PetroFit: A Python Package for Computing Petrosian Radii and Fitting Galaxy Light Profiles
arXiv:2202.13493 · doi:10.3847/1538-3881/ac5908 10.48550/arXiv.2202.13493
Abstract
PetroFit is an open-source Python package, based on Astropy and Photutils, that can calculate Petrosian profiles and fit galaxy images. It offers end-to-end tools for making accurate photometric measurements, estimating morphological properties, and fitting 2D models to galaxy images. Petrosian metric radii can be used for model parameter estimation and aperture photometry to provide accurate total fluxes. Correction tools are provided for improving Petrosian radii estimates affected by galaxy morphology. PetroFit also provides tools for sampling Astropy-based models (including custom profiles and multi-component models) onto image grids and enables PSF convolution to account for the effects of seeing. These capabilities provide a robust means of modeling and fitting galaxy light profiles. We have made the PetroFit package publicly available on GitHub (PetroFit/petrofit) and PyPi (pip install petrofit).
arXiv commentPublished AJ, 28 pages, 17 figures, see https://github.com/PetroFit/petrofit; typos corrected, footnote on PSFModel class, paper status update, DOI provided
References in corpus (19)
- SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
- Array Programming with NumPy
- Astropy: A Community Python Package for Astronomy
- Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Main Galaxy Sample
- Detailed Decomposition of Galaxy Images. II. Beyond Axisymmetric Models
- The Relationship Between Stellar Light Distributions of Galaxies and their Formation Histories
- The Luminosity Function of Galaxies in SDSS Commissioning Data
- A concise reference to (projected) Sersic R^{1/n} quantities, including Concentration, Profile Slopes, Petrosian indices, and Kron Magnitudes
- The Frontier Fields: Survey Design
- The optical morphologies of galaxies in the IllustrisTNG simulation: a comparison to Pan-STARRS observations
- Structural and Photometric Classification of Galaxies - I. Calibration Based on a Nearby Galaxy Sample
- A Correlation between Galaxy Light Concentration and Supermassive Black Hole Mass
- An investigation into the prominence of spiral galaxy bulges
- Total Galaxy Magnitudes and Effective Radii from Petrosian Magnitudes and Radii
- On the estimation of galaxy structural parameters: the Sersic Model
- Brightest Cluster Galaxy Profile Shapes
- The ASTRODEEP Frontier Fields Catalogues: I - Multiwavelength photometry of Abell-2744 and MACS-J0416
- Correlations among global photometric properties of disk galaxies
- The Relationship Between the Sersic Law Profiles Measured Along the Major and Minor Axes of Elliptical Galaxies
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