VizieR Online Data Catalog: Type IIP supernovae from Pan-STARRS1 (Sanders+, 2015)

We select an SN II light-curve sample from the transients discovered and monitored by Pan-STARRS1 (PS1) since the initiation of the survey in 2010, consisting of 18953 relevant photometric data points, 5096 of which are robust transient detections. The PS1 observations are obtained through a set of five broadband filters, which we refer to interchangeably as g_P1, r_P1, i_P1, z_P1, and y_P1 or simply grizy (Stubbs et al. 2010ApJS..191..376S).

We begin with a selection of PS1-discovered SNe that were classified as Type II through our spectroscopic follow-up campaign: 112 objects in total. Spectra were obtained using the Blue Channel and Hectospec spectrographs of the 6.5m MMT telescope, the Low Dispersion Survey Spectrograph (LDSS3) and Inamori-Magellan Areal Camera and Spectrograph (IMACS) of the 6.5m Magellan telescopes, the Gemini Multi-Object Spectrograph of the 8m Gemini telescopes (GMOS), and the Andalucia Faint Object Spectrograph and Camera (ALFOSC) at the 2.6m Nordic Optical Telescope. Details of our final SN IIP sample, as described in Section 3.4, are listed in Table 1.

(4 data files).