add ASCII to CLI bump version 0.0.5.2

README.md

@@ -18,6 +18,8 @@ $ pip install rgbmaker
 # Usage
 ```bash
 $ rgbmaker -h
+usage: rgbmaker [-h] [-p POSITION] [-r RADIUS] [-i IMAGESOPT] [-n NAME] [-a ARCHIVES] [-k KIND] [-s SPIDX_FILE] [-px PIXELS] [-A ANNOT]
+                [-S FLUX_LIST] [-S_e FLUX_ERROR] [-freq FREQ_LIST]
 
             _                     _             
            | |                   | |            
@@ -28,40 +30,37 @@ $ rgbmaker -h
        __/ |                                    
       |___/                                     
 
-
-usage: rgbmaker [-h] [-p POSITION] [-r RADIUS] [-i IMAGESOPT] [-n NAME] [-a ARCHIVES] [-k KIND] [-s SPIDX_FILE]
-                [-px PIXELS] [-A ANNOT]
-
 A python package which communicates to different 
-astronomical services and fetches fits and numerical data.
+astronomical services and fetches fits and numerical data
+
 
 optional arguments:
   -h, --help            show this help message and exit
   -p POSITION, --position POSITION
-                        (Required) The object name or the coordinates of the object in the FK5 (J2000) system. Ex: "14 09 48.86
-                        -03 02 32.6", M87, NGC1243, without quotes.
+                        (Required) The object name or the coordinates of the object in the FK5 (J2000) system. Ex: "14 09 48.86 -03 02
+                        32.6", M87, NGC1243, without quotes.
   -r RADIUS, --radius RADIUS
-                        (Required) (default = 0.12) (float) The size of the image in degrees, this size will be used for the field
-                        of view in the resultant image. For reference, in the night sky, the moon is about 0.52 degrees across.
+                        (Required) (default = 0.12) (float) The size of the image in degrees, this size will be used for the field of
+                        view in the resultant image. For reference, in the night sky, the moon is about 0.52 degrees across.
   -i IMAGESOPT, --imagesopt IMAGESOPT
                         (default=2)(string)(values=1,2,3) IOU ROR Optical (option = 1) Composite Contours on DSS2R (option = 2)
-  -n NAME, --name NAME  (Optional) (default=Anonymous) (string) Your name will be displayed on the image enabling mentors,
-                        professors, fellow students to be able to recognize your work. Credit is important!
+  -n NAME, --name NAME  (Optional) (default=Anonymous) (string) Your name will be displayed on the image enabling mentors, professors,
+                        fellow students to be able to recognize your work. Credit is important!
   -a ARCHIVES, --archives ARCHIVES
-                        (default=1)(string) This option currently offers access to the NVAS image archive. Selecting this option
-                        will return the top 5 results from NVAS (if exists). These can be downloaded as .imfits files
-  -k KIND, --kind KIND  (default='base64') choose from base64, plot, png, jpg to show base64 of resultant image, plot on output,
-                        save png/jpg files
+                        (default=1)(string) This option currently offers access to the NVAS image archive. Selecting this option will
+                        return the top 5 results from NVAS (if exists). These can be downloaded as .imfits files
+  -k KIND, --kind KIND  (default='base64') choose from base64, plot, png, jpg to show base64 of resultant image, plot on output, save
+                        png/jpg files
   -s SPIDX_FILE, --spidx_file SPIDX_FILE
                         (Default=None) enter path to spidx.fits file that contains spectral index data.
   -px PIXELS, --pixels PIXELS
                         (default=480) change pixel value for the final resulatant image.
   -A ANNOT, --annot ANNOT
                         (default=True) remove any annotation by setting this to False.
   -S FLUX_LIST, --flux_list FLUX_LIST
-                        (Optional) (Default=None) Takes input as list for spectral index calculation.
+                        (Optional)(list)(Default=None) Takes input as list for spectral index calculation.
   -S_e FLUX_ERROR, --flux_error FLUX_ERROR
-                        (Optional) (Default=None) Takes input as list for spectral index calculation.
+                        (Optional)(list)(Default=[0,0]) Takes input as list for spectral index calculation.
   -freq FREQ_LIST, --freq_list FREQ_LIST
                         (Optional) (Default=None) Takes input as list for spectral index calculation.
 ```

setup.cfg

@@ -1,6 +1,6 @@
 [metadata]
 name = rgbmaker
-version = 0.0.5.1.1
+version = 0.0.5.2
 author = Avinash Kumar
 author_email = [email protected]
 description = A python package which communicates to different astronomical services and fetches fits and numerical data.

setup.py

@@ -5,7 +5,7 @@
 
 setup(
     name = 'rgbmaker',
-    version = '0.0.5.1.1',
+    version = '0.0.5.2',
     url='https://github.com/avialxee/rgbmaker',
     author='Avinash Kumar',
     author_email='[email protected]',

src/rgbmaker/cli.py

@@ -13,14 +13,13 @@ def cli_ASCII():
        __/ |                                    
       |___/                                     
 
-
+A python package which communicates to different 
+astronomical services and fetches fits and numerical data
         """
         return ascii_rgbmaker
 
 
-parser = argparse.ArgumentParser('rgbmaker',description="""A python package which communicates to different 
-astronomical services and fetches fits and numerical data.
-""", formatter_class=argparse.RawDescriptionHelpFormatter)
+parser = argparse.ArgumentParser('rgbmaker',description=cli_ASCII(), formatter_class=argparse.RawDescriptionHelpFormatter)
 parser.add_argument('-p', '--position', type=str, help="""(Required)
         The object name or the coordinates of the object in the FK5 (J2000) system. 
         Ex: "14 09 48.86 -03 02 32.6", M87, NGC1243, without quotes.""")
@@ -54,6 +53,7 @@ def cli_ASCII():
 args=parser.parse_args()
 
 def cli():
+
     position=args.position or ""
     radius=args.radius or float(0.12)
     imagesopt=args.imagesopt or 2