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Title: Real-time Recovery Efficiencies and Performance of the Palomar Transient Factory's Transient Discovery Pipeline

Abstract

In this paper, we present the transient source detection efficiencies of the Palomar Transient Factory (PTF), parameterizing the number of transients that PTF found versus the number of similar transients that occurred over the same period in the survey search area but were missed. PTF was an optical sky survey carried out with the Palomar 48 inch telescope over 2009–2012, observing more than 8000 square degrees of sky with cadences of between one and five days, locating around 50,000 non-moving transient sources, and spectroscopically confirming around 1900 supernovae. We assess the effectiveness with which PTF detected transient sources, by inserting $$\simeq 7$$ million artificial point sources into real PTF data. We then study the efficiency with which the PTF real-time pipeline recovered these sources as a function of the source magnitude, host galaxy surface brightness, and various observing conditions (using proxies for seeing, sky brightness, and transparency). The product of this study is a multi-dimensional recovery efficiency grid appropriate for the range of observing conditions that PTF experienced and that can then be used for studies of the rates, environments, and luminosity functions of different transient types using detailed Monte Carlo simulations. Finally, we illustrate the technique using the observationally well-understood class of type Ia supernovae.

Authors:
ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [2];  [3]
  1. Univ. of Southampton (United Kingdom)
  2. Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  3. Stanford Univ., CA (United States)
Publication Date:
Research Org.:
Univ. of Southampton (United Kingdom); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR) (SC-21); European Research Council (ERC); Science and Technology Facilities Council (STFC) (United Kingdom)
OSTI Identifier:
1379822
Grant/Contract Number:  
AC02-05CH11231; 615929
Resource Type:
Journal Article: Accepted Manuscript
Journal Name:
The Astrophysical Journal. Supplement Series (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal. Supplement Series (Online); Journal Volume: 230; Journal Issue: 1; Journal ID: ISSN 1538-4365
Publisher:
American Astronomical Society/IOP
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; data analysis methods; supernovae; surveys

Citation Formats

Frohmaier, C., Sullivan, M., Nugent, P. E., Goldstein, D. A., and DeRose, J. Real-time Recovery Efficiencies and Performance of the Palomar Transient Factory's Transient Discovery Pipeline. United States: N. p., 2017. Web. doi:10.3847/1538-4365/aa6d70.
Frohmaier, C., Sullivan, M., Nugent, P. E., Goldstein, D. A., & DeRose, J. Real-time Recovery Efficiencies and Performance of the Palomar Transient Factory's Transient Discovery Pipeline. United States. doi:10.3847/1538-4365/aa6d70.
Frohmaier, C., Sullivan, M., Nugent, P. E., Goldstein, D. A., and DeRose, J. Tue . "Real-time Recovery Efficiencies and Performance of the Palomar Transient Factory's Transient Discovery Pipeline". United States. doi:10.3847/1538-4365/aa6d70. https://www.osti.gov/servlets/purl/1379822.
@article{osti_1379822,
title = {Real-time Recovery Efficiencies and Performance of the Palomar Transient Factory's Transient Discovery Pipeline},
author = {Frohmaier, C. and Sullivan, M. and Nugent, P. E. and Goldstein, D. A. and DeRose, J.},
abstractNote = {In this paper, we present the transient source detection efficiencies of the Palomar Transient Factory (PTF), parameterizing the number of transients that PTF found versus the number of similar transients that occurred over the same period in the survey search area but were missed. PTF was an optical sky survey carried out with the Palomar 48 inch telescope over 2009–2012, observing more than 8000 square degrees of sky with cadences of between one and five days, locating around 50,000 non-moving transient sources, and spectroscopically confirming around 1900 supernovae. We assess the effectiveness with which PTF detected transient sources, by inserting $\simeq 7$ million artificial point sources into real PTF data. We then study the efficiency with which the PTF real-time pipeline recovered these sources as a function of the source magnitude, host galaxy surface brightness, and various observing conditions (using proxies for seeing, sky brightness, and transparency). The product of this study is a multi-dimensional recovery efficiency grid appropriate for the range of observing conditions that PTF experienced and that can then be used for studies of the rates, environments, and luminosity functions of different transient types using detailed Monte Carlo simulations. Finally, we illustrate the technique using the observationally well-understood class of type Ia supernovae.},
doi = {10.3847/1538-4365/aa6d70},
journal = {The Astrophysical Journal. Supplement Series (Online)},
number = 1,
volume = 230,
place = {United States},
year = {Tue May 09 00:00:00 EDT 2017},
month = {Tue May 09 00:00:00 EDT 2017}
}

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