Deposited in DRO : 01 December 2016 Version of attached le : Published Version Peer-review status of attached le :

@inproceedings{Jian2018DepositedID,
  title={Deposited in DRO : 01 December 2016 Version of attached le : Published Version Peer-review status of attached le :},
  author={Hung-Yu Jian and Lihwai Lin and Kai-Yang Lin and Sebastien Foucaud and Chin-Wei Chen and Tzihong Chiueh and R. G. Bower and Shaun Cole and Wen-Ping Chen and W. S. Burgett and P. W. Draper and H. Flewelling and M. E. Huber and N. Kaiser and R.-P. Kudritzki and E. A. Magnier and N. Metcalfe and R. J. Wainscoat and C. Waters},
  year={2018}
}
  • Hung-Yu Jian, Lihwai Lin, +16 authors C. Waters
  • Published 2018
We make use of a catalog of 1600 Pan-STARRS1 groups produced by the probability friends-of-friends algorithm to explore how the galaxy properties, i.e., the specific star formation rate (SSFR) and quiescent fraction, depend on stellar mass and group-centric radius. The work is the extension of Lin et al. In this work, powered by a stacking technique plus a background subtraction for contamination removal, a finer correction and more precise results are obtained than in our previous work. We… CONTINUE READING