Skip to content

Commit

Permalink
fixed reference to xrt_teem in getting_started.rst
Browse files Browse the repository at this point in the history
  • Loading branch information
jslavin committed Oct 10, 2023
1 parent 551ed1b commit d63e365
Showing 1 changed file with 3 additions and 3 deletions.
6 changes: 3 additions & 3 deletions docs/getting_started.rst
Original file line number Diff line number Diff line change
Expand Up @@ -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.

Expand All @@ -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.
Expand Down

0 comments on commit d63e365

Please sign in to comment.