M., STOLARCZYK T., SANCHEZ-LOSA A., TAIUTI M., TAMBURINI C., TAYALATI Y., TROVATO A., VALLAGE B., VALLEE C., VAN ELEWYCK V., VERNIN P., VISSER E., WAGNER S., WILMS J., DE WOLF E., YATKIN K., YEPES H., ZORNOZA J.D., ZUNIGA J. and BAERWALD P.
Abstract (from CDS):
We search for muon neutrinos in coincidence with GRBs with the ANTARES neutrino detector using data from the end of 2007 to 2011. Expected neutrino fluxes were calculated for each burst individually. The most recent numerical calculations of the spectra using the NeuCosmA code were employed, which include Monte Carlo simulations of the full underlying photohadronic interaction processes. The discovery probability for a selection of 296 GRBs in the given period was optimised using an extended maximum-likelihood strategy. No significant excess over background is found in the data, and 90% confidence level upper limits are placed on the total expected flux according to the model.
Abstract Copyright:
∼
Journal keyword(s):
neutrinos - gamma-ray burst: general - methods: numerical
VizieR on-line data:
<Available at CDS (J/A+A/559/A9): table3.dat>
Status at CDS
:
All or part of tables of objects could be ingested in SIMBAD with priority 2.
(Ref) Object type as listed in the reference "Ref"
(acronym) Object type linked to the acronym according to the original reference
() Anterior to 2007, before we can link the objet type to a reference, or given by the CDS team in some particular cases
Other object types:
gB
(GRB)
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
ra dec : right ascension and declination (unit and frame defined according to your Output Options)
Grey values are increasing the original precision due to the computation of frame transformations
(wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
[error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
position angle (in degrees North celestial pole to East)
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
ra dec : right ascension and declination (unit and frame defined according to your Output Options)
Grey values are increasing the original precision due to the computation of frame transformations
(wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
[error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
position angle (in degrees North celestial pole to East)
quality : flag of quality
E ≥ 10"
D : 1-10" (and some old data)
C : 0.1-1"
B : 0.01-0.1" + 2MASS, Tyc
A : VLBI, Hipparcos
bibcode : bibcode of the coordinates reference
FK4
coord.
(ep=B1950 eq=1950) :
02 07 53.99 -27 20 27.3
[
]
Syntax of coordinates is : "ra dec (wtype) [error ellipse] quality bibcode" :
ra dec : right ascension and declination (unit and frame defined according to your Output Options)
Grey values are increasing the original precision due to the computation of frame transformations
(wtype) : wavelength class for the origin of the coordinates (Rad, mm, IR, Optical, UV, Xray, Gam)
[error ellipse] : measurement uncertainty, on (ra,dec) if the positional angle is 90 degrees, on (majaxis,minaxis) otherwise (in mas at defined epoch in the original catalogue),
position angle (in degrees North celestial pole to East)
quality : flag of quality
E ≥ 10"
D : 1-10" (and some old data)
C : 0.1-1"
B : 0.01-0.1" + 2MASS, Tyc
A : VLBI, Hipparcos
bibcode : bibcode of the coordinates reference
Gal
coord.
(ep=J2000) :
217.37833 -72.50160
[
]
Syntax of radial velocity (or/and redshift) is : "value [error] (wavelength) quality bibcode"
value : radial velocity or/and redshift (Heliocentric frame) according to your Output Options
(redshift may be not displayed if the data value is <0 and the database inside value is a radial velocity)
[error] : error of the corresponding value displayed before
(wavelength) : wavelength range of the measurement : Rad, mm, IR, Opt, UV, Xray, Gam or '∼'(unknown)
quality : flag of quality ( A=best quality -> E=worst quality, {� } =unknown quality)
References (71 between 1850 and 2023) (Total 71)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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