From aa2fd6111122c914a50369c5da113524a2472790 Mon Sep 17 00:00:00 2001 From: Ruby Byrne Date: Tue, 28 Mar 2023 15:22:42 -0700 Subject: [PATCH 1/2] dictionary updates --- dictionary.md | 9 ++++++++- 1 file changed, 8 insertions(+), 1 deletion(-) diff --git a/dictionary.md b/dictionary.md index 18d2d0fe..99478c60 100644 --- a/dictionary.md +++ b/dictionary.md @@ -31,7 +31,7 @@ This is a work in progress; please add keywords as you find them in alphabetical **beam_nfreq_avg**: the number of fine frequency channels to calculate a beam for, using the average of the frequencies. The beam is a function of frequency, and a calculation on the finest level is most correct (beam_nfreq_avg=1). However, this is computationally difficult for most machines.
-*Range*: 1-# of frequency channels, as long as it evenly divides the # of frequency channels
- -*Default*: 1
+ -*Default*: 16 !Q
-*eor_wrapper_defaults*: 16
**beam_offset_time**: calculate the beam at a specific time within the observation. 0 seconds indicates the start of the observation, and the # of seconds in an observation indicates the end of the observation.
@@ -492,6 +492,9 @@ WARNING! Options in this section may change without notice, and should never be ## Flagging +**channel_edge_flag_width**: number of channels to flag at the edge of each coarse band. Used only if instrument is set to "mwa" or "mwa32t".
+ -*Default*: 4 for instrument="mwa32t", depends on the number of frequency channels for instrument="mwa"
+ **dead_dipole_list**: an array of 3 x # of dead dipoles, where column 0 is the tile name, column 1 is the polarization (0:x, 1:y), and column 2 is the dipole number. These dipoles are flagged, which greatly increases memory usage due to the creation of many separate tile beams.
-*Default*: not set
@@ -520,6 +523,10 @@ WARNING! Options in this section may change without notice, and should never be -*Default*: not set
-*eor_wrapper_defaults*: 1
+**no_frequency_flagging**: do not flag frequency channels.
+ -*Turn off/on*: 0/1 (flag/don't flag)
+ -*Default*: not set
+ **no_ps** : Do not save output images in postscript format. Only png and fits.
-*Default*: 1
-*eor_wrapper_defaults*: 1
From 061c242df7c0e4750660c86f94fef225c96cddff Mon Sep 17 00:00:00 2001 From: elillesk <102777967+elillesk@users.noreply.github.com> Date: Thu, 18 Apr 2024 16:18:52 -0700 Subject: [PATCH 2/2] Update dictionary.md Adding entry for fill_model_visibilities --- dictionary.md | 4 ++++ 1 file changed, 4 insertions(+) diff --git a/dictionary.md b/dictionary.md index 99478c60..6fe0ff55 100644 --- a/dictionary.md +++ b/dictionary.md @@ -195,6 +195,10 @@ This is a work in progress; please add keywords as you find them in alphabetical -*Turn off/on*: 0/1
-*Default*: undefined (off)
+**fill_model_visibilities**: calculate model even where there are flags (without unflagging that data)
+ -*Turn off/on*: 0/1
+ -*Default*: undefined (off)
+ **gaussian_source_models**: uses SHAPE information provided in the sky catalog to build Gaussian models of extended sources. See Line et al. 2020 for more details on implementation. The models are only accurate to within ~10\%, and this is an ongoing issue (see Issue [\#211](https://github.com/EoRImaging/FHD/issues/211)).
-*Turn off/on*: 0/1
-*Default*: undefined (off)