|
Preparing for a sky flat
Obtaining a Sky Flat
Below we show a series of images taken as
sunrise approached on 20010630. D(time) is the time the exposure was taken
after the first frame; sunrise occurred at D(time) = 12 minutes.
Note also that the telescope was AT ZENITH.
At the bottom of the page there is a plot of the count rate per
three-second exposure, in which the sharp increase in counts just
after sunrise can be clearly seen. Note: these data were taken
in NDSTARE with NORMAL Gain. Hi-Gain will give twice as many counts
per photon!
|
Run |
Image |
D (time) in minutes |
Mean Count
(in 3 sec) |
|
329 |

|
0 |
0 |
|
330 |

|
1 |
2 |
|
331 |

|
3 |
2 |
|
332 |

|
5 |
3 |
|
333 |

|
7 |
3 |
|
334 |

|
10 |
3 |
|
**335 |

|
12 (sunrise)** |
3 |
|
336 |

|
15 |
3.5 |
|
337 |

|
17 |
5 |
|
338 |

|
19 |
7 |
|
339 |

|
21 |
10 |
|
340 |

|
22 |
12 |
|
341 |

|
23 |
12 |
|
342 |

|
25 |
16 |
|
Sky counts through the F-P with an exposure time of 3 seconds
(F-P set for H2 1-0 S(1) imaging; NDStare + Normal readout).
The
x-axis records the time in minutes; note that Sunrise occurred at
D(time) = 12 minutes. The y-axis is the
counts measured in 3 seconds. Consequently, a 30 second exposure time
would have given 10-times as many counts on the array. |

|
And Finally...
A recent observer had the following experience while taking a sky-flat
at sunrise:
"We did our skyflat yesterday morning with the telescope 3 hrs over
pointing towards the sunrise and got just the right counts
(1000-2000) in 60 sec by starting the sequence right at sunrise (this
was by accident as we were planning to do it 12 minutes after sunrise
but just as well we didn't; just noticed that your webpage does
actually say with telescope at zentih). Tried it just now
with telescope 3hrs to west at sunset. We started it a few minutes
before sunset but it was too late really (300-1000) counts. With
telescope in that position need to start it 5 mins before sunset I
reckon."
|