HI-MaNGA is a 21cm follow-up program for the SDSS-IV MaNGA survey, a survey of 10,010 unique galaxies with an Integral Field Unit (for resolved optical spectroscopy). The primary goal of HI-MaNGA is to observe all z<0.05 MaNGA galaxies with the Green Bank Telescope which lack HI data from other sources.
Acknowledgement
For publications that make use of these data please cite Masters et al. 2019 and Stark et al. 2021.
Please also acknowledge the GBT Legacy Archive and the Observatory by including the following acknowledgements in your publication:
This publication makes use of the GBT Legacy Archive.
The Green Bank Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Data Releases
Catalogs
Data
Additionally, here is the README for DR3 data and DR3.1 Catalog.