The Zwicky Transient Facility Bright Transient Survey. I. Spectroscopic Classification and the Redshift Completeness of Local Galaxy Catalogs

@article{Fremling2019TheZT,
  title={The Zwicky Transient Facility Bright Transient Survey. I. Spectroscopic Classification and the Redshift Completeness of Local Galaxy Catalogs},
  author={U. Christoffer Fremling and A. A. Miller and Yashvi Sharma and Alison M. Dugas and Daniel A. Perley and Kirsty Taggart and Jesper Sollerman and Ariel Goobar and Melissa L. Graham and James D. Neill and Jakob Nordin and Mickael Rigault and R. Walters and Igor Andreoni and Ashot Bagdasaryan and Justin Belicki and C. Cannella and Eric C. Bellm and S. Bradley Cenko and Kishalay De and Richard Dekany and Sara Frederick and V. Zach Golkhou and Matthew J. Graham and George Helou and Anna Y. Q. Ho and Mansi M. Kasliwal and Thomas Kupfer and Russ R. Laher and Ashish A. Mahabal and Frank J. Masci and Reed L. Riddle and Ben Rusholme and Steve Schulze and David L. Shupe and R. M. Smith and Lin Yan and Yuhan Yao and Zhuyun Zhuang and Shrinivas R. Kulkarni},
  journal={arXiv: High Energy Astrophysical Phenomena},
  year={2019}
}
The Zwicky Transient Facility (ZTF) is performing a three-day cadence survey of the visible Northern sky (~3$\pi$). The transient candidates found in this survey are announced via public alerts. As a supplementary product ZTF is also conducting a large spectroscopic campaign: the ZTF Bright Transient Survey (BTS). The goal of the BTS is to spectroscopically classify all extragalactic transients brighter than 18.5 mag at peak brightness and immediately announce those classifications to the… 
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A Morphological Classification Model to Identify Unresolved PanSTARRS1 Sources. II. Update to the PS1 Point Source Catalog
  • A. Miller, X. Hall
  • Geology
    Publications of the Astronomical Society of the Pacific
  • 2021
TLDR
An update to the PanSTARRS-1 Point Source Catalog (PS1 PSC), which provides morphological classifications of PS1 sources, is presented, which finds that the new methodology, which utilizes PS1 forced photometry, performs ∼6%–8% worse than the original method.
New Modules for the SEDMachine to Remove Contaminations from Cosmic Rays and Non-target Light: byecr and contsep
Currently time-domain astronomy can scan the entire sky on a daily basis, discovering thousands of interesting transients every night. Classifying the ever-increasing number of new transients is one
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