From 28d6a659e7a4b5cc0471c350e5c4edc207d3b36d Mon Sep 17 00:00:00 2001 From: Connor Stone Date: Thu, 21 Nov 2024 14:08:29 -0500 Subject: [PATCH] docs: fix faq --- docs/source/frequently_asked_questions.rst | 6 +++--- 1 file changed, 3 insertions(+), 3 deletions(-) diff --git a/docs/source/frequently_asked_questions.rst b/docs/source/frequently_asked_questions.rst index 870ff8a9..2cc82761 100644 --- a/docs/source/frequently_asked_questions.rst +++ b/docs/source/frequently_asked_questions.rst @@ -5,7 +5,7 @@ FAQs - Frequently asked questions | **A:** If you are using any ``Module``` object (so a simulator), then you can get the parameters using ``print(simulator)``. The order of the dynamical parameters (top to bottom) corresponds to the order you should use in your -parameter value tensor. Note that you can ignore the static parameters. | +parameter value tensor. Note that you can ignore the static parameters. | **Q:** Why can I put the lens redshift at higher values than the source redshift or to negative values for some parametric models? | **A:** We can calculate everything for those profiles with reduced deflection @@ -13,7 +13,7 @@ angles where the redshifts do not actually play into the calculation. If you use a profile defined by the lens mass, like a NFW lens, or a Multiplane lens then it does matter that the redshifts make sense and you will very likely get errors for those. Similarly, if you call the ``lens.physical_deflection_angle`` you -will encounter errors. | +will encounter errors. | **Q:** I do (multiplane-)lensing with pixelated convergence using the pixelated kappa map of a parametric profile. The lensing effect differs from directly using the parametric lens. Why is the lensing effect different? @@ -24,4 +24,4 @@ will encounter errors. | have to increase the resolution and/or FOV of your pixelated convergence map. Especially for SIE or EPL profiles (which go to infinity density in the center, and have infinite mass outside any FOV) you will miss infinite mass - when pixelating. | + when pixelating.