Supernovae in Low‐Redshift Galaxy Clusters: Observations by the Wise Observatory Optical Transient Search (WOOTS)

Abstract

We describe the Wise Observatory Optical Transient Search (WOOTS), a survey for supernovae (SNe) and other variable and transient objects in the fields of redshift 0.06-0.2 Abell galaxy clusters. We present the survey design and data analysis procedures, and our object detection and follow-up strategies. We have obtained follow-up spectroscopy for all viable SN candidates and present the resulting SN sample here. Out of the 12 SNe we have discovered, 7 are associated with our target clusters while 5 are foreground or background field events. All but 1 of the SNe (a foreground field event) are Type Ia SNe. Our noncluster SN sample is uniquely complete, since all SN candidates have been either spectroscopically confirmed or ruled out. This allows us to estimate that the sample of field (noncluster) SNe, found in flux-limited surveys similar to WOOTS, would be dominated (~80%) by SNe Ia. Our spectroscopic follow-up observations also elucidate the difficulty in distinguishing active galactic nuclei from SNe. In separate papers we use the WOOTS sample to derive the SN rate in clusters for this redshift range and to measure the fraction of intergalactic cluster SNe. We also briefly report here on some quasars and asteroids discovered by WOOTS.