TITLE: GCN CIRCULAR NUMBER: 24320 SUBJECT: LIGO/Virgo S190425z: KPED Follow-Up of ZTF transients DATE: 19/04/28 05:08:34 GMT FROM: Tomas Ahumada at U. of Maryland Tomas Ahumada (UMD), Michael W. Coughlin (Caltech), Kai Staats (Northwestern), Kevin Burdge (Caltech), Richard G. Dekany (Caltech), Dmitry A. Duev (Caltech), Michael Feeney (Caltech), S. R. Kulkarni (Caltech), Reed Riddle (Caltech) on behalf of the KPED team and the Global Relay of Observatories Watching Transients Happen (GROWTH) collaboration. We used the Kitt Peak EMCCD Demonstrator (KPED) on the Kitt Peak 84-inch telescope (Coughlin et al 2019b) to obtain 300 s r-band images for ZTF optical transients listed in Kasliwal et al. (GCN 24191) and Anand et al. (GCN 24311) starting at 9:13:24 UT on 2019-04-27. The measurement of ZTF19aasckkq is consistent with Perley et al. (GCN 24314) and we report upper limits for the rest of the transients. Magnitudes are derived after calibrating against PS1: ID JD RA DEC magnitude ZTF19aasckkq 2458600.9291 248.413102 13.910183 r = 20.29 +- 0.18 ZTF19aaskbzh 2458600.9541 206.393046 69.329244 r > 19.65 +- 0.03 ZTF19aasejil 2458600.9837 261.945810 1.653720 r > 20.38 +- 0.34 ZTF19aasckkm 2458600.9248 247.302345 12.930679 r > 19.79 +- 0.18 More observations for this objects are scheduled. The KPED team thanks the National Science Foundation, the National Optical Astronomical Observatory and the Murty family for support in the building and operation of KPED.