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SUSI2Sky Brightness |
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The following table gives the sky brightness as measured at CTIO (near La Silla) as function of the phase of the Moon. The values are taken from a NOAO newsletter (Walker 1987).
Days from New Moon |
Sky brightness [mag/sq.arcsec] |
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U | B | V | R | I | |
0 | 22.0 | 22.7 | 21.8 | 20.9 | 19.9 |
3 | 21.5 | 22.4 | 21.7 | 20.8 | 19.9 |
7 | 19.9 | 21.6 | 21.4 | 20.6 | 19.7 |
10 | 18.5 | 20.7 | 20.7 | 20.3 | 19.5 |
14 | 17.0 | 19.5 | 20.0 | 19.9 | 19.2 |
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In the past, the NTT was affected by a problem of scattered light inside the dome, especially during bright Moon. This was greatly improved by painting the inside walls with a high diffusion paint in December 1999.
The sky brightness has been measured on all long (exp.time > 200s) images obtained with SuSI2 after September 2001. The sky was measured using an iterative sigma clipping median estimation. The figures below show the sky brightness as a function of position, and the table lists the median values. These values are in very good agreement with those from CTIO.
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V sky brightness (in adu/2x2pix/s) | R sky brightness (in adu/2x2pix/s) |
Filter | Median Sky Brightness | |
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[adu/(2x2bin)pix/sec] | mag/sq.arcsec | |
V | 1.8 |
21.67 |
R | 2.5 |
20.63 |
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Last modified: Thu Nov 06 2003 |
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