Astronomy · Observatories, surveys and archives
Catalogues, detection limits and selection
Treat catalogue entries as documented measurements, then distinguish selection probability, completeness and purity with original examples whose denominators remain explicit.
Continue in the approved chapter order. Necessary vocabulary, quantities and assumptions are explained in the lesson.
Back to the chapterAfter reading, you can
- Read a catalogue row together with its quantity definitions, observing context and quality information.
- Explain how selection changes the distribution of an observed sample.
- Calculate completeness and purity for a declared known-truth example and state what the calculation cannot establish.
A catalogue row needs a data model
An astronomical catalogue is a documented collection of entries and measured or derived quantities. A row might describe a detection, a combined source estimate or a candidate selected for a particular purpose. Its relation to a physical object is part of the catalogue’s data model.
Read the release, quantity definitions, units, band, observing epoch, coordinate conventions and uncertainty information. A derived temperature or distance is not the same kind of quantity as a detector count. Its meaning depends on the inputs and the method that produced it.
One row need not represent one isolated star. Crowded sources can blend; one physical object can be split into detections; measurements in different bands can be matched incorrectly. The 2MASS explanatory notes provide concrete examples of crowding, artefacts, merging and deblending limitations.
Quality flags identify specified concerns under the release’s definitions. A flag is a reason to investigate its meaning, not a universal verdict that a row is unusable. An unflagged value is likewise not a guarantee of physical truth or perfect measurement.
Inclusion probability can change the apparent class mixture
A selection function describes the probability of inclusion under declared observations and processing. It can depend on position, brightness, colour, angular extent, crowding and other relevant properties. It belongs to a specified sample and measurement design, not to an object in all possible observing circumstances.
Consider an original synthetic parent population containing exactly 100 objects of class A and 100 of class B. Stipulate inclusion probabilities 0.8 for A and 0.2 for B. The expected selected counts are 100 × 0.8 = 80 and 100 × 0.2 = 20.
Class A is half the parent population, but its ratio of expected selected counts is 80 / (80 + 20) = 0.8. Equal parent counts can therefore produce an unequal selected mixture. The plotted values are expectations, not promised observed counts; random realised samples can differ.
The ratio of expected counts is not in general the expectation of a random realised sample fraction. Here it supplies a transparent teaching comparison. Applying such a model to data would require evidence for the selection probabilities and the eligible population, with uncertainty retained.
| Class | Parent objects | Inclusion probability | Expected selected objects |
|---|---|---|---|
| A | 100 | 0.8 | 80 |
| B | 100 | 0.2 | 20 |
Equal parents, unequal expected selection
Scroll sideways to see the full diagram. Its explanation is below.
A denominator determines what a quality fraction means
Completeness asks what fraction of eligible true objects were included. Purity, also called reliability under some stated conventions, asks what fraction of selected candidates are genuine members of the desired class. The denominators differ.
In a known-truth synthetic test, stipulate 100 eligible true objects. A loose cut includes 80 of them and 40 false candidates. Its completeness is 80/100 = 0.8, while its purity is 80/(80 + 40) = 2/3, about 66.7 percent.
A stricter cut, chosen as a subset of that loose selection in this example, includes 60 true objects and 10 false candidates. Completeness is 60/100 = 0.6; purity is 60/70 = 6/7, about 85.7 percent. Here the stricter choice improves purity while losing true objects. That tradeoff is a result of this stipulated test, not a theorem about every cut.
Real estimates need a validation strategy, such as suitable comparison data or injection-and-recovery tests, together with matching rules and uncertainty. The truth labels stipulated here are not obtained merely by reading the candidate list. Completeness and contamination can vary across brightness, position, morphology and observing conditions.
| Selection | True included | False included | Completeness | Purity |
|---|---|---|---|---|
| Loose | 80 | 40 | 80/100 = 80% | 80/120 ≈ 66.7% |
| Strict subset | 60 | 10 | 60/100 = 60% | 60/70 ≈ 85.7% |
A larger list does not automatically repair missing information
A catalogue’s footprint is one part of selection. Overlapping fields must be counted as a union, and repeated entries must be related to their source identities. Adding counts without that accounting can count the same opportunity or object more than once.
For a probability example, stipulate two independent inclusion opportunities with probabilities 0.5 and 0.4. Inclusion at least once has probability 0.5 + 0.4 − 0.5 × 0.4 = 0.7, not 0.9. Multiplication for the overlap is justified only by the declared independence. Dependent selections require their actual joint model.
With known nonzero selection probabilities, inverse-probability methods can help estimate population quantities under appropriate assumptions. The expectation example gives 80/0.8 + 20/0.2 = 200 when applied to its expected counts. This illustrates the model; it does not validate a correction for an actual catalogue.
If a region or class has zero inclusion probability, the catalogue contains no direct sample of that missing component to recover by division. Uncertain selection, measurement error and dependence also need modelling. The retained survey-selection Foundation develops a deeper version of this relationship rather than promising an automatic cure.
Use catalogue documentation as part of the scientific argument
The Gaia Data Release 3 collaboration paper illustrates that related catalogue products can use different input choices and selection thresholds, with distinct completeness and contamination limitations. Its historical examples support the method of reading a release; they do not establish the latest release or current mission status.
The Subaru survey design and 2MASS cautionary notes similarly show that depth, observing conditions and processing affect what enters a list. Their documentation is useful precisely because it describes a particular measurement and release, rather than an ideal census of everything that exists.
A missing entry therefore does not by itself establish that a physical source is absent. An entry does not by itself establish every proposed classification or derived property. A population claim must explain how observations, selection, quantity definitions and inference connect.
The next lesson follows that connection into archives. Reusing a catalogue or image requires enough metadata and provenance to identify its inputs, processing and limits, including relationships between products that share observations.
Worked examples
Separate the parent mixture from expected selection
In the stipulated 100 A and 100 B population, what follows from inclusion probabilities 0.8 and 0.2?
- Expected selected A = 100 × 0.8 = 80; expected selected B = 100 × 0.2 = 20.
- The parent A fraction is 100/200 = 0.5.
- The ratio of expected selected A counts to expected total is 80/100 = 0.8.
Different inclusion probabilities change the selected mixture. These are expectations, and they do not establish a universal class abundance.
Check which question a percentage answers
Why does the loose known-truth test have 80 percent completeness but only about 66.7 percent purity?
- Completeness divides the 80 included true objects by all 100 eligible true objects.
- Purity divides those same 80 genuine candidates by all 120 selected candidates.
- The 40 false candidates enter the purity denominator, not the eligible-truth denominator.
The two fractions answer different questions about the same selection. Neither can replace the other.
Try the reasoning
Does absence from a catalogue prove that a source does not exist?
Show the answer and reasoning
No.
Coverage, sensitivity, crowding, masking and processing or selection can prevent inclusion.
What is the strict synthetic cut’s completeness if it includes 60 of 100 eligible true objects?
Show the answer and reasoning
60 percent.
The denominator is the 100 eligible true objects, not its 70 selected candidates.
May two inclusion probabilities always be multiplied to calculate their overlap?
Show the answer and reasoning
No.
That product requires independence; a general union uses the actual joint inclusion probability.
Can inverse weighting of selected entries alone recover a class with zero inclusion probability?
Show the answer and reasoning
No.
There are no sampled entries from that component, and division by zero does not supply missing evidence.
What to carry forward
- Catalogue entries obtain their meaning from quantity definitions, context and release documentation.
- Selection can reshape an observed sample before any population inference is made.
- Completeness and purity need distinct denominators and an appropriate validation model.
References
Teaching resources and research supporting this lesson’s explanations and examples.
- seestar: Selection functions for spectroscopic surveys of the Milky WayAndrew Everall and Payel Das (2019)Reference guide
- 2MASS All-Sky Data Release Explanatory Supplement — Point Source Catalog cautionary notes2MASS team / NASA-IPAC Infrared Science ArchiveReference guide
- Gaia Data Release 3: Summary of the content and survey propertiesGaia Collaboration, A. Vallenari et al., 2022 accepted manuscript; arXiv 2208.00211v1Reference guide
- Hyper Suprime-Cam Subaru Strategic Program — SurveyHSC-SSP / Subaru / National Astronomical Observatory of JapanReference guide