Difference: PaulHallamMsciProject (7 vs. 8)

Revision 804 Dec 2013 - PaulHallam

Line: 1 to 1
 
META TOPICPARENT name="WebHome"
-- PaulHallam - 18 Oct 2013

Aims

Line: 9 to 9
 
  • Use Python to analyse these dark frames via Histogram plots and plots of column mean and standerd deviation, to determine if the pixels follow a Poisson distribution.
  • To compare my results regarding dark frames with Chris Haynes and Ryan Cheale's results.

List of Potential Targets

Deleted:
<
<
  • Gamma Cassiopeia - Variable Star (Gamma Cassiopeia Variable), magnitude variation 1.5 - 3.0, period Unknown, Good Visibility - Poor Choice
 
  • Delta Cephei - Variable Star (Cephid Variable), magnitude variation 3.5 - 4.4, period 5.4 day, Good Visibility
Changed:
<
<
  • Beta Persei - Variable Star (Algol Variable), magnitude variation 2.1 - 3.4, period 2.9 day, Good Visibility
>
>
  • Beta Persei - Variable Star (Algol Variable), magnitude variation 2.1 - 3.4, period 2.9 day, Good Visibility-> eclipsing binary - Not Good
 
  • Eta Aquila - Variable Star (Cephid Variable), magnitude variation 3.5 - 4.4, period 7.2 day, Poor Visibility
  • RR Lyrae - Variable Star (RR Lyrae Variable) magnitude variation 7.06 - 8.12, period 0.6 day, Good Visibilty
  • TU Cassiopeia - Variable Star (Cephid Variable) magnitude variation 6.88 - 8.18, period 2.14 day, Good Visibilty
Changed:
<
<
  • RZ CAssiopeia - Variable Star (Cephid Variable) magnitude variation 6.18 - 7.72, period 1.2 day, Good Visibilty
>
>
  • RZ Cassiopeia - Variable Star (Algol Variable) magnitude variation 6.18 - 7.72, period 1.2 day, Good Visibilty- > eclipsing binary - Not Good
 
  • AB Auriga - Variable Star (Tau Tauri Variable) magnitude variation 6.3 - 8.4, period 6.5 day (Eruptive - but period given by AAVSO), Good Visibilty,
  • W Gemini - Variable Star (Delta Cephei Variable) magnitude variation 6.54 - 7.38, period 7.9 day, Good Visibilty (although rises at 19:00),

Data and Logs

 
This site is powered by the TWiki collaboration platform Powered by PerlCopyright © 2008-2020 by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding RHUL Physics Department TWiki? Send feedback