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Table 2.

Photometry of the 42 SNe IIn in the sample.

SN Epoch Magnitude Magnitude Limiting Telescope Camera Filter Reference Pipeline
(JD) (AB) error magnitude image
PTF09tm 2454959.6605 99.00 99.0 20.02 P48 CFH12K R P48ref PTFIDE
PTF09tm 2454959.7523 99.00 99.0 20.26 P48 CFH12K R P48ref PTFIDE
... ... ... ... ... ... ... ... ... ...
PTF09tm 2455005.8071 18.87 0.09 99.00 P48 CFH12K R P48ref PTFIDE
PTF09tm 2455005.8816 18.83 0.09 99.00 P48 CFH12K R P48ref PTFIDE
... ... ... ... ... ... ... ... ... ...
PTF10weh 2455724.9677 21.46 0.13 99.00 P60 GRBCam r SDSSref FPipe
PTF10weh 2455481.6718 18.69 0.01 99.00 P60 GRBCam i SDSSref FPipe
... ... ... ... ... ... ... ... ... ...
PTF11qnf 2456037.7320 19.99 0.09 99.00 P60 GRBCam r PS1ref FPipe
... ... ... ... ... ... ... ... ... ...
iPTF15aym 2457480.9090 21.31 0.06 99.00 P60 SEDM g SDSSref FPipe
... ... ... ... ... ... ... ... ... ...

Notes. All magnitudes reported are AB magnitudes from PSF photometry on reference subtracted images. The columns give the name of the SN, the Julian Date (JD) of the photometry, the magnitude and its 1σ error (if SN detected, otherwise given as “99”) or the upper limit (magnitudes, if SN not detected, otherwise given as “99”), the telescope used (P48 or P60), the camera used (CFH12K, GRBCam or SEDM), the filter used (Mould R or SDSS g for P48, SDSS griz or Johnson B for P60), the source of the reference image (P48, P60, SDSS or PS1 i.e. Pan-STARRS) and the pipeline used for the photometry (PTFIDE or FPipe). FPipe uses SDSS stars as reference stars, or PS1 stars when outside the SDSS footprint. Details on instruments etc. are given in Sect. 2. Photometric upper limits from PTFIDE are given at 5σ level. Upper limits from FPipe are given at 3σ for GRBCam and at 5σ for SEDM, respectively. Selected parts of the table are shown here, as a guide to its content. The full table is available at the CDS.

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