Lab spectroscopy extension |
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Iterated from SSHADE and other proposals in Rome |
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Initial proposal from PDS_speclib implementation |
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Existing parameters in italics |
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No longer consistent with workshop outcomes |
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New from workshop |
group related to: |
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target_class |
sample reference |
'sample', constant |
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'sample', constant |
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target_name |
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Provides name of a meteorite, lunar sample, IDP, micrometeorite, etc from which the sample is extracted |
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provides an ID of the sample |
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- empty otherwise, no local ID |
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Introduces the name of a meteorite or lunar sample when applicable. |
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alt_target_name |
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has to be related to target_name only - can't be used to store extra info on sample identification |
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sample_id |
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will provide name/ID of measured sample in local collection |
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Various parts of the same sample can be indicated and described in sample_desc (such as "Location A", etc) |
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producer_name |
measurement origin |
These two provide enough credits in the table (agreed) |
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provide reference to whom measured the sample |
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producer_institute |
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instrument_host_name |
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Standard name of the lab/facility |
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Standard name of the lab/facility |
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instrument_name |
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Name of instrument (as in publications) |
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Name of instrument (as in publications) |
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sample_classification |
sample description |
provides composition as group, class, sub-class, etc… of sample, concatenated in a hash-list (=> flexible searches with LIKE and %) |
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Name of mineral to be included |
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Should include specification "meteorite" plus the meteorite type when applicable, as well as description of (main) mixtures ingredients |
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Meteorite types as in Krot et al 2005. Dana or Struntz classification tags can be used for minerals. |
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Minor/trace components are not welcome here (would multiply false alarms) |
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grain_size_min |
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Min/max defined somehow, left to data provider |
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provide the particle size range in µm |
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grain_size_max |
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(not expected to be intensively used) - code for bulk ? |
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A very large value (eg, >1000 µm) can be used locally in a service to identify bulk material |
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- see if we define a code for this (-1 could do, but we also have to reserve a code for N/A |
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? Sample_origin ? |
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Need to have a separated Origin parameter ? Eg: Natural/synthetic, etc, including "mixture"? |
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Azimuth angle in degrees - see if negative values of angles can have a special meaning |
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azimuth_min |
environment parameters |
complement incidence, emergence, and phase |
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azimuth_max |
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negative values for azi and phase have a special meaning? |
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pressure |
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unit TBC (bar in PDS speclib) |
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experimental conditions, in bar and K |
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temperature |
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K |
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measurement_atmosphere |
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description of experimental conditions, free string. Measurements under vacuum are indicated here with the word "vacuum". |
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measurement_type |
relative to setup |
Contains UCD for this type of spectrum |
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The type of measurement/scale (REFF, I_over_F, etc…) provided as a UCD |
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Being discussed in IVOA |
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geometry_type |
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? |
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such as bidirectional, biconical, directional-hemispherical, etc - see if this list can be frozen (not likely) |
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spectrum_type |
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proposed to store measurement_type in clear, associated to a specific UCD (proposal to be forwarded to IVOA) |
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(may need to remove duplicates from Bernard's list) |
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sample_desc |
descriptions |
free string or hash-list describing the sample, its origin, and possible preparation |
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free string or hash-list describing the sample, its origin, and possible preparation |
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setup_desc |
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free string or hash-list describing the experimental setup if needed - may include Aperture (size of sample measured), etc |
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free string or hash-list describing the experimental setup if needed - may include Aperture (size of sample measured), etc |
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data_calibration_desc |
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free string or hash-list describing data post-processing / calibration |
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free string or hash-list describing data post-processing / calibration |
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thumbnail_url |
std parameters |
provides a link to a small spectral plot for quicklook only in VESPA portal |
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provides a link to a small spectral plot - caution should be taken to have units / values readable in full size (will be reduced in VESPA portal) |
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with special use |
(larger plots to be provided as separated granules with dataproduct_type = im) |
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datalink_url |
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Can contain a series of links to descriptive files providing extra information (image, text…) |
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Best solution to link descriptive files providing extra information |
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Species |
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Use it to store a chemical formula (alt: a list of atoms) - TBD |
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More for basic atm in obsevational data, not used here |
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Comment: this parameter can be misleading if used only in some services / cases - will suggest products not found do not exist at all |
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see if usage can be enlarged (e.g., to InChiKeys) - but for minerals? |
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species_inchikey ? |
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Check if required/useful |
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dataproduct_type |
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'sp' for spectra |
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spectral_range_min (& *_max) |
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Provide spectral range as frequency in Hz (EPNCore standard) |
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spectral_sampling_step_min (& *_max) |
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Provide sampling step as frequency in Hz (EPNCore standard) |
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spectral_resolution_min (& *_max) |
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spectral_resolution_min/max should instead provide | fq / Dfq | = | lam / Dlam | |
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Provides Dfreq in EPNCore 2.0 |
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(agree upon during workshop, but TBC with other fields) |
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Other ideas: |
A parameter to identify a source database in a compilation service (such as SSHADE, or PDS speclib) |
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Photometric measurement sets? |
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Optical constants: ~ two associated spectra or complex one? Description / table should be identical |
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Band lists: tables with characteristics and attributions - EPNCore is not be the best solution, see later proposal |
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