TITLE: GCN CIRCULAR NUMBER: 24190 SUBJECT: LIGO/Virgo S190425z: Xinglong/Schmidt follow-up observations DATE: 19/04/25 16:21:40 GMT FROM: Dong Xu at NAOC/CAS Dong Xu, Zi-Pei Zhu, Bang-Yao Yu, Tian-Meng Zhang, Xu Zhou, Xiao-Ming Teng, Peng-Fei Liu, Xiang-Nan Guan (NAOC), Sheng Yang (INAF-OAPd), Hai-Bin Zhao, Bin Li (PMO), Jin-Zhong Liu, Hu-Biao Niu, Jun-Hui Liu, Xuan Zhang (XAO), Ji-Rong Mao, Jin-Ming Bai (YNAO), Xing Gao (Urumqi No.1 Senior High School) report on behalf of the GWFUNC collaboration: We performed the search for the optical counterpart of LIGO/Virgo S190425z (GCN 24168) using the 0.9-m Schmidt telescope located at Xinglong, Hebei, China. Observations started at 12:40:09 UT on 2019-04-25 and ended at 13:42:18 UT on 2019-04-25, and the 1.5 x 1.5 deg^2 imager scanned high probability regions of the LVC localization that are accessible to the Xinglong/Schmidt telescope. The unfiltered images were taken with 60 sec exposure time and typical limiting depth is around 18 mag. The searching was stopped by growing heavy clouds. Listed below are the field centers observed. RA(J2000) DEC(J2000) 15:01:34.100 +29:55:26.00 15:01:29.990 +31:25:33.00 15:01:30.100 +32:55:36.00 15:08:22.990 +29:55:27.00 15:08:33.290 +31:25:29.00 15:08:37.090 +32:55:24.00 15:15:20.500 +29:55:46.00 15:15:34.890 +31:25:28.00 15:15:40.000 +32:54:55.00 14:43:21.790 +34:25:01.00 14:43:19.900 +35:54:50.00 14:43:19.590 +37:24:42.00 14:50:26.690 +34:25:58.00 14:50:44.790 +35:55:17.00 14:50:38.800 +37:24:51.00 14:57:44.190 +34:25:15.00 14:58:09.000 +35:55:29.00 14:58:07.900 +37:25:22.00 15:22:27.600 +29:55:45.00 15:22:37.500 +31:25:34.00 15:22:37.190 +32:55:04.00 15:29:39.890 +29:55:55.00 15:29:35.400 +31:26:06.00 15:29:39.600 +32:55:48.00 14:21:09.600 +34:24:48.00 14:21:03.590 +35:54:44.00 14:21:05.100 +37:24:14.00 14:28:32.890 +34:24:47.00 14:28:31.000 +35:54:32.00 14:28:30.400 +37:24:52.00 14:35:40.790 +34:24:50.00 14:35:55.700 +35:54:37.00 14:35:56.300 +37:23:56.00 15:06:26.900 +34:25:18.00 15:06:06.990 +35:55:32.00 Data analysis is ongoing. Optical transient(s) from the above fields, if interesting, will be reported later.