From d63e3652c0bf61c4d7c2bb64c10a6d477b2a72c5 Mon Sep 17 00:00:00 2001 From: Jonathan Slavin Date: Tue, 10 Oct 2023 11:46:00 -0400 Subject: [PATCH] fixed reference to xrt_teem in getting_started.rst --- docs/getting_started.rst | 6 +++--- 1 file changed, 3 insertions(+), 3 deletions(-) diff --git a/docs/getting_started.rst b/docs/getting_started.rst index 1c549ce7a..ac7ad6c8b 100644 --- a/docs/getting_started.rst +++ b/docs/getting_started.rst @@ -33,7 +33,7 @@ The XRT default emission model is `CHIANTI`_ atomic database version 10.0 with c Deriving Temperature and Emission Measure for a Pair of Images -------------------------------------------------------------- -XRTpy provides a routine, *xrt_teem*, that employs the objects listed above to derive the temperature and emission +XRTpy provides a routine, *temperature_from_filter_ratio*, that employs the objects listed above to derive the temperature and emission measure in for a given pair of images using the filter ratio method. This uses the same methods as in the SolarSoft IDL routine of the same name. Familiarize yourself with the utilization of this function through the notebook example provided on our Example page. @@ -42,11 +42,11 @@ Enhancing Images Sharpness with Point Spread Function - Deconvolution --------------------------------------------------------------------- Deconvolution is a powerful technique used to enhance image sharpness by mitigating the blurring effect caused by the telescope's point spread function (PSF). It is particularly useful for removing the blurring -around sharp objects or features in the XRT image. To learn how to use *xrt_deconvolve*, refer to the notebook examples provided on our Example page. +around sharp objects or features in the XRT image. To learn how to use *deconvolve*, refer to the notebook examples provided on our Example page. Subtracting Light Leak from XRT Synoptic Composite Images --------------------------------------------------------- -We have developed a specialized function designed to subtract light leak, *xrt_remove_lightleak*, which refers to visible stray +We have developed a specialized function designed to subtract light leak, *remove_lightleak*, which refers to visible stray light, from XRT synoptic composite images. By applying this function, you can effectively remove the unwanted artifacts caused by light leak, resulting in cleaner and more accurate images for further analysis and interpretation. Explore our Example page for a notebook example that demonstrate the usage of this function.