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Removing Atmospheric Fringes from Zwicky Transient Facility i-band Images using Principal Component Analysis

Medford, Michael S. and Nugent, Peter and Goldstein, Danny and Masci, Frank J. and Andreoni, Igor and Beck, Ron and Coughlin, Michael W. and Duev, Dmitry A. and Mahabal, Ashish A. and Riddle, Reed L. (2021) Removing Atmospheric Fringes from Zwicky Transient Facility i-band Images using Principal Component Analysis. Publications of the Astronomical Society of the Pacific, 133 (1024). Art. No. 064503. ISSN 0004-6280. doi:10.1088/1538-3873/abfe9d. https://resolver.caltech.edu/CaltechAUTHORS:20210604-142610228

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Abstract

The Zwicky Transient Facility is a time-domain optical survey that has substantially increased our ability to observe and construct massive catalogs of astronomical objects by use of its 47 square degree camera that can observe in multiple filters. However the telescope's i-band filter suffers from significant atmospheric fringes that reduce photometric precision, especially for faint sources and in multi-epoch co-additions. Here we present a method for constructing models of these atmospheric fringes using Principal Component Analysis that can be used to identify and remove these artifacts from contaminated images. In addition, we present the Uniform Background Indicator as a quantitative measurement of the reduced correlated background noise and photometric error present after removing fringes. We conclude by evaluating the effect of our method on measuring faint sources through the injection and recovery of artificial stars in both single-image epochs and co-additions. Our method for constructing atmospheric fringe models and applying those models to produce cleaned images is available for public download in the open source Python package fringez (https://github.com/MichaelMedford/fringez).


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1088/1538-3873/abfe9dDOIArticle
https://arxiv.org/abs/2102.10738arXivDiscussion Paper
https://github.com/MichaelMedford/fringezRelated Itemcode
ORCID:
AuthorORCID
Medford, Michael S.0000-0002-7226-0659
Nugent, Peter0000-0002-3389-0586
Goldstein, Danny0000-0003-3461-8661
Masci, Frank J.0000-0002-8532-9395
Andreoni, Igor0000-0002-8977-1498
Coughlin, Michael W.0000-0002-8262-2924
Duev, Dmitry A.0000-0001-5060-8733
Mahabal, Ashish A.0000-0003-2242-0244
Riddle, Reed L.0000-0002-0387-370X
Additional Information:© 2021. The Astronomical Society of the Pacific. Received 2021 February 16; accepted 2021 May 5; published 2021 June 24. This work is based on observations obtained with the Samuel Oschin Telescope 48 inch and the 60 inch Telescope at the Palomar Observatory as part of the Zwicky Transient Facility project. ZTF is supported by the National Science Foundation under grant No. AST-1440341 and a collaboration including Caltech, IPAC, the Weizmann Institute for Science, the Oskar Klein Center at Stockholm University, the University of Maryland, the University of Washington, Deutsches Elektronen-Synchrotron and Humboldt University, Los Alamos National Laboratories, the TANGO Consortium of Taiwan, the University of Wisconsin at Milwaukee, and Lawrence Berkeley National Laboratories. Operations are conducted by COO, IPAC, and UW. We acknowledge support from the University of California Office of the President for the UC Laboratory Fees Research Program In-Residence Graduate Fellowship (Grant ID: LGF-19-600357). This research used resources of the National Energy Research Scientific Computing Center, a DOE Office of Science User Facility supported by the Office of Science of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. We acknowledge support from the DOE under grant DE-AC02-05CH11231, Analytical Modeling for Extreme-Scale Computing Environments. M.W.C. acknowledges support from the National Science Foundation with grant No. PHY-2010970.
Group:Zwicky Transient Facility, Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NSFAST-1440341
ZTF partner institutionsUNSPECIFIED
University of California, Office of the PresidentLGF-19-600357
Department of Energy (DOE)DE-AC02-05CH11231
NSFPHY-2010970
Subject Keywords:Algorithms – Computational methods – Open source software – Principal component analysis – Publicly available software – Astronomical optics – CCD photometry
Issue or Number:1024
DOI:10.1088/1538-3873/abfe9d
Record Number:CaltechAUTHORS:20210604-142610228
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210604-142610228
Official Citation:Michael S. Medford et al 2021 PASP 133 064503
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:109403
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:07 Jun 2021 14:34
Last Modified:25 Jun 2021 18:15

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