Difference: GlenCowanPhotmetry2019 (21 vs. 22)

Revision 2220 Feb 2020 - SamRyan

Line: 1 to 1
 
META TOPICPARENT name="StewartBoogertMSciProjects"

Major Project 2019-20

Photometry

HR Code

17/10/19

Start: 18:13

Took some Dark Frames at various temp and exposures

19:30 Andrey Abramov came to dome

Calibrated using Vega

problems with telescope syncranisation (dec reading -40deg) and Stelarium saying the telescope was in Paris

Vega was saturated at lowest exposure (0.001s)

Moved to a field of stars and focused on them

Then moved back to vega, was focused

Imaged an unknown binary

Finished at 22:44

Need to find out:

telescope position 'bug'

Link telescope to stelarium and guiding camera

20191017_final.zip

22/10/19

Observation 2 22/10/19

Meeting--24/10/19

Dark frame histograms taken at -5C

Histograms

mu_vs_t.pdf

λ = 0.055 0.022

μ = 953.22 0.37

29/10/19

Dark Frames taken at 10C

20191029.zip

04/11/19

Observation 04/11/19

Meeting--7/11/19

Meeting_071119.pdf

7/11/19

Observation 07/11/19

18/11/19

Observation 18/11/19

29/11/19

Observation 29/11/19

03/12/19

Observation 03/12/19

06/12/19

Manged to use Maxim_DL to aligne two images:

b100s_aligned.fit

g100s_aligned.fit

Also a 30 min dark frame exposure was taken to investigate the flux of cosmic rays on to the CCD chip

df30m.fit

13/12/19

Took some more 30 and 20 min dark frames to investiage possiable cosmic rays and decays.

As well as aligned two images of m29 taken at 40s from 29/11/19

20191212.zip

15/01/20

Observation 15/01/20

17/01/20

20200117.zip

m37_3sig.pdf

10/02/20

20200210.zip

11/02/20

20200211.zip

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20/02/20

20200220.zip

 

Comments


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