Policy, Copyrights, DOIs

Policy
In order for us to be able to report publications using IDOC to our funding agencies, please inform us and include the following text in the acknowledgements:

We recognize the use of IDOCs for the provision of data and services. IDOC support is provided by CNRS & CNES & Universite-Paris-Saclay.

If you wish to be more specific to your research theme, please use this type of acknowledgementa ccording to the thematic of the data or code used
MEDOC : This work used data provided by the MEDOC data and operations centre (CNES / CNRS / Universite-Paris-Saclay), MEDOC"
COSMO : We acknowledge the use of the COSMO archive for the Integrated Data & Operation Center (IDOC). Support for IDOC/COSMO is provided by CNRS & CNES & Universite-Paris-Saclay.
PSUP : We acknowledge the use of the PSUP archive for the Integrated Data & Operation Center (IDOC). Support for IDOC/PSUP is provided by CNRS & CNES & Universite-Paris-Saclay.
D2S : We acknowledge the use of the D2S archive for the Integrated Data & Operation Center (IDOC). Support for IDOC/D2S is provided by CNRS & CNES & Universite-Paris-Saclay.
AMIS : We acknowledge the use of the AMIS archive for the Integrated Data & Operation Center (IDOC). Support for IDOC/AMIS is provided by CNRS & CNES & Universite-Paris-Saclay.

Copyright & licensing
Data access is mainly open and free of charge.
The general license for the data, unless otherwise specified in the dataset-specific copyright  (according to french government recommandations https://www.data.gouv.fr/en/licences) is the following :
https://www.etalab.gouv.fr/wp-content/uploads/2018/11/open-licence.pdf
The general license for available software codes, unless otherwise specified in the specific download page is the following:
https://spdx.org/licenses/GPL-3.0-or-later.html#licenseText
Note : A small part of the hosted data may be subject to a temporary embargo or Moratorium = delay before open access to provide time for publication to scientist
 In the French law about “open science”, this delay is under a maximum of 6 month for science, technical and medical (STM) disciplines, after scientific qualification of data.
This moratorium depends mainly on the contracts proposed by the space agencies concerning the data from the missions they have financed.
- As far as NASA is concerned, the data are immediately open.
- ESA proposes a period of 6 months

DOIs
             The IDOC platform has decided on a nomenclature for the management of the DOIs assigned under its aegis:
The common prefix is 10.48326

10.48326/IDOC has been defined for IDOC as a platform (thus to identify for example the IDOC website)

then this first DOI is then broken down according to the thematic areas hosted by IDOC.

Here as an example, with regard to data sets or information from planetology:

10.48326/IDOC.PSUP

Then these elements are again declined again by data set (we will indicate these DOIs in the references of the interfaces).

example :

10.48326/IDOC.PSUP.OMEGA for OMEGA instrument data of the Mars-express probe.

Note: the level of declination used is not limited if this hierarchy created allows to finely account for the structure of the concerned interface, data or code :
As an example, the information on Oxia comes from two CTX and HIRISE instruments hosted on the MARSSI platform of the PSUP portal.
 This gives two DOIs to be used depending on the origin of the data used:
https://doi.org/10.48326/idoc.psup.marssi.ctx.oxia
and
https://doi.org/10.48326/idoc.psup.marssi.hirise.oxia
DOI's have been affixed on the different data sets to allow their referencing.
Please mention one of the DOIs listed below in your references if you use data from this repository in a scientific publication. Choose the DOI of the dataset used or a more generic DOI according to the datasets used and their degree of granularity.

             IDOC as a platform and root resource is referenced under the identifier : https://doi.org/10.48326/idoc
Others available DOIs
https://doi.org/10.48326/idoc
https://doi.org/10.48326/idoc.corot
https://doi.org/10.48326/idoc.corot.bright_stars_seismo_fields    
https://doi.org/10.48326/idoc.corot.confirmed_exoplanets           
https://doi.org/10.48326/idoc.corot.red_giants_Hekker_et_al        
https://doi.org/10.48326/idoc.corot.rotation_periods_Affer_et_al   
https://doi.org/10.48326/idoc.corot.rotation_periods_Medeiros_et_al
https://doi.org/10.48326/idoc.cosmo
https://doi.org/10.48326/idoc.cosmo.herschel
https://doi.org/10.48326/idoc.cosmo.herschel.cluster_Low-Z
https://doi.org/10.48326/idoc.cosmo.herschel.ddt_mustdo_4
https://doi.org/10.48326/idoc.cosmo.herschel.h-atlas
https://doi.org/10.48326/idoc.cosmo.herschel.lens_malhotra
https://doi.org/10.48326/idoc.cosmo.herschel.ot1_atielens
https://doi.org/10.48326/idoc.cosmo.herschel.ot1_mmiville
https://doi.org/10.48326/idoc.cosmo.herschel.ot1lho
https://doi.org/10.48326/idoc.cosmo.herschel.ot2_ehabart
https://doi.org/10.48326/idoc.cosmo.herschel.planck-high-z
https://doi.org/10.48326/idoc.cosmo.herschel.sag-1
https://doi.org/10.48326/idoc.cosmo.herschel.sag-3
https://doi.org/10.48326/idoc.cosmo.iris
https://doi.org/10.48326/idoc.cosmo.magyc
https://doi.org/10.48326/idoc.cosmo.szcluster
https://doi.org/10.48326/idoc.medoc
https://doi.org/10.48326/idoc.medoc.coronas-f
https://doi.org/10.48326/idoc.medoc.coronas-f.spirit
https://doi.org/10.48326/idoc.medoc.coronas-f.spirit.hr2-175a
https://doi.org/10.48326/idoc.medoc.coronas-f.spirit.hr2-304a
https://doi.org/10.48326/idoc.medoc.eit-syn
https://doi.org/10.48326/idoc.medoc.monsoon
https://doi.org/10.48326/idoc.medoc.picard
https://doi.org/10.48326/idoc.medoc.picard.premos
https://doi.org/10.48326/idoc.medoc.picard.sodism
https://doi.org/10.48326/idoc.medoc.picard.sodism2
https://doi.org/10.48326/idoc.medoc.sdo
https://doi.org/10.48326/idoc.medoc.sdo.aia
https://doi.org/10.48326/idoc.medoc.sdo.aia-syn
https://doi.org/10.48326/idoc.medoc.sdo.gaia-dem
https://doi.org/10.48326/idoc.medoc.sdo.hmi
https://doi.org/10.48326/idoc.medoc.sdo.hmi-currents
https://doi.org/10.48326/idoc.medoc.soho
https://doi.org/10.48326/idoc.medoc.solar_movies
https://doi.org/10.48326/idoc.medoc.stereo
https://doi.org/10.48326/idoc.medoc.stereo.secchi
https://doi.org/10.48326/idoc.medoc.stereo.secchi.cor1
https://doi.org/10.48326/idoc.medoc.stereo.secchi.cor2
https://doi.org/10.48326/idoc.medoc.stereo.secchi.euvi
https://doi.org/10.48326/idoc.medoc.stereo.secchi.hi1
https://doi.org/10.48326/idoc.medoc.stereo.secchi.hi2
https://doi.org/10.48326/idoc.medoc.trace
https://doi.org/10.48326/idoc.psup
https://doi.org/10.48326/idoc.psup.jovial
https://doi.org/10.48326/idoc.psup.jovial.n2a
https://doi.org/10.48326/idoc.psup.jovial.n2b
https://doi.org/10.48326/idoc.psup.marssi
https://doi.org/10.48326/idoc.psup.marssi.ctx.oxia
https://doi.org/10.48326/idoc.psup.marssi.hirise.oxia
https://doi.org/10.48326/idoc.psup.omega
https://doi.org/10.48326/idoc.psup.omega.C_channel_After_Filtering
https://doi.org/10.48326/idoc.psup.omega.Catalogs
https://doi.org/10.48326/idoc.psup.omega.data_cubes
https://doi.org/10.48326/idoc.psup.omega.mineral_maps
DOIs for software codes
https://doi.org/10.48326/idoc.medoc.radtransfer.prom4
https://doi.org/10.48326/idoc.medoc.radtransfer.prom5
https://doi.org/10.48326/idoc.medoc.radtransfer.prom7
https://doi.org/10.48326/idoc.medoc.radtransfer.prodop
https://doi.org/10.48326/idoc.medoc.radtransfer.promcor
https://doi.org/10.48326/idoc.medoc.radtransfer.hydr_nv
 
 
https://doi.org/10.48326/idoc.medoc.radtransfer.2d-crd-mali-gs     ...  
https://doi.org/10.48326/idoc.medoc.radtransfer.1d-crd-ali-semiinf   
https://doi.org/10.48326/idoc.medoc.radtransfer.1d-crd-ali-filament  
https://doi.org/10.48326/idoc.medoc.radtransfer.1d-crd-ali-prominence
 
https://doi.org/10.48326/idoc.medoc.cst