Table 1
VLT/NACO observations.
Date-Obs | Filter | DIT | NDIT | EXPTIME | N frames | N used | t driz | Seeing | FWHM | NGS |
[s] | [s] | [min] | [′′] | [mas] | [mag] | |||||
|
||||||||||
Arches Field 1 | ||||||||||
|
||||||||||
2002-Mar-31 | K s | 0.5 | 8 | 4.0 | 10 | 10 | 0.7 | 0.8 | 84 | V = 16.3 |
2002-Mar-31 | K s | 15.0 | 4 | 60.0 | 20 | 7 | 7.0 | 0.8 | 84 | V = 16.3 |
2010-Aug-09 | K s | 10.0 | 2 | 20.0 | 40(80) | 11(22) | 3.7 | 0.7 | 130 | Ks = 10.4 |
2011-Mar-31 | K s | 3.0 | 23 | 69.0 | 31(713) | 27(621) | 31.0 | 0.8 | 108 | Ks = 10.4 |
2012-Jun-15 | L p | 0.2 | 57 | 11.4 | 91 | 67 | 12.73 | 0.6 | 162 | Ks = 10.4 |
|
||||||||||
Arches Field 2 | ||||||||||
|
||||||||||
2008-Jun-06 | K s | 15.0 | 2 | 30.0 | 40 | 38 | 19.0 | 0.7 | 87 | Ks = 9.2 |
2010-Aug-09 | K s | 10.0 | 2 | 20.0 | 40(80) | 36(72) | 12.0 | 0.7 | 122 | Ks = 9.2 |
2011-Sep-09 | L p | 0.175 | 170 | 29.75 | 22 | 22 | 10.9 | 0.9 | 122 | Ks = 9.2 |
|
||||||||||
Arches Field 3 | ||||||||||
|
||||||||||
2008-Jun-06 | K s | 15.0 | 2 | 30.0 | 40 | 32 | 16.0 | 0.8 | 108 | Ks = 9.8 |
2011-Sep-17 | K s | 3.0 | 23 | 69.0 | 20(460) | 10(224) | 11.2 | 0.9 | 157 | V = 16.0 |
2012-Jun-12 | K s | 3.0 | 20 | 60.0 | 20(400) | 19(381) | 19.0 | 0.8 | 87 | Ks = 9.8 |
2012-Aug-05 | L p | 0.175 | 170 | 29.75 | 22 | 22 | 10.9 | 1.2 | 145 | Ks = 9.8 |
|
||||||||||
Arches Field 4 | ||||||||||
|
||||||||||
2008-Jun-06 | K s | 15.0 | 2 | 30.0 | 40 | 33 | 16.5 | 0.9 | 87 | Ks = 10.4 |
2011-Sep-18 | K s | 6.0 | 11 | 66.0 | 20(220) | 20(220) | 22.0 | 0.7 | 81 | Ks = 10.4 |
2012-Jun-12 | K s | 3.0 | 20 | 60.0 | 20(400) | 17(339) | 17.0 | 0.9 | 108 | Ks = 10.4 |
2012-Jun-15 | L p | 0.2 | 58 | 11.6 | 40 | 31 | 6.0 | 0.9 | 122 | Ks = 10.4 |
|
||||||||||
Arches Field 5 | ||||||||||
|
||||||||||
2008-Jun-10 | K s | 15.0 | 2 | 30.0 | 40 | 29 | 14.5 | 0.8 | 135 | Ks = 10.3 |
2011-Sep-19 | K s | 3.0 | 23 | 69.0 | 20(460) | 15(352) | 17.6 | 0.6 | 135 | V = 16.1 |
2012-Jun-12 | K s | 3.0 | 20 | 60.0 | 20(400) | 16(319) | 16.0 | 0.8 | 92 | Ks = 10.3 |
2012-Jun-15 | L p | 0.2 | 58 | 11.6 | 40 | 40 | 7.7 | 1.0 | 122 | Ks = 10.3 |
|
||||||||||
Quintuplet Field 1 | ||||||||||
|
||||||||||
2003-Jul-22 | K s | 2.0 | 30 | 60.0 | 16 | 16 | 16.0 | 0.4 | 87 | Ks = 6.6 |
2003-Jul-22 | K s | 20.0 | 2 | 40.0 | 16 | 16 | 10.7 | 0.4 | 76 | Ks = 6.6 |
2008-Jul-24 | K s | 2.0 | 15 | 30.0 | 44 | 33 | 16.5 | 0.5 | 87 | Ks = 6.6 |
2009-Jun-17 | L p | 0.175 | 170 | 29.75 | 36 | 36 | 17.9 | 0.6 | 106 | Ks = 6.6 |
|
||||||||||
Quintuplet Field 2 | ||||||||||
|
||||||||||
2008-Jul-24 | K s | 2.0 | 15 | 30.0 | 47 | 34 | 17.0 | 0.5 | 70 | Ks = 7.3 |
2011-Sep-19 | K s | 2.0 | 30 | 60.0 | 22 | 13(397) | 13.2 | 0.9 | 108 | V = 16.2 |
2012-Jun-14 | K s | 2.0 | 30 | 60.0 | 38 | 30(901) | 30.0 | 0.9 | 119 | Ks = 7.3 |
2011-Sep-10 | L p | 0.175 | 170 | 29.75 | 21 | 21 | 10.4 | 1.2 | 108 | Ks = 7.3 |
|
||||||||||
Quintuplet Field 3 | ||||||||||
|
||||||||||
2008-Aug-25 | K s | 2.0 | 15 | 30.0 | 63 | 17 | 8.5 | 0.7 | 108 | Ks = 7.8 |
2009-Apr-07 | K s | 2.0 | 15 | 30.0 | 87 | 32 | 16.0 | 0.5 | 108 | Ks = 7.8 |
2012-Jun-14 | K s | 2.0 | 30 | 60.0 | 34 | 27(827) | 27.6 | 0.8 | 108 | Ks = 7.8 |
2011-Sep-11 | L p | 0.175 | 170 | 29.75 | 22 | 22 | 10.9 | 0.9 | 108 | Ks = 7.8 |
|
||||||||||
Quintuplet Field 4 | ||||||||||
|
||||||||||
2009-Apr-10 | K s | 2.0 | 15 | 30.0 | 44 | 32 | 16.0 | 0.5 | 81 | Ks = 7.1 |
2012-Jun-14 | K s | 2.0 | 30 | 60.0 | 20 | 17(515) | 17.2 | 0.9 | 108 | Ks = 7.1 |
2012-Jun-13 | L p | 0.2 | 66 | 13.2 | 63 | 20 | 4.4 | 1.5 | 154 | Ks = 7.1 |
|
||||||||||
Quintuplet Field 5 | ||||||||||
|
||||||||||
2009-Apr-10 | K s | 2.0 | 15 | 30.0 | 44 | 31 | 15.5 | 0.5 | 84 | Ks = 7.5 |
2012-Aug-02 | K s | 2.0 | 30 | 60.0 | 12 | 9(269) | 9.0 | 0.7 | 108 | Ks = 7.5 |
2012-Jun-13 | L p | 0.2 | 66 | 13.2 | 44 | 38 | 8.4 | 1.0 | 114 | Ks = 7.5 |
Notes. Seeing refers to the optical seeing measured with the DIMM facility at the time of observations. DIT: detector integration time, NDIT: number of DITs obtained per frame, EXPTIME: resulting exposure time per position, Nframes: number of images obtained, Nused: number of images with good quality, tdriz: total integration time in the final, drizzled image, FWHM: full width at half maximum of the PSF in milliarcseconds (mas), NGS: brightness of the natural guide star. The Arches 2002 data are described in detail in Stolte et al. (2002).
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