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| name: Check the IVOA document | ||
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| doc_name: HighEnergyObsCoreExt | ||
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| DOCVERSION = 1.0 | ||
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| # Publication date, ISO format; update manually for "releases" | ||
| DOCDATE = 2026-04-27 | ||
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| # What is it you're writing: NOTE, WD, PR, REC, PEN, or EN | ||
| DOCTYPE = PEN | ||
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| # An e-mail address of the person doing the submission to the document | ||
| # repository (can be empty until a make upload is being made) | ||
| AUTHOR_EMAIL=ian.evans@ , bruno.khelifi@, mathieu.servillat@ | ||
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| # Source files for the TeX document (but the main file must always | ||
| # be called $(DOCNAME).tex) | ||
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| Vocabulary: http://www.ivoa.net/rdf/response-type | ||||||
| Author: Mireille Louys for HEIG IG <mireille.louys@unistra.fr> | ||||||
| Date: 2025-11-13 | ||||||
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| New Term: response-function | ||||||
| Action: Addition | ||||||
| Label: response-function | ||||||
| Description: | ||||||
| A data product type describing instrumental response functions for calibration and analysis. | ||||||
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| Relationships: response-function is a top level term. | ||||||
| Usually related to an event-list data product in high energy astrophysics. | ||||||
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| Used-in: Data sets made accessible via the Chandra CS2 catalog | ||||||
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| Rationale: | ||||||
| The distribution of event-list data in multi-messenger astronomy. | ||||||
| For example, Chandra primary products distributed via the Chandra | ||||||
| Data Archive include around half a dozen different types of products neces- | ||||||
| sary to analyse Chandra data (for example, L2 event-list, Aspect solution, | ||||||
| bad pixel map, spacecraft ephemeris, V&V Report). | ||||||
| For VHE gamma rays and neutrinos, the DL3 event-lists should manda- | ||||||
| torily be associated to their associated IRFs files. The links between the | ||||||
| event-list and these IRFs should be well defined in the event-bundle. | ||||||
| ---------- | ||||||
| New Term: Point Spread Function | ||||||
| Action: Addition | ||||||
| Label: psf | ||||||
| Description: A dataset that records the probability density function of | ||||||
| spatial/angular spreading of incident photons from a point source caused | ||||||
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| by the instrument (detector and/or mirror and/or analysis) | ||||||
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| Relationships: narrower than #response-function | ||||||
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There was a problem hiding this comment. Should this be narrower than #pdf ? |
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| Used-in: HESS test data release (https://doi.org/10.5281/zenodo.1421099) | ||||||
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| ---------- | ||||||
| New Term: Effective Area | ||||||
| Action: Addition | ||||||
| Label: aeff | ||||||
| Description: A dataset that records the “effective area” of a telescope | ||||||
| and/or instrument. The effective area is the geometric area | ||||||
| of the telescope and/or instrument reduced by efficiency factors | ||||||
| such as reflectivity and vignetting, cuts efficiency, among other effects | ||||||
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| Relationships: narrower than #response-function | ||||||
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| Used-in: HESS test data release (https://doi.org/10.5281/zenodo.1421099) | ||||||
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| ---------- | ||||||
| New Term: Ancillary Response File | ||||||
| Action: Addition | ||||||
| Label: arf | ||||||
| Description: A dataset that records the | ||||||
| combined telescope/instru- | ||||||
| ment effective area and | ||||||
| detector quantum efficiency as | ||||||
| a function of energy | ||||||
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There was a problem hiding this comment. Description: A dataset that records the combined telescope/instrument effective area and |
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| Relationships: narrower than #response-function | ||||||
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| Used-in: XMM data products ? | ||||||
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| ---------- | ||||||
| New Term: Background Rate | ||||||
| Action: Addition | ||||||
| Label: bkgrate | ||||||
| Description: A dataset that models the rate of residual events that are | ||||||
| not from the expected source type (e.g. for gamma-ray instrument it | ||||||
| measures residual non-gamma-ray events coming). | ||||||
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| Relationships: narrower than #response-function | ||||||
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| Used-in: HESS test data release (https://doi.org/10.5281/zenodo.1421099) | ||||||
| ---------- | ||||||
| New Term: Energy Dispersion | ||||||
| Action: Addition | ||||||
| Label: edisp | ||||||
| Description: A dataset that records the | ||||||
| probability density of detecting an event with an energy estimator given the true | ||||||
| energy of the event. | ||||||
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| Relationships: narrower than #response-function | ||||||
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| Used-in: HESS test data release (https://doi.org/10.5281/zenodo.1421099) | ||||||
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| New Term: Redistribution Matrix File | ||||||
| Action: Addition | ||||||
| Label: rmf | ||||||
| Description: A dataset that records the probability density function | ||||||
| mapping from energy space into detector pulse height (or position) space | ||||||
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There was a problem hiding this comment. Description: A dataset that records the probability density function mapping from energy space into detector pulse height (or position) space in a NASA OGIP Redistribution Matrix File compliant format. |
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| Relationships: narrower than #response-function | ||||||
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| Used-in: Chandra response data products ? | ||||||
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| Reference: | ||||||
| - IVOA Note: https://github.com/ivoa/HighEnergyObsCoreExt section 5.1.5 | ||||||
| - IVOA Note Virtual Observatory and High Energy Astrophysics Version 1.0 | ||||||
| https://ivoa.net/documents/Notes/VOHE/20241112/VOHE-Note-draft_1.0.pdf | ||||||
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| Vocabulary extension proposal for UCDs / | ||
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| Vocabulary: http://www.ivoa.net/rdf/datalink/core | ||
| Author: mireille.louys@astro.unistra.fr with EST solar group | ||
| Date: 2026-02-11 | ||
| Nb of terms discussed together : 1 | ||
| ----------------------- | ||
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| New Term: stat.confidenceLevel | ||
| Action: Amendement | ||
| Label: Level of confidence for *a statistical measure*, detection or classification process | ||
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| Description: statistical confidence level to assess a statistical distribution. | ||
| In the analysis of statistical products, the stat confidence levels is used to establish data quality. | ||
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| Rationale: Enhance definition of term to include statistical measures | ||
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| Used_in: Statistical data sets |
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