Background Estimation

The module provides tools and algorithms for estimating the background of astronomical data.

Usage

Estimating backgrounds is an important step in performing photometry. Ideally, we could perfectly describe the background with a scalar value or with some distribution. Unfortunately, it's impossible for us to precisely separate the background and foreground signals. Here, we use mixture of robust statistical estimators and meshing to let us get the spatially varying background from an astronomical photo.

Let's show an example

using Photometry
using FITSIO
using Plots

# Download our image, courtesy of astropy
hdu = FITS(download("https://github.com/astropy/photutils-datasets/raw/master/data/M6707HH.fits"))
image = read(hdu[1])'

default(aspect_ratio=1, size=(600, 600),
    xlims=(1, size(image, 2)), ylims=(1, size(image, 1)))

heatmap(image, size=(500, 500))