Images
MIGHTEE Continuum Data Release 1
Below are a selection of jpeg images from the MIGHTEE continuum Data Release 1 (DR1). For access to the full data, see the data access page.
If you use these images, please credit Hale et al. (in press)
COSMOS
Full size image here.
COSMOS zoom
Full size image here.
COSMOS - high resolution
Full size image here.
COSMOS zoom - high resolution
Full size image here.
XMM-LSS
Full size image here.
XMM-LSS zoom
Full size image here.
XMM-LSS - high resolution
Full size image here.
XMM-LSS zoom - high resolution
Full size image here.
CDFS-DEEP
Full size image here.
CDFS-DEEP zoom
Full size image here.
CDFS-DEEP - high resolution
Full size image here.
CDFS-DEEP zoom - high resolution
Full size image here.
MIGHTEE Continuum Early Science Data
Below are a selection of jpeg images from the MIGHTEE continuum early science data. For access to the full data, see the data access page.
If you use these images, please credit Heywood et al. (2022).
MIGHTEE HI
The discovery of a large gas-rich group with MIGHTEE. If you use these images please cite Ranchod et al. (2021).
Optical image of the galaxy group with 3-colour optical images of each member galaxy using data from the Hyper-Suprime Camera on the Subaru telescope. The red outline indicates the extent of the neutral hydrogen gas around each galaxy. (Credit: Shilpa Ranchod/MIGHTEE/HSC project)
A 3-colour optical image from the Hyper-Suprime Camera on the Subaru telescope of two of the group galaxies. The diffuse red structure is the neutral hydrogen gas, which envelops both galaxies, and indicates they are in the process of merging. (Credit: MIGHTEE/HSC Project)
MIGHTEE Giant Radio Galaxies
Two giant radio galaxies in the COSMOS field. If you use this image please cite Delhaize et al. (2021). Full size image here.
MIGHTEE-HI
This gif shows resolved rotational velocity maps of a subset of MIGHTEE-HI galaxies.
Red shows gas that is moving away from the observer, and blue show gas moving towards us.
If you use this gif please cite Ponomareva et al. (2021).