NGC 3198 was one of 18 galaxies targeted by the Hubble Space Telescope (HST) Key Project on the Extragalactic Distance Scale, which aimed to calibrate various secondary distance indicators and determine the Hubble constant to an accuracy of 10%. The type and orientation of NGC 3198 made it suitable for these measurements.[8] The Wide Field and Planetary Camera 2 (WFPC2) of the HST was used to measure the magnitudes of 52 Cepheid variables, and the resulting distance modulus corresponded to a distance of 14.5 Mpc (47 million light years).[8]
SN 1966J (typeIa, mag. 13)[10] was discovered by Paul Wild on 18 December 1966.[11] Some sources list this supernova as a typeIb.[3]
At magnitude 17.8, SN 1999bw was significantly fainter than expected when discovered, and was initially classified as a Type IIn supernova.[12] In 2021, researchers reclassified it as a gap transient.[13][14]
^"SN1966J". Transient Name Server. IAU. Retrieved 31 August 2024.
^Gingerich, Owen (22 December 1966). "Circular No. 1986". Central Bureau for Astronomical Telegrams. Smithsonian Astrophysical Observatory. Retrieved 2 December 2024.