Quantifying the poor purity and completeness of morphological samples selected by galaxy colour

The galaxy population is strongly bimodal in both colour and morphology, and the two measures correlate strongly, with most blue galaxies being late-types (spirals) and most early-types, typically ellipticals, being red. This observation has led to the use of colour as a convenient selection criteri...

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Bibliographic Details
Published in:Monthly notices of the Royal Astronomical Society 2021-12, Vol.510 (3)
Main Authors: Smethurst, Rebecca Jane, Masters, Karen L., Simmons, Brooke D., Garland, Izzy L., Géron, Tobias, Häußler, Boris, Kruk, Sandor, Lintott, Chris John, O’Ryan, David, Walmsley, Mike
Format: Article
Language:English
Subjects:
abundances
astronomy
ASTRONOMY AND ASTROPHYSICS
astrophysics
disc
elliptical
evolution
galaxies
lenticular
statistics
structure
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Summary:The galaxy population is strongly bimodal in both colour and morphology, and the two measures correlate strongly, with most blue galaxies being late-types (spirals) and most early-types, typically ellipticals, being red. This observation has led to the use of colour as a convenient selection criterion to make samples that are then labelled by morphology. Such use of colour as a proxy for morphology results in necessarily impure and incomplete samples. In this paper, we make use of the morphological labels produced by Galaxy Zoo to measure how incomplete and impure such samples are, considering optical (ugriz), near-ultraviolet (NUV), and near-infrared (NIR; JHK) bands. The best single colour optical selection is found using a threshold of g - r = 0.742, but this still results in a sample where only 56 per cent of red galaxies are smooth and 56 per cent of smooth galaxies are red. Use of the NUV gives some improvement over purely optical bands, particularly for late-types, but still results in low purity/completeness for early-types. No significant improvement is found by adding NIR bands. With any two bands, including NUV, a sample of early-types with greater than two-thirds purity cannot be constructed. In conclusion, advances in quantitative galaxy morphologies have made colour–morphology proxy selections largely unnecessary going forward; where such assumptions are still required, we recommend studies carefully consider the implications of sample incompleteness/impurity.
ISSN:0035-8711
1365-2966