VizieR Online Data Catalog: UV, optical and IR light curve of supernova SN2019dge (Yao+, 2020)

SN2019dge was discovered by Zwicky Transient Facility (ZTF), which runs on the Palomar Oschin Schmidt 48-inch (P48) telescope. We perform forced point-spread function (PSF) photometry on ZTF difference images generated with the ZTF real-time reduction and image subtraction pipeline.

Following the discovery of SN2019dge, we obtain follow-up photometry in ugriz with an optical imager on the Liverpool Telescope (LT).

Observations with the Neil Gehrels Swift Observatory (Swift) was triggered on April 9 and April 10. Ultraviolet/Optical Telescope (UVOT) data were obtained in the UVW1, UVM2, UVW2, U, B, and V filters.

(1 data file).