J-PLUS: Turning Off the Bright Stars
arXiv:2510.12940 · doi:10.1051/0004-6361/202556547
Abstract
Photometric surveys require precise point spread function (PSF) characterization, as it varies across filters and is crucial for accurate photometry and low surface brightness (LSB) studies. However, the small PSF size provided by default pipelines suits only barely resolved objects, making it difficult to analyze regions near bright stars (rendering those regions unusable). These components are then combined to generate a final PSF for each exposure and filter, spanning 15 mag arcsec-2 in surface brightness and 4 arcmin in radius in the broad bands. In narrow-band filters, the J-PLUS PSF exhibits two rings, whereas in broad-band filters, only one ring is observed. Additionally, the position of the ring shifts with filter wavelength: as the filters become redder, the ring radius increases. We find that there is no significant variation in the extended PSF observed as a function of time (within 2.5h) or position in the field of view. The radial profile of NGC 4212 (which is close to a star) is also studied before/after PSF-subtraction. We developed a novel method to determine the central coordinates of saturated stars, and classify stars without using Gaia magnitudes. Additionally, mirror reflections are automatically detected and masked. Furthermore, in combining different stars and various components of the PSF, we avoided the use of a fixed radius by introducing a new method that does not depend on radial measurements. Accurate characterization of the extended PSF and its subtraction improves sky subtraction, increases the effective area of the survey by about 10%, and enables the study of extended large LSB features in wide area surveys like J-PLUS. Our pipeline is published as free software (GNU GPLv3) an can be customized to other surveys such as J-PAS, where its impact will be even greater due to its depth. This paper is fully reproducible and produced from Commit 4860c70.
Accepted for publication in A&A. Supplementary data on Zenodo (http://doi.org/10.5281/zenodo.17348653), project source on Gitlab (https://gitlab.com/Sepideh.Esk/psf-j-plus) and archived on Software Heritage (swh:1:dir:fc95ed9ad173de6fa64690e3d71ab041c630f32c; see text for usage). Abstract is summarized to fit arXiv limit
References in corpus (30)
- Gaia Data Release 3: Summary of the content and survey properties
- Toward High-Precision Astrometry with WFPC2. I. Deriving an Accurate PSF
- J-PLUS: The Javalambre Photometric Local Universe Survey
- The effects of seeing on Sersic profiles. II. The Moffat PSF
- Beyond 31 mag/arcsec^2: the low surface brightness frontier with the largest optical telescopes
- Noise Based Detection and Segmentation of Nebulous Objects
- The ghost of a dwarf galaxy: fossils of the hierarchical formation of the nearby spiral galaxy NGC 5907
- The bright-star masks for the HSC-SSP survey
- The miniJPAS survey: a preview of the Universe in 56 colours
- Galactic cirri in deep optical imaging
- The influence of diffuse scattered light I. The PSF and its role to observations of the edge-on galaxy NGC 5907
- The effects of seeing on Sersic profiles
- Removing Internal Reflections from Deep Imaging Datasets
- The Sloan Digital Sky Survey extended point spread functions
- The Extended Optical Disk of M101
- Stellar Photometry and Astrometry with Discrete Point Spread Functions
- The influence of diffuse scattered light II. Observations of galaxy haloes and thick discs and hosts of BCGs
- The reports of thick discs' deaths are greatly exaggerated: thick discs are NOT artefacts caused by diffuse scattered light
- Photometry and astrometry with JWST -- I. NIRCam Point Spread Functions and the first JWST colour-magnitude diagrams of a globular cluster
- Euclid preparation: XVI. Exploring the ultra low-surface brightness Universe with Euclid/VIS
- Dragonfly imaging of the galaxy NGC5907: a revised view of the iconic stellar stream
- Stellar Disc Truncations and Extended Haloes in Face-on Spiral Galaxies
- A Method To Characterize the Wide-Angle Point Spread Function of Astronomical Images
- Properties of extragalactic thick discs recovered from ultra-deep Stripe82 imaging
- Strategies for optimal sky subtraction in the low surface brightness regime
- A Study of the Point Spread Function in SDSS Images
- Ultra-deep Imaging: Structure of Disks and Haloes
- A Recipe for Unbiased Background Modeling in Deep Wide-Field Astronomical Images
- Accurate PSF-matched photometry and photometric redshifts for the Extreme Deep Field with the Chebyshev-Fourier functions
- Validation of PSF Models for HST and Other Space-Based Observations