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102 changes: 102 additions & 0 deletions VEP-25_response-function.txt
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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

New Term: response-function
Action: Addition
Label: response-function
Description:
A data product type describing instrumental response functions for calibration and analysis.

Relationships: response-function is a top level term.
Usually related to an event-list data product in high energy astrophysics.

Used-in: Data sets made accessible via the Chandra CS2 catalog

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
by the instrument (detector and/or mirror and/or analysis)

Relationships: narrower than #response-function

Used-in: HESS test data release (https://doi.org/10.5281/zenodo.1421099)


----------
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

Relationships: narrower than #response-function

Used-in: HESS test data release (https://doi.org/10.5281/zenodo.1421099)

----------
Comment thread
bkhelifi marked this conversation as resolved.
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

Relationships: narrower than #response-function

Used-in: XMM data products ?

----------
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).

Relationships: narrower than #response-function

Comment thread
bkhelifi marked this conversation as resolved.
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.

Relationships: narrower than #response-function

Used-in: HESS test data release (https://doi.org/10.5281/zenodo.1421099)

----------
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

Relationships: narrower than #response-function

Used-in: Chandra response data products ?

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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