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Table · dataset · 2026

WALLABY Hydra I cl. H I galaxy morphometrics

Listed in IVOA Registry (Virtual Observatory)

Galaxy morphology in atomic hydrogen (H I) and in the ultraviolet (UV) are closely linked.

Description

This has motivated their combined use to quantify morphology over the full H I disc for both H I and UV imaging. We apply galaxy morphometrics: concentration, asymmetry, gini, M20 and multimode-intensity-deviation statistics to the first moment-0 maps of the WALLABY Survey of galaxies in the hydra cluster centre.

Taking advantage of this new H I survey, we apply the same morphometrics over the full H I extent on archival GALEX FUV and NUV data to explore how well H I truncated, extended ultraviolet disc (XUV) and other morphological phenomena can be captured using pipeline WALLABY data products. Extended H I and UV discs can be identified relatively straightforward from their respective concentration. Combined with WALLABY H I, even the shallowest GALEX data are sufficient to identify XUV discs.

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Our second goal is to isolate galaxies undergoing ram-pressure stripping in the H I morphometric space. We employ four different machine learning techniques, a decision tree, a k-nearest neighbour, a support-vector machine, and a random forest. Up to 80 per cent precision and recall are possible with the random forest giving the most robust results.

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Stated by source
Optical · Radio
Inferred from text
Astronomical sciences 69% · Imaging 75%
Provenance · 1 source records, 11 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/mnras/521/150213 d agoJSON v1
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concepts[modality].ivoa_waveband:radiosource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].local:modality:imagingenrichment · IVOA Registrykeyword-concept-rules@1.0.0title+description (75%)
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