From 57b6d07540ab26c5cc7b3c21db133efa50a5fa06 Mon Sep 17 00:00:00 2001 From: Kyle Westfall Date: Fri, 1 Oct 2021 16:13:10 -0700 Subject: [PATCH] CHANGES --- CHANGES.rst | 7 ++----- 1 file changed, 2 insertions(+), 5 deletions(-) diff --git a/CHANGES.rst b/CHANGES.rst index fc4be7faa5..1f76a509c2 100644 --- a/CHANGES.rst +++ b/CHANGES.rst @@ -1,7 +1,7 @@ -1.5.1.dev ---------- +1.6.0 (1 Oct 2021) +------------------ - Modifications to reduce header crashes - Added `image_proc.rst` doc, which includes a table with the primary parameters @@ -31,15 +31,12 @@ from the tabulated value. - Whether or not you add the shot noise and a noise floor to the variance image are now optional and controlled by parameters in ProcessImagesPar. - - Changes to default ProcessImagesPar parameters: use_specillum = False for all frame types; shot_noise = False and noise_floor = 0 for biases; and use_overscan=True, use_biasimage=True, noise_floor=0., and mask_cr=True for darks. Adjustments propagated to individual spectrographs. - - BPM is not recalculated after applying the flat-field correction because it is not longer changed by that function. - - The code keeps track of the image scaling via the flat-field correction, and propagates this to the noise model. - Compute and save a "base-level variance" that includes readnoise, dark