Summary Data Products¶
Module: astra.products.pipeline_summary
Summary products are FITS files that collect pipeline results across all sources into convenient catalog tables. There are several types of summary products.
astraAllStar¶
Created by create_all_star_product(), these files contain results from a given pipeline run on co-added (star-level) spectra.
FITS structure:
HDU |
Contents |
|---|---|
0 |
Primary HDU with metadata header (pipeline name, Astra version, HDU descriptions) |
1 |
BOSS results – one row per source with a co-added BOSS spectrum analyzed by the pipeline, joined with |
2 |
APOGEE results – one row per source with a co-added APOGEE spectrum analyzed by the pipeline, joined with |
Each row contains:
Source-level information (identifiers, astrometry, photometry)
Spectrum-level metadata (SNR, radial velocities)
All pipeline output fields (stellar parameters, abundances, flags)
If the pipeline defines
flag_warnandflag_badproperties, these are included as boolean columns
File naming: astraAllStar<Pipeline>-<version>.fits (optionally gzip-compressed)
astraAllVisit¶
Created by create_all_visit_product(), these files have the same HDU structure as astraAllStar but contain per-visit results instead of per-star results.
FITS structure:
HDU |
Contents |
|---|---|
0 |
Primary HDU with metadata header |
1 |
BOSS visit-level results (using |
2 |
APOGEE visit-level results (using |
File naming: astraAllVisit<Pipeline>-<version>.fits (optionally gzip-compressed)
astraBest¶
Created by create_astra_best_product(), these files contain the “best” result per source across all pipelines. The HDU structure is simpler: a primary HDU and a single binary table extension with one row per source.
File naming: astraFrankenstein-<version>.fits
mwmStar¶
An mwmStar file contains the co-added spectra for a source, with one stacked spectrum per telescope/instrument combination.
FITS structure:
HDU |
Contents |
|---|---|
0 |
Primary HDU with source information (identifiers, photometry, astrometry) |
1 |
BOSS co-added spectrum from Apache Point Observatory ( |
2 |
BOSS co-added spectrum from Las Campanas Observatory ( |
3 |
APOGEE co-added spectrum from Apache Point Observatory ( |
4 |
APOGEE co-added spectrum from Las Campanas Observatory ( |
These represent the best available spectrum for a source and are the primary input to most Astra analysis pipelines.
File path pattern: $MWM_ASTRA/<v_astra>/spectra/star/<sdss_id_groups>/mwmStar-<v_astra>-<sdss_id>.fits
mwmVisit¶
An mwmVisit file contains all visit spectra for a source, organized by telescope and instrument.
FITS structure:
HDU |
Contents |
|---|---|
0 |
Primary HDU with source information (identifiers, photometry, astrometry) |
1 |
All BOSS spectra from Apache Point Observatory ( |
2 |
All BOSS spectra from Las Campanas Observatory ( |
3 |
All APOGEE spectra from Apache Point Observatory ( |
4 |
All APOGEE spectra from Las Campanas Observatory ( |
Key properties of mwmVisit spectra:
All wavelengths are in vacuum and in the source rest frame (unlike
apVisitwhich is in the observed frame, andspecFullwhich is in the barycentric frame).All spectra are resampled onto common wavelength grids (BOSS: 4648 pixels; APOGEE: 8575 pixels).
Spectra deemed unreliable are still included (unlike
apStar), with anin_stackboolean column indicating whether each spectrum was used for the co-added product.
File path pattern: $MWM_ASTRA/<v_astra>/spectra/visit/<sdss_id_groups>/mwmVisit-<v_astra>-<sdss_id>.fits