PhoPS: An automated photometric pipeline for survey-era astronomy

arXiv:2607.27414 · astro-ph.IM, astro-ph.EP, astro-ph.GA, astro-ph.SR · Submitted 2026-07-29 · Read on arXiv

Orhan Erece, Yucel Kilic

astro-ph.IM, astro-ph.EP, astro-ph.GA, astro-ph.SR

Submitted: 2026-07-29

Comments: 11 pages, 9 figures, 3 tables

Code: https://github.com/orhanerece/PhoPShttps:

Project page: https://iraf-community.github.io

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Calibration — 32× in this paper · explained in 7 episodes
• Aperture — 8× in this paper · explained in 1 episode
• Accuracy — 6× in this paper · explained in 1 episode
• Julian Date — 2× in this paper
• Abundance — 1× in this paper · explained in 1 episode
• After the World Coordinate System — 1× in this paper
• Aperture Photometry — 1× in this paper · explained in 1 episode
• European Space Agency — 1× in this paper
• Flexible Image Transport System — 1× in this paper
• National Optical Astronomy Observatories — 1× in this paper
• Robustness — 1× in this paper · explained in 5 episodes
• Verification — 1× in this paper · explained in 2 episodes

Sources

• Do fast stellar centroiding methods saturate the Cram'{e}r-Rao lower bound?

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