Commit 9a63587eb507058fe5e924c4a3f0b990ea32b1ce

Authored by Jürgen Knödlseder
1 parent a11d582a

Update change log.

Showing 2 changed files with 22 additions and 51 deletions
ChangeLog
  1 +2015-06-02 Juergen Knoedlseder <jurgen.knodlseder@irap.omp.eu>
  2 +
  3 + * Version 0.10.0 released
  4 + =========================
  5 +
  6 + Move cscripts into the ctools Python module (#1470)
  7 +
  8 +
1 2015-05-22 Juergen Knoedlseder <jurgen.knodlseder@irap.omp.eu> 9 2015-05-22 Juergen Knoedlseder <jurgen.knodlseder@irap.omp.eu>
2 10
3 * Version 0.9.0 released 11 * Version 0.9.0 released
1 -New Features and Important Changes in ctools 0.9.0 1 +New Features and Important Changes in ctools 0.10.0
2 2
3 Author(s) : Juergen Knoedlseder 3 Author(s) : Juergen Knoedlseder
4 4
5 -22 May 2015 5 +2 June 2015
6 6
7 7
8 1. Introduction 8 1. Introduction
9 --------------- 9 ---------------
10 This document briefly summarizes executable by executable the most important 10 This document briefly summarizes executable by executable the most important
11 changes made since the last release of ctools. The code complies to GammaLib 11 changes made since the last release of ctools. The code complies to GammaLib
12 -version 1.0.0 or above. 12 +version 0.11.0 or above.
13 13
14 14
15 2. Configuration 15 2. Configuration
@@ -19,11 +19,8 @@ None @@ -19,11 +19,8 @@ None
19 19
20 3. Python interface 20 3. Python interface
21 ------------------- 21 -------------------
22 -The ctools module does no longer import automatically Python scripts. This  
23 -prevents to break the ctools interface in case that some dependencies in  
24 -the scripts are broken. Scripts (such as obsutils, analysisutils or plotutils)  
25 -are support scripts that may not be fully supported throughout the  
26 -development. They may be moved into a special contributions area in the future. 22 +The cscripts have been moved to the ctools module. Now everything is comprised
  23 +in that module.
27 24
28 25
29 4. Support model 26 4. Support model
@@ -33,14 +30,12 @@ None @@ -33,14 +30,12 @@ None
33 30
34 5. ctobssim - CTA observation simulation 31 5. ctobssim - CTA observation simulation
35 ---------------------------------------- 32 ----------------------------------------
36 -The rate check is now also correctly done for map cubes. Before, the rate check  
37 -made simulations with a diffuse map cube fail (#1452). 33 +None
38 34
39 35
40 6. ctselect - CTA event selection 36 6. ctselect - CTA event selection
41 --------------------------------- 37 ---------------------------------
42 -If INDEF, UNDEF, NONE or UNDEFINED are passed for the selection parameters, no  
43 -selection will be performed. 38 +None
44 39
45 40
46 7. ctbin - CTA event binning 41 7. ctbin - CTA event binning
@@ -50,14 +45,12 @@ None @@ -50,14 +45,12 @@ None
50 45
51 8. ctlike - Maximum likelihood fitting 46 8. ctlike - Maximum likelihood fitting
52 -------------------------------------- 47 --------------------------------------
53 -The bkgcube parameter has been added to allow specification of a background  
54 -cube for stacked analysis. 48 +None
55 49
56 50
57 9. cttsmap - Generation of Test Statistics map 51 9. cttsmap - Generation of Test Statistics map
58 ---------------------------------------------- 52 ----------------------------------------------
59 -The bkgcube parameter has been added to allow specification of a background  
60 -cube for stacked analysis. 53 +None
61 54
62 55
63 10. ctskymap - CTA sky mapping 56 10. ctskymap - CTA sky mapping
@@ -67,14 +60,7 @@ None @@ -67,14 +60,7 @@ None
67 60
68 11. ctmodel - CTA counts cube modelling 61 11. ctmodel - CTA counts cube modelling
69 --------------------------------------- 62 ---------------------------------------
70 -The ctmodel tool can now be used for stacked analysis from the command line.  
71 -It directly makes use of the cube response to compute the model without using  
72 -the original IRF information. This makes generation of model cubes substantially  
73 -faster. The old method of accessing the IRF response for model computation is  
74 -still possible.  
75 -  
76 -The bkgcube parameter has been added to allow specification of a background  
77 -cube for stacked analysis. 63 +None
78 64
79 65
80 12. ctexpcube - CTA exposure cube generation 66 12. ctexpcube - CTA exposure cube generation
@@ -99,16 +85,12 @@ None @@ -99,16 +85,12 @@ None
99 85
100 16. ctbutterfly - Generate butterfly diagrams 86 16. ctbutterfly - Generate butterfly diagrams
101 --------------------------------------------- 87 ---------------------------------------------
102 -The bkgcube parameter has been added to allow specification of a background  
103 -cube for stacked analysis. 88 +None
104 89
105 90
106 17. ctulimit - Compute upper limit 91 17. ctulimit - Compute upper limit
107 ---------------------------------- 92 ----------------------------------
108 -Added an initial version of the upper limit computation tool.  
109 -  
110 -The bkgcube parameter has been added to allow specification of a background  
111 -cube for stacked analysis. 93 +None
112 94
113 95
114 18. Examples 96 18. Examples
@@ -118,31 +100,12 @@ None @@ -118,31 +100,12 @@ None
118 100
119 19. Scripts 101 19. Scripts
120 ----------- 102 -----------
121 -The user parameter interface of cssens has been modified. The script  
122 -now reads a source model that is used for sensitivity estimation.  
123 -This provides more flexibility in the choice of the model for  
124 -sensitivity estimation.  
125 -  
126 -The csobsdef script has been added that allows creation of observation  
127 -definition XML files from colon separated value ASCII files. The  
128 -observation definition files from csobsdef can be fed to ctobssim for  
129 -simulation of multiple pointings in one shot. This enables for example  
130 -survey observations to be simulated in a single ctobssim run.  
131 -  
132 -The csspec script has been added that creates a spectrum for a given  
133 -dataset and source.  
134 -  
135 -The cslightcrv script has been added that creates a lightcurv for a given  
136 -dataset and source.  
137 -  
138 -The sensitivity computation in cssens has been corrected so that the script  
139 -actually returns the differential flux for a given set of energies. 103 +None
140 104
141 105
142 20. caldb 106 20. caldb
143 --------- 107 ---------
144 -Official Prod2 instrument response functions for the Southern and Northern  
145 -array have been added. 108 +None
146 109
147 110
148 21. models 111 21. models