MaNGA galaxy properties -- I. An extensive optical, mid-infrared photometric, and environmental catalogue

Understand

We present an extensive catalog of non-parametric structural properties derived from optical and mid-infrared imaging for 4585 galaxies from the MaNGA survey.

• DESI and WISE imaging are used to extract surface brightness profiles in the g, r, z, W1, W2 photometric bands.
• Our optical photometry takes advantage of the automated algorithm AutoProf and probes surface brightnesses that typically reach below 29 mag/arcsec^2 in the r band, while our WISE photometry achieves 28 mag/arcsec^2 in the W1 band.
• Neighbour density measures and central/satellite classifications are also provided for a large sub-sample of the MaNGA galaxies.