VizieR Online Data Catalog: IR water vapor emission from planet-forming disks (Banzatti+, 2023)

Water rovibrational emission spectra at 2.9-2.98μm are included as observed with the Cryogenic High-Resolution IR Echelle Spectrograph (CRIRES) on Very Large Telescope (VLT) as part of a survey from 2007-2008 (R=95000).

Water rovibrational emission spectra at 5μm are included as observed with iSHELL at the NASA Infrared Telescope Facility (IRTF), as part of an ongoing M-band survey of protoplanetary disks. iSHELL covers a wide portion of the observable M band at 4.5~5.25μm with a resolution of 60000.

Water rotational emission spectra at 12.2-12.9μm were obtained within a Large Program with VLT Imager and Spectrometer for the Mid-Infrared (VISIR), (R=30000).

Additional water rotational emission spectra at 12.2-12.4μm are included as obtained with Texas Echelon Cross Echelle Spectrograph (TEXES) on Gemini with a resolving power of 100000.

(2 data files).