David's Astronomy Pages
Images - Session 586 (2015-05-02)

Objects Session Notes
Bullet Vega - A0V Star
Bullet P Cyg - Star
   
Bullet NGC 6118 - Spiral Galaxy
   
Bullet Photometric Monitoring - Variables
  - R CrB, CI Cyg, ER UMa

- RZ LMi attempt failed (due to star drift)
   
Bullet Astrometric Monitoring - Nearby Stars
  - Barnards Star
- Night session (1.5 hrs duration), aborted when cloud developed  
- Session operated under semi-automated control, with remote monitoring from indoors computer.  
- Ambient Temperature:  tube temperature fell to -2.5°C (minimum)
- CCD operation -30°C (at 63% average cooling). 
- Planned objectives of the session were to monitor selected variable stars & nearby stars and to take Spectral images.
-  

Vega - A0V Star

Vega Spectra Analysis

Vega - Seeing
Image 
CCD Image Animation (frames rotated, but not aligned, cropped)
0.11s exposure, 2x2 binning, Half Frame, SA 200 Filter
2015-05-02  00:27h UT (#586051-55)
12" LX200R  (at f/10.4) + ST-10XME
(Rotation S586: 184.5 deg)
Rotation S286 : 221 deg)
  
Vega - Raw Spectral Profiles
Comparison between 5 individual image profiles and stacked image profile
(profiles produced in RSpec)
Image 
  
Image
Profiles from CCD Images
Image details as above
  
  0.11s image (at / near saturation)
Image 
Stacked CCD Image
5 x 0.11s (aligned, rotated, cropped), 2x2 binning, Half Frame, SA 200 Filter
Image details as above
  
  0.2s image (effectively saturated)
Image 
Stacked CCD Image
5 x 0.2s (aligned, rotated, cropped), 2x2 binning, Half Frame, SA 200 Filter
2015-05-02  00:04h UT (#586017-21)
12" LX200R  (at f/10.4) + ST-10XME
  
Vega - Calibrated Spectral Profiles
Comparison between profiles from 0.11s and 0.2s image exposures
The Red Profile (0.2s) is noticeably flatter in higher intensity regions
of the profile due to saturation of CCD Pixels
  Image
CCD Image details as above
Red Line :  Vega.20150502.im586017-21.av5x0.2s.S
Blue Line :  Vega.20150502.im586051-55.5x0.11s.S
(Plot produced in RSpec)
 
  Spectral Image / Histogram Plots
Comparison between profiles from 0.11s and 0.2s image exposures
Plots both displayed with 50000-65535 ADU black-white range
Image 
Stacked CCD Image (5 x 0.11s)
Image details as above
  
Image 
Stacked CCD Image (5 x 0.2s)
Image details as above

Whilst the CCD image values are not reaching near the 65535 ADU mark, 
and represent the sum of 4 physical pixels at 1x1 binning,
they are photons are 'filling' the pixel bins at a very rapid rate.
and are being ? 'absorbed' into the silica of CCD chip somehow rather than being converted
into electron count when read.  This process whilst worse with 0.2s exposure,
is applying also to the shorter exposure 0.11s images
(NB. the shortest exposures possible with my ST-10E Camera is 0.11s/0.12s)

The following 90s CCD Image of NGC 6118 taken 6 minutes / 4 CCD reads
after the last Vega 0.11s spectral image still shows traces of Vega's first and zero order spectra.
Image 
CCD Image (cropped)
90s exposure (single frame), 3x3 binning, C Filter
2015-05-02 00:32 h UT (#586059)
12" LX200R  (at f/10.4) + ST-10XME
 
Calculated Instrument Response 
(IR = raw vega spectra / smoothed a0V library spectra
Image 
S586 profile produced using 0.11s exposures of Vega at Alt 50 deg (airmass 1.30)
S585 profile produced using 0.2s exposures of Vega at Alt 68 deg (airmass 1.07)
 
Vega - Corrected Spectral Profile
  Image
 
  Image
 
 
Image 
 
Vega - Normalised Spectra 
(corrected Vega profile / smoothed library a0V profile
Image 
 

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P Cyg -  Star

P Cyg (Lyra)    
     
     
CCD Spectra Image (Star Analyser 200)
(Image rotated & cropped)
5 x 5s exposure, 2x2 binning, S Filter
2015-04-21 03:38 h UT (#585280)
12" LX200R  (at f/10.4) + ST-10XME
Dispersion 25.44 A/px.
  CCD Spectra Image (150%)
Image details as left
     
P Cyg - Earlier Spectral Image (2008)   Spectral Emission Lines in P Cyg (Cygnus)
       
     
     

CCD Spectra Image (Star Analyser 100)
3 x 10s, 1x1 binning, 
2008-05-08 01:16hUT (#286177-79)
8" LX200 + ST-7e
Dispersion 33.6 A/px

  CCD Spectra Image (200%)
Image details as left
     
     
     

P Cyg Spectra Analysis

Profile:  0.2s, 2x2 binning, #585280 (calibrated on H alpha line & dispersion 25.44 A/px)
Reference: Example Raw Vega profile supplied with RSpec
 
Analysis made using RSpec
 

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NGC 6118 - Spiral Galaxy

NGC 6118 / Herschel II-402 (Serpens)
Image
CCD Image (cropped)
5 x 90s exposure (average combine), 3x3 binning, C Filter
2015-05-02 00:48 h UT (#586064-73)
12" LX200R  (at f/10.4) + ST-10XME
 
NGC 6118 / Herschel II-402 - Wider View
Image
CCD Image (50% size)
Image details as above

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