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authordencheva <dencheva@stsci.edu>2012-10-31 15:13:58 -0400
committerdencheva <dencheva@stsci.edu>2012-10-31 15:13:58 -0400
commit2c50a08d025cb82ac0dda2294b4cefea992c36a5 (patch)
treeb8b4044d4da608512e07858c888278833b255c0d /doc
parent06c6706c3b6df0702779446633fa9ee6e1ad022a (diff)
downloadstwcs_hcf-2c50a08d025cb82ac0dda2294b4cefea992c36a5.tar.gz
formatting the tsr
git-svn-id: http://svn.stsci.edu/svn/ssb/stsci_python/stsci_python/trunk/stwcs@20136 fe389314-cf27-0410-b35b-8c050e845b92
Diffstat (limited to 'doc')
-rw-r--r--doc/headerlet_tsr/source/hdrlet_tsr.rst23
-rw-r--r--doc/headerlet_tsr/source/index.rst20
2 files changed, 19 insertions, 24 deletions
diff --git a/doc/headerlet_tsr/source/hdrlet_tsr.rst b/doc/headerlet_tsr/source/hdrlet_tsr.rst
index 6ab423b..398e58f 100644
--- a/doc/headerlet_tsr/source/hdrlet_tsr.rst
+++ b/doc/headerlet_tsr/source/hdrlet_tsr.rst
@@ -1,26 +1,3 @@
-==================================================================
-Definition of a Headerlet and Its Role in Updating WCS Information
-==================================================================
-
-.. abstract::
- :author: Warren Hack, Nadezhda Dencheva
- :date: 22 Oct 2012
-
-
- A headerlet is a self-consistent representation of a single WCS solution for a single
- exposure complete with all distortion information. FITS is the data
- storage format currently supported. It has no observational data
- which makes it relatively small and light to distribute.
- It is, essentially, a mechanism for encapsulating WCS information
- which can later be used to update the WCS of a science file and allows
- improved astrometric solutions to be stored and passed around easily.
- The HST archive is expected to start accepting headerlets for HST data soon.
- However the implementaiton is not HST specific and FITS WCS standard, as well as
- all WCS conventions implemented in pywcs are supported.
- This report describes the format and contents of a headerlet
- along with the software implementation and methods for creating headerlets and using them
- to update the WCS of a science observation.
-
Introduction
============
diff --git a/doc/headerlet_tsr/source/index.rst b/doc/headerlet_tsr/source/index.rst
index c6ef136..cec192c 100644
--- a/doc/headerlet_tsr/source/index.rst
+++ b/doc/headerlet_tsr/source/index.rst
@@ -1,8 +1,26 @@
.. Headerlet Definition TSR master file
TSR 2012-02: Definition of a Headerlet and Its Role in Updating WCS Information
-================================================================================
+===============================================================================
+.. abstract::
+ :author: Warren Hack, Nadezhda Dencheva
+ :date: 22 Oct 2012
+
+ A headerlet is a self-consistent representation of a single WCS solution for a single
+ exposure complete with all distortion information. FITS is the data
+ storage format currently supported. It has no observational data
+ which makes it relatively small and light to distribute.
+ It is, essentially, a mechanism for encapsulating WCS information
+ which can later be used to update the WCS of a science file and allows
+ improved astrometric solutions to be stored and passed around easily.
+ The HST archive is expected to start accepting headerlets for HST data soon.
+ However the implementaiton is not HST specific and FITS WCS standard, as well as
+ all WCS conventions implemented in pywcs are supported.
+ This report describes the format and contents of a headerlet
+ along with the software implementation and methods for creating headerlets and using them
+ to update the WCS of a science observation.
+
Contents:
.. toctree::