dark_subtract¶
Subtract a master dark from ctx.image.
| Category | Preprocessing (2-D image) |
| Backend | numpy - implemented here on top of numpy primitives |
| Version | 1.0.0 |
| Reads | ctx.image (an ImageFrame) |
| Writes | image |
Reads the master dark from ctx.extras['master_dark'] (an ImageFrame) or from dark_key if you stored it under a different key.
Parameters¶
| Parameter | Default | Required | Description |
|---|---|---|---|
dark_key |
'master_dark' |
- | Key in ctx.extras where the master dark is stored. |
scale_by_exptime |
True |
- | Scale the dark by EXPTIME(science)/EXPTIME(dark) before subtracting. |
Use it¶
The CLI loads a single 1-D spectrum with --input; this algorithm needs
ctx.image (an ImageFrame). Run it from Python or as a step of a pipeline preset.
References¶
- Howell 2006 — Handbook of CCD Astronomy, ch. 4.
Related algorithms¶
correct_slant_affine- Make monochromatic lines parallel to the rows by a horizontal shear.correct_smile_polynomial- Undo smile curvature via the Schroeder even-order expansion.correct_tilt_affine- Re-align the slit with the detector columns by a vertical shear.denoise_gaussian_2d- Separable isotropic Gaussian smoothing ofctx.image.denoise_median_2d- Square median filter overctx.image, optionally banded by rows.flat_normalize- Dividectx.imageby a master flat normalised to unity.flat_normalize_easyspec- Flat-field correct a science frame viacleaning.flatten.outlier_rejection_mad_adaptive- Replace pixels whose deviation from a local median exceedsthreshold·MAD.subtract_bias_easyspec- Subtract a master bias from a single science frame viacleaning.debias.subtract_dark_easyspec- Subtract a master dark from a science frame viacleaning.sub_dark.subtract_sky_2d- Subtract a per-column sky model fitted from off-trace rows ofctx.image.