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MOST Guide Star Photometry

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Presentation on theme: "MOST Guide Star Photometry"— Presentation transcript:

1 MOST Guide Star Photometry
Overview, Statistical Analysis by Rainer Kuschnig & the MOST Team COROT WEEK June – Nice

2 MOST Photometry Sources
Science CCD Star Tracker CCD open field direct imaging micro Lens Array Fabry target Direct imaging targets Guide stars COROT WEEK June – Nice

3 MOST Guide Star Photometry
up to 20 guide stars per field the magnitude range exposure time is 1.5 sec no images are recovered brightest guide stars -> 30ppm COROT WEEK June – Nice

4 MOST Guide Star Photometry COROT WEEK 10 - 5-9 June 2006 – Nice
1.5 sec exposure calculate background apply threshold Sigexp = S (Ipix > backgr+threshold) Sigtot = S N*Sigexp -> stored in the science data stream N = integer (target sampling time / guide Star exposure Time) COROT WEEK June – Nice

5 MOST Guide Stars – Performance
COROT WEEK June – Nice

6 MOST Guide Stars – NOISE
COROT WEEK June – Nice

7 MOST Guide Stars - Stats
Total number of 263 – Feb 2006 time base: 7 to 47 days COROT WEEK June – Nice

8 MOST Guide Stars – Locations
typically field stars clusters: NGC2264,NGC2244 dense fields: WR123,WR103 COROT WEEK June – Nice

9 COROT WEEK 10 - 5-9 June 2006 – Nice
MOST Guide Stars – NGC2264 COROT WEEK June – Nice

10 COROT WEEK 10 - 5-9 June 2006 – Nice

11 COROT WEEK 10 - 5-9 June 2006 – Nice

12 COROT WEEK 10 - 5-9 June 2006 – Nice
MOST Guide Stars – Variables 3 eclipsing binaries 3 gam Dor 2 K puls 3 rotational variables 7 SPB(e,sg,classical) 12 LPVs 10 del Scuti ~15 to be finally classified …….. to be continued …… COROT WEEK June – Nice


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