WebJan 28, 2024 · 31 2 5 While it might also be on-topic in photography-SE, I think it's perfectly on-topic here as astronomical data reduction has its own quirks beyond "normal" photography and is an essential part of observational work – planetmaker Jan 28, 2024 at 15:41 2 "My final goal is to obtain the best image possible to perform the source extraction." WebPSF Photometry NIRISS WFSS Spectra - Optimal Extraction WFSS Spectra - Combine and Normalize 1D Spectra ... Astropy modeling for fitting a line to the residuals of the background subtraction Astropy block_reduce for looking at the RMS of the residuals as a function of scale (blocking factor) import numpy as np from scipy import stats, ndimage ...
CCDData — Astropy v5.2.3.dev0+g32d49b960.d20240411
WebWe performed point-spread function (PSF) fitting using the Astropy Photutils package v0.6 on shallow HST Wide Field Camera 3 images taken in filters F110W, F139M, and F160W … Web10.5 PSF construction and subtraction. The point spread function (PSF) describes how the light of a point-like source is affected by several optical scattering effects (atmosphere, … burlington vt to washington dc
Table Operations — Astropy v5.2.3.dev0+g32d49b960.d20240411
WebFirst, you pick the PSF function, which is a 2D gaussian in this case. Then, the routine will choose a centroid, mu, and variance (or mus and variances). A couple of things that will … WebFirst, you pick the PSF function, which is a 2D gaussian in this case. Then, the routine will choose a centroid, mu, and variance (or mus and variances). A couple of things that will complicate the routine. i) Local peak due to a noise. This will mess up the centroid. WebJul 5, 2024 · In principle, no. psf_model x_0, y_0, and flux as parameters. Member Maybe related to astropy/astropy#6027 which added a fwhm attribute which is a scalar (so no .value attribute) ? value Contributor Gaussian2D: @saimn (or x_0 and y_0 this Fittable2DModel Contributor I tried with prepare_psf_model but still no luck. hal steakhouse