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Journal article : Review

MIGHTEE-HI: The H I emission project of the MeerKAT MIGHTEE survey

Abstract:
We present the H I emission project within the MIGHTEE survey, currently being carried out with the newly commissioned MeerKAT radio telescope. This is one of the first deep, blind, medium-wide interferometric surveys for neutral hydrogen (H I) ever undertaken, extending our knowledge of H I emission to z = 0.6. The science goals of this medium-deep, medium-wide survey are extensive, including the evolution of the neutral gas content of galaxies over the past 5 billion years. Simulations predict nearly 3000 galaxies over 0 <  z <  0.4 will be detected directly in H I, with statistical detections extending to z = 0.6. The survey allows us to explore H I as a function of galaxy environment, with massive groups and galaxy clusters within the survey volume. Additionally, the area is large enough to contain as many as 50 local galaxies with H I mass < 108 M⊙, which allows us to study the low-mass galaxy population. The 20 deg2 main survey area is centred on fields with exceptional multi-wavelength ancillary data, with photometry ranging from optical through far-infrared wavelengths, supplemented with multiple spectroscopic campaigns. We describe here the survey design and the key science goals. We also show first results from the Early Science observations, including kinematic modelling of individual sources, along with the redshift, H I, and stellar mass ranges of the sample to date.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1051/0004-6361/202039655

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Role:
Author


Publisher:
EDP Sciences
Journal:
Astronomy and Astrophysics More from this journal
Volume:
646
Issue:
February 2021
Article number:
A35
Publication date:
2021-02-02
Acceptance date:
2020-11-10
DOI:
EISSN:
1432-0746
ISSN:
0004-6361


Language:
English
Keywords:
Subtype:
Review
Pubs id:
1161374
Local pid:
pubs:1161374
Deposit date:
2021-03-10

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