The Palomar Transient Factory photometric calibration
E. O. Ofek, R. Laher, N. Law, J. Surace, D. Levitan, B. Sesar, A., Horesh, D. Poznanski, J. C. van Eyken, S. R. Kulkarni, P. Nugent, J., Zolkower, R. Walters, M. Sullivan, M. Agueros, L. Bildsten, J. Bloom, S. B., Cenko, A. Gal-Yam, C. Grillmair, G. Helou, M. M. Kasliwal

TL;DR
This paper details the photometric calibration process of the Palomar Transient Factory, establishing a reliable magnitude system for R and g bands with high precision and consistency across different observing conditions.
Contribution
It introduces a calibration method using SDSS standards, enabling accurate photometry and transformations for PTF data across various sky regions and conditions.
Findings
Achieved 0.02-0.04 mag precision in calibrated PTF data.
Calibrated data are consistent within ~0.02 mag across nights.
Provided transformation guides to SDSS and Johnson-Cousins systems.
Abstract
The Palomar Transient Factory (PTF) provides multiple epoch imaging for a large fraction of the sky. Here we describe the photometric calibration of the PTF data products that relates the PTF magnitudes to other mag systems. The calibration process utilizes SDSS r~16 mag point source objects as photometric standards. During photometric conditions, this allows us to solve for the extinction coefficients and color terms, and to estimate the camera illumination correction. This also enables the calibration of fields that are outside the SDSS footprint. We test the precision and repeatability of the PTF photometric calibration. Given that PTF is observing in a single filter each night, we define a PTF calibrated magnitude system for R-band and g-band. We show that, in this system, 59% (47%) of the photometrically calibrated PTF R-band (g-band) data achieve a photometric precision of…
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