{"push_id":672592373,"size":20,"distinct_size":3,"ref":"refs/heads/master","head":"df7aafa3c91ac5708d0bfbadd60ab1b277521aab","before":"0ebb3d4e010e6d86585fd58ed65a997bccf8f6f0","commits":[{"sha":"ef111a31efb573b826bb91e51b0b6b4589abc572","author":{"email":"44fad0f7d1d4dbca2fcd645d90bd24a0825e6cb8@astro.princeton.edu","name":"Jim Bosch"},"message":"Set config default to proceed with CModel fits even when shape fails.","distinct":false,"url":"https://api.github.com/repos/HyperSuprime-Cam/meas_multifit/commits/ef111a31efb573b826bb91e51b0b6b4589abc572"},{"sha":"13eb9dcbabc1e822c848a07856a53a27b9de7bc7","author":{"email":"44fad0f7d1d4dbca2fcd645d90bd24a0825e6cb8@astro.princeton.edu","name":"Jim Bosch"},"message":"Ensure initial flux scale estimates are always positive.\n\nWhen fitting objects that are pure noise (which\nnow happens frequently when fitting in other than\nthe detection band), fall back to the RMS to set\nthe photometric scale for the problem when the\nflux is 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