A test of Ca ii H & K photometry for isolating massive globular clusters below the metallicity floor
Bas van Heumen, William E. Harris, S{\o}ren S. Larsen, Else Starkenburg

TL;DR
This study evaluates the effectiveness of Ca II H & K photometry in identifying massive, extremely metal-poor globular clusters like EXT8, demonstrating its potential for candidate selection with minimal influence from horizontal branch morphology.
Contribution
It introduces and tests CaHK photometry as a reliable method for selecting metal-poor GCs below the metallicity floor, improving candidate identification accuracy.
Findings
CaHK colours can distinguish GCs below the metallicity floor.
CaHK photometry reduces false positives in candidate selection.
Horizontal branch morphology has limited impact on CaHK colours.
Abstract
The serendipitous discovery of the M31 globular cluster (GC) EXT8 has presented a significant challenge to current theories for GC formation. By finding other GCs similar to EXT8, it should become clear if and/or how EXT8 can fit into our current understanding of GC formation. We aim to test the potential of integrated-light narrow-band Ca II H & K photometry as a proxy for the metallicity of GCs to be able to provide effective candidate selection for massive GCs below the GC metallicity floor ([Fe/H] -2.5), such as EXT8. We investigate the behaviour of two colours involving the CaHK filter employed by the Pristine survey, CaHK-u and CaHK-g, as a function of metallicity through CFHT MegaCam imaging of EXT8 and a wide set of M31 GCs covering the metallicity range of -2.9 [Fe/H] +0.4. Additionally, we investigate if the CaHK colours are strongly influenced by…
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Taxonomy
TopicsSurface Roughness and Optical Measurements
