From 6778d4542cbbaad884217a7ffada39cf386678c7 Mon Sep 17 00:00:00 2001 From: Steffen Hallmann Date: Tue, 16 Jun 2026 15:10:27 +0200 Subject: [PATCH 1/3] adjust use cases for neutrinos --- UseCases.tex | 43 +++++++++++++++++++++++++------------------ 1 file changed, 25 insertions(+), 18 deletions(-) diff --git a/UseCases.tex b/UseCases.tex index a568fe1..cccffa2 100644 --- a/UseCases.tex +++ b/UseCases.tex @@ -290,14 +290,14 @@ \subsubsection{Use Case --- Get all the \glspl{IRF} for a given CTAO observation AND (obs_collection = 'CTAO-DR1') \end{verbatim} -\subsubsection{Use Case --- Search for all ANTARES neutrino events for a given dataset in the direction of a point source} +\subsubsection{Use Case --- Search for all ANTARES data products for a given collection in the direction of a point source} {\em Using the ANTARES 2007--2017 point source data set, retrieve all events, background estimate, and detector acceptance to calculate the expected neutrino flux from a given point source, e.g. HESSJ0632+057, as in \textit{G. Illuminati for the ANTARES Collaboration, PoS(ICRC2019)920} and recalculate the significance of the neutrino flux.} \medskip \noindent Find all datasets satisfying \begin{enumerate}[(i)] - \item Position inside 5 degrees from (98.24, 5.81), + \item Source (98.24, 5.81) within detector field of view, \item dataproduct\_type = ``event-bundle'' or ``event-list'' or ``response-function'', \item obs\_collection = ``ANTARES-2017-PS''. \end{enumerate} @@ -306,7 +306,7 @@ \subsubsection{Use Case --- Search for all ANTARES neutrino events for a given d SELECT * FROM ivoa.obscore NATURAL JOIN ivoa.obscore_hea WHERE -(CONTAINS(POINT(s_ra, s_dec), CIRCLE(98.24, 5.81, 5.0)) = 1) +(CONTAINS(POINT('ICRS', 98.24, 5.81), CIRCLE('ICRS', s_ra, s_dec, s_fov)) = 1) AND (dataproduct_type IN ('event-bundle', 'event-list', 'response-function')) AND (obs_collection = 'ANTARES-2017-PS') \end{verbatim} @@ -318,23 +318,25 @@ \subsubsection{Use Case --- Retrieve the instrument response functions for a com \medskip \noindent Find all IRF datasets satisfying: \begin{enumerate}[(i)] - \item Position inside 5 degrees from (0.8, -45.19), + \item Source (0.8, -45.19) within detector field of view \item dataproduct\_type = ``response-function'', - \item instrument\_name = ``KM3NeT-ARCA'', + \item instrument\_name LIKE ``\%ARCA\%'', \item t\_min/t\_max from 2027--2030, ({\em i.e.\/}, MJD 61406--62870), - \item event\_type = ``track''. + \item event\_type = ``track'', + \item analysis mode optimised for pointsource searches. \end{enumerate} \begin{verbatim} SELECT * FROM ivoa.obscore NATURAL JOIN ivoa.obscore_hea WHERE -(CONTAINS(POINT(s_ra, s_dec), CIRCLE(0.8, -45.19, 5.0)) = 1) +(CONTAINS(POINT('ICRS', 0.8, -45.19), CIRCLE('ICRS', s_ra, s_dec, s_fov)) = 1) AND (dataproduct_type = 'response-function')) -AND (instrument_name = '%ARCA%') -AND (t_min >= 61406) -AND (t_max <= 62870) +AND (instrument_name LIKE '%ARCA%') +AND (t_max >= 61406) +AND (t_min <= 62870) AND (event_type = 'track') +AND (analysis_mode = 'pointsource') \end{verbatim} \subsubsection{Use Case --- Study the combined neutrino flux for the Galactic plane} @@ -344,9 +346,10 @@ \subsubsection{Use Case --- Study the combined neutrino flux for the Galactic pl \medskip \noindent Find all neutrino datasets satisfying: \begin{enumerate}[(i)] - \item messenger = ``neutrino'', \item dataproduct\_type = ``event-bundle'', - \item analysis\_mode = ``diffuse''. + \item messenger = ``neutrino'', + \item analysis\_mode = ``diffuse'', + \item Galactic plane box within the detector field of view. \end{enumerate} % diffuse @@ -355,20 +358,23 @@ \subsubsection{Use Case --- Study the combined neutrino flux for the Galactic pl NATURAL JOIN ivoa.obscore_hea WHERE (dataproduct_type = 'event-bundle') -AND (messenger = '%neutrino%') +AND (messenger = 'neutrino') AND (analysis_mode = 'diffuse') +AND 1 = INTERSECTS( + CIRCLE('ICRS', s_ra, s_dec, 80), + BOX('GALACTIC', 0, 0, 30, 2)) \end{verbatim} \subsubsection{Use Case --- Calculate the probability for a source class to be emitters of tau neutrinos} -{\em Using a catalog of potential sources, calculate the probability of measuring a $\nu_{\tau}$ neutrino flux from a stacking of all sources of that type with 10 years of data taking with widely spaced, high energy detectors like ARCA.} +{\em Using a catalog of potential sources, calculate the probability of measuring a $\nu_{\tau}$ neutrino flux from a stacking of all sources of that type with 10 years of data taking with widely spaced, high energy optical detectors like ARCA.} \medskip \noindent Find all neutrino datasets satisfying: \begin{enumerate}[(i)] - \item dataproduct\_type = ``response-function'', + \item dataproduct\_type = ``response-function'', dataproduct\_subtype = ``aeff`` \item messenger contains ``pdgid-16'' or ``pdgid+16'', - \item obs\_mode = ``wide-array'', + \item obs\_mode = ``optical'', \item analysis\_mode = ``pointsource''. \end{enumerate} @@ -377,8 +383,9 @@ \subsubsection{Use Case --- Calculate the probability for a source class to be e NATURAL JOIN ivoa.obscore_hea WHERE (dataproduct_type = 'response-function') -AND (messenger = '%pdgid-16%' OR messenger = '%pdgid+16%') -AND (obs_mode LIKE '%wide-array%') +AND (dataproduct_subtype = 'aeff') +AND (messenger = 'pdgid-16' OR messenger = 'pdgid+16') +AND (obs_mode LIKE '%optical%') AND (analysis_mode LIKE '%pointsource%') \end{verbatim} From 1d0b3f60249679f5c082532af381cf17756e0ad3 Mon Sep 17 00:00:00 2001 From: Steffen Hallmann Date: Wed, 24 Jun 2026 09:58:55 +0200 Subject: [PATCH 2/3] incorporating Bruno K suggestions --- UseCases.tex | 3 ++- 1 file changed, 2 insertions(+), 1 deletion(-) diff --git a/UseCases.tex b/UseCases.tex index be0b4ee..081c38a 100644 --- a/UseCases.tex +++ b/UseCases.tex @@ -302,7 +302,7 @@ \subsubsection{Use Case --- Retrieve the instrument response functions for a com \begin{enumerate}[(i)] \item Source (0.8, -45.19) within detector field of view \item dataproduct\_type = ``response-function'', - \item instrument\_name LIKE ``\%ARCA\%'', + \item dataproducts from the ``ARCA'' instrument of the ``KM3NeT'' facility, \item t\_min/t\_max from 2027--2030, ({\em i.e.\/}, MJD 61406--62870), \item event\_type = ``track'', \item analysis mode optimised for pointsource searches. @@ -314,6 +314,7 @@ \subsubsection{Use Case --- Retrieve the instrument response functions for a com WHERE (CONTAINS(POINT('ICRS', 0.8, -45.19), CIRCLE('ICRS', s_ra, s_dec, s_fov)) = 1) AND (dataproduct_type = 'response-function')) +AND (facility_name = 'KM3NeT') AND (instrument_name LIKE '%ARCA%') AND (t_max >= 61406) AND (t_min <= 62870) From 8979a52273606685ce9dd350133e3ecc998ebfea Mon Sep 17 00:00:00 2001 From: Steffen Hallmann Date: Wed, 24 Jun 2026 10:04:26 +0200 Subject: [PATCH 3/3] Update ANTARES data product descriptions --- UseCases.tex | 8 ++++---- 1 file changed, 4 insertions(+), 4 deletions(-) diff --git a/UseCases.tex b/UseCases.tex index 081c38a..d62db61 100644 --- a/UseCases.tex +++ b/UseCases.tex @@ -272,7 +272,7 @@ \subsubsection{Use Case --- Get all the \glspl{IRF} for a given CTAO observation AND (obs_collection = 'CTAO-DR1') \end{verbatim} -\subsubsection{Use Case --- Search for all ANTARES data products for a given collection in the direction of a point source} +\subsubsection{Use Case --- Search for all ANTARES neutrino data products for a given collection in the direction of a point source} {\em Using the ANTARES 2007--2017 point source data set, retrieve all events, background estimate, and detector acceptance to calculate the expected neutrino flux from a given point source, e.g. HESSJ0632+057, as in \textit{G. Illuminati for the ANTARES Collaboration, PoS(ICRC2019)920} and recalculate the significance of the neutrino flux.} @@ -352,14 +352,14 @@ \subsubsection{Use Case --- Study the combined neutrino flux for the Galactic pl \subsubsection{Use Case --- Calculate the probability for a source class to be emitters of tau neutrinos} -{\em Using a catalog of potential sources, calculate the probability of measuring a $\nu_{\tau}$ neutrino flux from a stacking of all sources of that type with 10 years of data taking with widely spaced, high energy optical detectors like ARCA.} +{\em Using a catalog of potential sources, calculate the probability of measuring a $\nu_{\tau}$ neutrino flux from a stacking of all sources of that type with 10 years of data taking with widely spaced, high energy optical detectors like KM3NeT/ARCA.} \medskip \noindent Find all neutrino datasets satisfying: \begin{enumerate}[(i)] \item dataproduct\_type = ``response-function'', dataproduct\_subtype = ``aeff`` \item messenger contains ``pdgid-16'' or ``pdgid+16'', - \item obs\_mode = ``optical'', + \item obs\_mode = ``wide-array'', \item analysis\_mode = ``pointsource''. \end{enumerate} @@ -370,7 +370,7 @@ \subsubsection{Use Case --- Calculate the probability for a source class to be e (dataproduct_type = 'response-function') AND (dataproduct_subtype = 'aeff') AND (messenger = 'pdgid-16' OR messenger = 'pdgid+16') -AND (obs_mode LIKE '%optical%') +AND (obs_mode LIKE '%wide-array%') AND (analysis_mode LIKE '%pointsource%') \end{verbatim}