From 495348a1ee902b40c7df3fba26533202d37ddeec Mon Sep 17 00:00:00 2001
From: Roman Krivonos <krivonos@cosmos.ru>
Date: Thu, 5 Dec 2024 17:12:01 +0300
Subject: [PATCH] Acknowledgements

---
 scripts/03_grxe_flux.sh    | 23 -----------------------
 scripts/03_grxe_galprof.py |  4 ++--
 scripts/03_grxe_map.py     |  2 +-
 scripts/README.md          |  8 ++++----
 4 files changed, 7 insertions(+), 30 deletions(-)

diff --git a/scripts/03_grxe_flux.sh b/scripts/03_grxe_flux.sh
index f66375a..e69de29 100644
--- a/scripts/03_grxe_flux.sh
+++ b/scripts/03_grxe_flux.sh
@@ -1,23 +0,0 @@
-#./03_grxe_flux.py GC06 1
-#./03_grxe_flux.py GC06 2
-#./03_grxe_flux.py GC06 3
-#./03_grxe_flux.py GC06 4
-#./03_grxe_flux.py GC06 5
-#./03_grxe_flux.py GC06 10
-#./03_grxe_flux.py GC06 15
-#./03_grxe_flux.py GC06 20
-#./03_grxe_flux.py GC06 25
-#./03_grxe_flux.py GC06 30
-#./03_grxe_flux.py GC06 35
-#./03_grxe_flux.py GC06 40
-#./03_grxe_flux.py GC06 45
-#./03_grxe_flux.py GC06 50
-#./03_grxe_flux.py GC06 55
-#./03_grxe_flux.py GC06 60
-#./03_grxe_flux.py GC06 65
-#./03_grxe_flux.py GC06 70
-#./03_grxe_flux.py GC06 75
-#./03_grxe_flux.py GC06 80
-#./03_grxe_flux.py GC06 85
-#./03_grxe_flux.py GC06 90
-#./03_grxe_flux.py GC06 95
diff --git a/scripts/03_grxe_galprof.py b/scripts/03_grxe_galprof.py
index 36aedb6..a13fb83 100755
--- a/scripts/03_grxe_galprof.py
+++ b/scripts/03_grxe_galprof.py
@@ -110,8 +110,8 @@ for i in range(lon_nbin):
 
     sg_mean,sg_sem,skew_val,skew_err  = get_spec(df0, sigma=sigma,  grxe_err_cut=grxe_err_cut, enkey=enkey, plotme=True, nscw_min=nscw_min, gaussfit=True)
         
-    nsel = int(df0.shape[0]*simfrac/100)
-    print("lon {:.2f} ".format(glon[i]),"nsel=",nsel,df0.shape[0])
+    #nsel = int(df0.shape[0]*simfrac/100)
+    #print("lon {:.2f} ".format(glon[i]),"nsel=",nsel,df0.shape[0])
 
     #print('sg_sem',sg_sem)
     mean_map[i] = sg_mean
diff --git a/scripts/03_grxe_map.py b/scripts/03_grxe_map.py
index aea1939..dd2e49d 100755
--- a/scripts/03_grxe_map.py
+++ b/scripts/03_grxe_map.py
@@ -143,7 +143,7 @@ for i in range(sx):
         #print('sg_sem',sg_sem)
         mean_map[j][i] = sg_mean
         sem_map[j][i]  = sg_sem
-        sign_map[j][i] = sg_mean/sg_sem
+        #sign_map[j][i] = sg_mean/sg_sem
         cnt_map[j][i]  = df0.shape[0]
 
 """ Filter by error map """
diff --git a/scripts/README.md b/scripts/README.md
index 87d6b57..18b4022 100644
--- a/scripts/README.md
+++ b/scripts/README.md
@@ -16,11 +16,11 @@ Calibrates Crab detector count rate model.
 
 ### 01_crabmodel_plot_poly.py
 
-Plot long-term Crab detector count rate approximated by cubic polynomial function (Fig. B7 in paper).
+Plot long-term Crab detector count rate approximated by cubic polynomial function (Fig. B8 in paper).
 
 ### 01_crabmodel_plot_sys.py
 
-Plots the normalized distribution of the residuals between the IBIS/ISGRI Crab count rate and the corresponding polynomial fit (Fig. B8 in the paper). The distribution is approximated with a Gaussian function. 
+Plots the normalized distribution of the residuals between the IBIS/ISGRI Crab count rate and the corresponding polynomial fit (Fig. B9 in the paper). The distribution is approximated with a Gaussian function. 
 
 ### 02_grxe_resid.py/02_grxe_resid.sh
 
@@ -28,9 +28,9 @@ Calculates difference between detector count rate and that predicted by backgrou
 
 ### 02_grxe_resid_plot.py
 
-Plots normalized distribution of the relative residuals of the background model obtained in three energy bands for BKG region (Figs. A5 and A6 in the paper).
+Plots normalized distribution of the relative residuals of the background model obtained in three energy bands for BKG region (Figs. A6 and A7 in the paper).
 
-### 02_grxe_map.py/03_grxe_map.sh
+### 03_grxe_map.py
 
 Makes the map of the residuals in mCrab units (not shown in the paper).