Session
Displayed is the area of sky where the scope is currently pointed :
Sky Map

All Sky Cam
Devices
The current status of the devices used to capture the images are shown below. Hover your mouse over rows in the Status column to view more info about the state of the device.
Attached Devices
DEVICE | STATUS | INFO | POWER |
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Power Box
Sensors | Consumption | Dew |
---|---|---|
|
|
|
Name | Version | Date |
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Last updated: Not Available
Image
The last successfully captured sub should be displayed below along with data from the FITS header :
Observation Date | Invalid Date |
---|---|
Object | Not Available |
Object (RA, Dec) | Not Available |
Object RA (hms) | Noth Availablem undefineds |
Object Dec (dms) | Not° Available' undefined" |
Object Altitude (°) | Not Available |
SQM (mag./arc sec2) | |
Average AirMass | Not Available |
Humidity (%) | Not Available |
Dew Point (°C) | Not Available |
Ambient Temp (°C) | Not Available |
Sensor Angle (°) | Not Available |
Sensor Setpoint (°C) | Not Available |
Sensor Binning | Not Available |
arc sec/pixel | Not Available |
Focal Length (mm) | Not Available |
Filter | Not Available |
Exposure (secs) | Not Available |
Profile | Not Available |
Creator | Not Available |
Annotated
The last successfully plate solved and annotated version should be displayed below.
Conditions
Reading | Not Available |
---|---|
MSAS | Not Available |
Max MSAS | Not Available |
Max NELM | Not Available |
Max Bortle | Not Available |
Weather
About
This project aims to show the state and image capture of the current or last astroimaging session. The data capture and processing was performed by GingerGeeks and the web based front end was created in cooperation with Neil Munday.

The following software is used locally to capture, process and format the raw astrophotography data :
The following Python modules are used for processing, communication and transfer of data :
The following software is used to create the interface on the public web server :