Information on Service '2007-2017 ANTARES search for cosmic neutrino point sources'

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The ANTARES neutrino telescope aims for the identification of neutrinos from cosmic accelerators. The good visibility towards the Southern sky for neutrino energies below 100 TeV and the good angular resolution for reconstructed events make the telescope excellent to test for the presence of point-like sources, especially of Galactic origin. The data set corresponds to the track sample (muon neutrino candidates) of a study meant to search for a point sources with data collected from January 2007 to December 2017 by the ANTARES neutrino telescope.

For a list of all services and tables belonging to this service's resource, see Information on resource '2007-2017 ANTARES search for cosmic neutrino point sources'

Overview

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This service is published as follows:

local means it is listed on our front page, ivo_managed means it has a record in the VO registry.

Input Fields

The following fields are available to provide input to the service (with some renderers, some of these fields may be unavailable):

NameTable Head DescriptionUnitUCD
DEC Delta (ICRS) Declination (ICRS decimal) deg pos.eq.dec
hscs_pos Position/Name Coordinates (as h m s, d m s or decimal degrees), or SIMBAD-resolvable object N/A N/A
hscs_sr Search radius Search radius in arcminutes N/A N/A
ID ID Event identifier, continuous event number in the data set N/A meta.id;meta.main
maxrec Match limit Maximum number of records returned. Pass 0 to retrieve service parameters. N/A N/A
RA Alpha (ICRS) Right Ascension (ICRS decimal) deg pos.eq.ra
responseformat Output Format File format requested for output. N/A meta.code.mime
SR Search Radius Search radius deg N/A
verb Verbosity Exhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns. N/A N/A

Default Output Fields

The following fields are contained in the output by default. More fields may be available for selection; these would be given below in the VOTable output fields.

NameTable Head DescriptionUnitUCD
_r Dist. Distance to cone center deg pos.distance
Beta Beta angular error estimate on reconstruction N/A stat.error;pos
Decl declination ICRS declination N/A pos.eq.dec;meta.main
ID ID Event identifier, continuous event number in the data set N/A meta.id;meta.main
MJD MJD Modified Julian Day N/A time.epoch
Nhit number of hits number of discrete integrated light signals in photomultipliers N/A phys.energy
RA right ascension ICRS right ascension N/A pos.eq.ra;meta.main

VOTable Output Fields

The following fields are available in VOTable output. The verbosity level is a number intended to represent the relative importance of the field on a scale of 1 to 30. The services take a VERB argument. A field is included in the output if their verbosity level is less or equal VERB*10.

NameTable Head DescriptionUnitUCD Verb. Level
_r Dist. Distance to cone center deg pos.distance 10
MJD MJD Modified Julian Day N/A time.epoch 20
Beta Beta angular error estimate on reconstruction N/A stat.error;pos 20
Nhit number of hits number of discrete integrated light signals in photomultipliers N/A phys.energy 20
RA right ascension ICRS right ascension N/A pos.eq.ra;meta.main 20
Decl declination ICRS declination N/A pos.eq.dec;meta.main 20
ID ID Event identifier, continuous event number in the data set N/A meta.id;meta.main 20

Citation Info

VOResource XML (that's something exclusively for VO nerds)