Astronomy · Observatories, surveys and archives
Archives, metadata and data provenance
Trace measurements through their inputs and processing, then examine how documented citizen classifications contribute evidence without becoming automatic discoveries or independent confirmations.
Continue in the approved chapter order. Necessary vocabulary, quantities and assumptions are explained in the lesson.
Back to the chapterAfter reading, you can
- Distinguish archive access, metadata, provenance and verification.
- Recognise shared observations beneath multiple data products.
- Interpret a conditional classification fraction and separate contribution, candidate and verified discovery.
A reusable file needs a documented meaning
An astronomical archive provides access to retained observations and data products. Downloading a file is the beginning of reuse: the scientific question still requires an understanding of what its values mean, how they were obtained and whether they are suitable for the proposed comparison.
Metadata describe the data and their context. Useful information includes the target or field, observing time and time system, instrument and band, coordinate frame, units, exposure information, uncertainty quantities, masks, quality flags and release identity. The exact requirements depend on the intended analysis.
Provenance describes relationships between inputs, producing activities, outputs and responsible agents. Here an agent means a person, organisation or system with a recorded role. The IVOA Provenance Data Model formalises these relationships so that processing history can be represented and shared.
A filename or timestamp alone cannot supply that history. Nor does an archive’s name guarantee that every relevant processing setting is recorded. The amount of available detail must be checked against what the proposed inference needs.
| Information | Question it helps answer |
|---|---|
| Observation IDs, field, band and time conventions | Which original measurements and epochs contribute? |
| Quantity definitions, units and uncertainty fields | What is measured or derived, and how uncertain is it? |
| Calibration and software versions, settings | Which relations and transformations produced the output? |
| Masks, flags, exclusions and selection | Which measurements or objects could be missing or unreliable? |
| Product/release identity and responsible groups | Which documented version is being used? |
| Usage terms, acknowledgements and citations | How should the material be reused and attributed? |
A traceable history supports checking but does not certify truth
The Hubble Spectroscopic Legacy Archive documentation gives a concrete example: science quantities and errors have defined units, while provenance information identifies contributing spectra, instruments, exposure details and calibration versions. Its coadded products also have documented quality and exclusion rules.
Calibration itself relates instrument indications to reference values under stated conditions with uncertainties. Knowing a calibration filename is helpful provenance, but it does not establish all those metrological conditions. A file lineage alone is not a demonstration of a measurement result’s metrological traceability.
Reproducibility asks whether a sufficiently specified analysis can be repeated to obtain its stated result under the relevant conditions. A reproducible pipeline can still use an unrepresentative sample, an inappropriate model or a mistaken calibration. Provenance helps locate and examine such possibilities rather than removing the need to test them.
Related releases can also reuse observations. The Gaia Data Release 3 collaboration paper illustrates why product definitions, input choices and limitations must be read at the release level. Counting published catalogues is not the same as counting independent observations.
Documented public contributions can become research inputs
Citizen-science projects invite members of the public to contribute to research tasks. NASA’s Galaxy Zoo introduction describes classifying galaxy images through questions. These classifications can provide useful evidence when the project documents how they are recorded, combined, checked and related to the scientific question.
The historical Galaxy Zoo 2 release paper describes image, participant and time associations, handling of repeated user-image submissions, user weighting and comparisons with overlapping expert and automated catalogues. Those documented methods describe that release; they should not be assumed to specify every later project.
An image’s apparent size, quality and viewing conditions can affect its classification. Decision-tree tasks can also have conditional denominators: a classification may reach one question only after particular earlier answers. A classification that never reaches a task is not automatically a “no” answer to it.
Raw vote fractions, weighted fractions and fractions adjusted for a documented classification bias are different quantities. Their definitions and assumptions need to be read before interpretation. Agreement between methods sharing images or assumptions is valuable evidence with dependencies, rather than automatic independent ground truth.
State the fraction and the level of verification
For an original hypothetical decision-tree example, 50 classifications concern one image. Only 20 reach a particular task, and 16 of those answer yes. The raw conditional task fraction is 16/20 = 0.8. The fraction of all 50 classifications following that yes branch is 16/50 = 0.32.
These fractions answer different questions. Neither is the percentage of galaxies in the Universe with that feature, a calibrated 80 percent probability of physical truth, or a verified discovery. Actual release columns may use weighting or bias adjustments absent from this simple unweighted example.
A participant’s documented contribution, a candidate identification, subsequent checking and a verified discovery are distinct states. A surprising classification can motivate investigation; scientific claims require appropriate validation, comparison and sometimes new observations. Credit and attribution follow the project and data-release records rather than a promise attached to every click.
Archives and public participation widen the community able to examine evidence. Their value grows when quantities, history, selection and verification remain inspectable. The next original chapter changes physical focus to gravity and orbits, while retaining this discipline of connecting measurements to the models they can support.
| Count or fraction | Value | Denominator or scope |
|---|---|---|
| All classifications | 50 | One image |
| Classifications reaching task | 20 | Conditional path in the question tree |
| Yes answers at task | 16 | Those reaching this task |
| Conditional yes fraction | 16/20 = 0.8 | Task responses |
| Whole-path fraction | 16/50 = 0.32 | All classifications of this image |
Worked examples
Follow the shared inputs before adding exposure
Two archive products each use the same E1 and E2 exposures of 300 seconds each, with different calibration inputs. How much unique original target exposure is represented?
- Identify the original exposure IDs rather than counting output filenames.
- E1 contributes 300 seconds and E2 contributes 300 seconds once each to the unique set.
- Both processing branches use that same set, so two outputs do not double it.
600 seconds of unique original target exposure. The products can differ, but they do not constitute 1,200 seconds of new observations or automatic independent confirmation.
Keep the task denominator visible
In the synthetic classification example, why are both 0.8 and 0.32 legitimate fractions?
- Sixteen yes answers among the twenty task responses give 16/20 = 0.8.
- Sixteen classifications following that branch among all fifty give 16/50 = 0.32.
- The other thirty classifications did not reach the task, so treating all thirty as task-level no votes changes the question.
The fractions describe different denominators. Neither directly measures a universal physical population fraction or verifies a discovery.
Try the reasoning
Does an observation date in a filename supply complete data provenance?
Show the answer and reasoning
No.
Inputs, quantities, processing, versions, conditions, exclusions and responsible roles may also be needed.
Are two reductions of the same exposures independent new observations?
Show the answer and reasoning
No.
They can reveal processing differences while retaining shared measurement noise and limitations.
Does 16 out of 20 yes votes establish an 80 percent calibrated probability that a physical interpretation is true?
Show the answer and reasoning
No.
That is a raw conditional task fraction in the invented example. Validation, image limitations and the inference model remain relevant.
Can a reproducible analysis still have a selection bias or wrong physical model?
Show the answer and reasoning
Yes.
Reproducing a calculation checks a different property from the suitability of its inputs and assumptions.
What to carry forward
- Metadata give quantities and context; provenance connects inputs, activities, outputs and responsibilities.
- Shared input observations remain shared evidence across different products and releases.
- Citizen classifications contribute documented research inputs whose denominators, validation and attribution must be stated.
References
Teaching resources and research supporting this lesson’s explanations and examples.
- IVOA Provenance Data Model v1.0, Recommendation 11 April 2020Mathieu Servillat et al. / International Virtual Observatory AllianceReference guide · PDF
- Hubble Spectroscopic Legacy Archive — file structure, provenance and caveatsMAST / Space Telescope Science InstituteReference guide
- Galaxy ZooNASA Science Citizen ScienceReference guide
- Galaxy Zoo 2: detailed morphological classifications for 304122 galaxies from the Sloan Digital Sky SurveyKyle W. Willett et al. (2013), MNRAS; arXiv 1308.3496Reference guide
- Gaia Data Release 3: Summary of the content and survey propertiesGaia Collaboration, A. Vallenari et al., 2022 accepted manuscript; arXiv 2208.00211v1Reference guide
- International vocabulary of metrology, third edition, JCGM200:2012Joint Committee for Guides in Metrology / BIPMReference guide · PDF