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                        The Optical Gravitational Lensing Experiment.

            Supernovae and Other Transients in the OGLE-IV Magellanic Bridge Data

                    S. Kozlowski, A. Udalski, L. Wyrzykowski, R. Poleski,
                 P. Pietrukowicz, M.K. Szymanski, M. Kubiak, G. Pietrzynski,
                          I. Soszynski, K. Ulaczyk, and J. Skowron

                                2013, Acta Astronomica, 63, 1

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e-mail: simkoz@astrouw.edu.pl




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TABLE 2. Cumulative estimated number of SNe 100^-1 deg^-2 yr^-1 to the limiting peak magnitude I.

Peak               Total SN Number      Cumulative Detection        OGLE-IV SN Number*
I (mag)      All SNe      SNe Ia    ccSNe   Efficiency [%]    All SNe    SNe Ia    ccSNe
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17.0             1          1         0           100             1          1         0       
17.5             3          2         1           100             2          1         1       
18.0             6          5         1           100             4          3         1       
18.5            14         12         2           100             9          8         1       
19.0            31         28         3            83            17         15         2       
19.5            78         71         7            58            30         27         3       
20.0           224        211        13            38            56         53         3       
20.5           589        562        27            21            83         79         4       
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Notes. *The reported SNe numbers are corrected for the OGLE-IV SNe "season length" (~65% of year).