Recent Results from the ANTARES Neutrino Telescope 2013

S. Mangano (on behalf of the ANTARES Collaboration)

RECORD

Recent Results from the ANTARES Neutrino Telescope 2013

S. Mangano (on behalf of the ANTARES Collaboration)

High Energy Astrophysical Phenomena · Submitted 20 May 2013

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim For example we will show the latest results from searches for neutrinos from steady cosmic point-like sources, for neutrinos from Fermi Bubbles, for neutrinos from Dark Matter in the Sun and the measurement of atmospheric neutrino oscillation parameters.

how it is stated · asserted 0.95 read the record →

Comment (0) Read on arXiv ↗

Cite ▾

Claim paper

The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,618 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.07 · human participants 0.02 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.09 · compares with prior results 0.09 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; show every role.

The ANTARES experiment is currently the largest underwater neutrino telescope. It is taking high quality data since 2007 and aims to detect high energy neutrinos that are expected from the acceleration of cosmic rays from astrophysical sources. We will review the status of the detector and present several analyses carried out on atmospheric muons and neutrinos. For example we will show the latest results from searches for neutrinos from steady cosmic point-like sources, for neutrinos from Fermi Bubbles, for neutrinos from Dark Matter in the Sun and the measurement of atmospheric neutrino oscillation parameters.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	The ANTARES experiment is currently the largest underwater neutrino telescope.	background 0.96	0.15	0.04	asserted 1.00
s1	It is taking high quality data since 2007 and aims to detect high energy neutrinos that are expected from the acceleration of cosmic rays from astrophysical sources.	background 0.91	0.58	0.04	asserted 0.99
s2	We will review the status of the detector and present several analyses carried out on atmospheric muons and neutrinos.	contribution 0.94	0.58	0.04	asserted 0.91
s3	For example we will show the latest results from searches for neutrinos from steady cosmic point-like sources, for neutrinos from Fermi Bubbles, for neutrinos from Dark Matter in the Sun and the measurement of atmospheric neutrino oscillation parameters.	contribution 0.96	0.88	0.08	asserted 0.95

What kind of paper the classifier reports this is: empirical study 0.70 · evidence from analysis of existing data 0.54.

What was examined, and what was not

sources read

arXiv listing abstract v1

not examined

full text
figures and tables
references and citing sentences
relations to other papers

levels run

P abstract

not run

S sections
T body sentences
C citations
R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper

Original abstract

The ANTARES experiment is currently the largest underwater neutrino telescope. It is taking high quality data since 2007 and aims to detect high energy neutrinos that are expected from the acceleration of cosmic rays from astrophysical sources. We will review the status of the detector and present several analyses carried out on atmospheric muons and neutrinos. For example we will show the latest results from searches for neutrinos from steady cosmic point-like sources, for neutrinos from Fermi Bubbles, for neutrinos from Dark Matter in the Sun and the measurement of atmospheric neutrino oscillation parameters.

Human review

How Pith checks papers → · Full audit of this paper →

References

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Reconstruction of Interstellar Cosmic Ray Anisotropy via Heliospheric Propagation Modeling and SVD Inversion
astro-ph.HE 2026-10 conditional novelty 5.0 of 10

A heliospheric transport simulation plus SVD inversion recovers the interstellar cosmic-ray dipole once a circle-fitting algorithm restores the detector-blind North-South component, with Poisson count noise dominating...
Probing the Galactic Origin of the IceCube Excess with Gamma-Rays
astro-ph.HE 2013-09 conditional novelty 5.0 of 10

Existing TeV to PeV diffuse gamma-ray limits disfavor an isotropic Galactic origin for the IceCube neutrino excess, supporting a mostly extragalactic interpretation, though the relevant Southern Sky is poorly covered.

How the literature uses it

1 arXiv paper cite this in 1 sentence

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

What it cites · 4 sentences without a confident label

Compares with 2 papers

For comparison the limits from the other experiments such as IceCube [ref] and Super-Kamiokande [ref] are also shown.

Search for dark matter annihilations in the Sun with the 79-string IceCube detector · Dark Matter · 0.99
Figure [ref] right shows the upper limits and compares it to expected signal for optimistic models [ref] .

The Fermi Bubbles: Giant, Multi-Billion-Year-Old Reservoirs of Galactic Center Cosmic Rays · Fermi Bubbles · 0.91

Cites as background 1 paper

In this proceeding there was not enough room to discuss other topics which were illustrated at the Rencontres de Moriond, such as the atmospheric muon [ref] and neutrino fluxes [ref] , the time system [ref] , the acoustic neutrino detection system [ref] , the search for relativistic magnetic monopoles [ref] , the searches for nuclearites [ref] and the correlation of neutrinos with gravitational waves [ref] , for which the reader is referred to elsewhere.

A First Search for coincident Gravitational Waves and High Energy Neutrinos using LIGO, Virgo and ANTARES data from 2007 · Conclusion · 0.99

Discussion

Know something about this paper? Leave a comment, or highlight any passage above to comment on it.