Difference: Gaia16aye (1 vs. 2)

Revision 22016-12-17 - ChowChoongNgeow

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

Follow-up Gaia16aye

Line: 13 to 13
 

Date Telescope Bands
Changed:
<
<
2016 November 18t 40cm BVgriz
2016 November 19 40cm BVgriz
2016 November 20 40cm BVgriz
2016 November 21 40cm BVgriz
2016 November 22 40cm BVgriz
2016 November 23 40cm BVgriz
2016 November 24 40cm BVgriz
2016 November 25 40cm BVgriz
2016 November 26 40cm BVgriz
2016 November 27 40cm BVgriz
2016 November 28 40cm BVgriz
>
>
2016 November 19 40cm gri
(The observation was planned for Nov 18 to 24, unfortunately other nights were weathered out, and we only obtained data on Nov 19, uploaded to CPCS).
  and:

Revision 12016-12-14 - NadiaBlagorodnova

Line: 1 to 1
Added:
>
>
META TOPICPARENT name="CoordinatedFollowup"

Follow-up Gaia16aye

The Gaia16aye has been followed-up spectroscopically by:

Date Telescope
2016 November 21st 2m HCT
2016 November 24th 2m HCT

And photometrically by:

Date Telescope Bands
2016 November 18t 40cm BVgriz
2016 November 19 40cm BVgriz
2016 November 20 40cm BVgriz
2016 November 21 40cm BVgriz
2016 November 22 40cm BVgriz
2016 November 23 40cm BVgriz
2016 November 24 40cm BVgriz
2016 November 25 40cm BVgriz
2016 November 26 40cm BVgriz
2016 November 27 40cm BVgriz
2016 November 28 40cm BVgriz

and:

Date Telescope Bands
2016 November ? 50cm in Japan g,R,I
2016 November ? 50cm in Japan g,R,I

The photometry has been uploaded to the Cambridge photometric calibration server: https://www.ast.cam.ac.uk/ioa/wikis/gsawgwiki/index.php/Calibration_Server

-- NadiaBlagorodnova - 14 Dec 2016

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