AstroBin saves small pieces of text information (cookies) on your device in order to deliver better content and for statistical purposes. You can disable the usage of cookies by changing the settings of your browser. By browsing AstroBin without changing the browser settings, you grant us permission to store that information on your device.
I agreeImaging telescopes or lenses:C9.25
Imaging cameras:Moravian Instruments G3-16200 Mark II
Mounts:10 Micron GM1000 HPS
Guiding cameras:10Micron HPS System
Software:Main Sequence Software Seqence Generator Pro , Pixinsight
Filters:Baader Planetarium G 2" , Baader Planetarium R 2" , Baader Planetarium B 2" , Baader Planetarium Baader 1,25" L
Dates:April 15, 2020
Frames:
Baader Planetarium B 2": 15x300" bin 1x1
Baader Planetarium G 2": 13x300" bin 1x1
Baader Planetarium L 2": 61x300" bin 1x1
Baader Planetarium R 2": 13x300" -25C bin 1x1
Integration: 8.5 hours
Darks: ~30
Flats: ~20
Flat darks: ~20
Bias: ~50
Avg. Moon age: 22.66 days
Avg. Moon phase: 44.59%
Bortle Dark-Sky Scale: 7.00
Mean SQM: 18.70
Astrometry.net job: 3436142
RA center: 12h 18' 51"
DEC center: +14° 24' 25"
Pixel scale: 0.514 arcsec/pixel
Orientation: 270.374 degrees
Field radius: 0.366 degrees
Resolution: 4054x3151
Locations: Castenedolo, Castenedolo, Italy
Data source: Backyard
The main goals of this experiment were two:
1) verify if RGB imaging under a light polluted sky (Average SQM 18.5) is possible or not.
2) test the new procedure of gradient removal by Vicent Peris described here
Well
1) it is clearly possible if the target is bright; harder a fainter one.
2) it is a great technique much more superior than other gradient removal routines.
Description: Plate solved and annotated by Pixinsight
| Imagers of Italy |
| Moravian Users |
| PixInsight Addicts |
Comments