Table 1.
Instruments used in this study.
| Telescope | Instrument | Type | Platescale | Ref. |
|---|---|---|---|---|
| [pixel−1] | ||||
| CTIO Blanco | DECam | CCD | 0 26 |
(1) |
| CTIO Blanco | MOSAIC2 | CCD | 0 26 |
(2) |
| KPNO Mayall | MOSAIC1 | CCD | 0 26 |
(2) |
| KPNO Mayall | NEWFIRM | IR | 0 4 |
(3) |
| CFHT | MegaCam | CCD | 0 18 |
(4) |
| CFHT | CFH12K | CCD | 0 21 |
(5) |
| CFHT | UH8K | CCD | 0 21 |
(6) |
| INT | WFC | CCD | 0 33 |
(7) |
| UKIRT | WFCAM | IR | 0 4 |
(8) |
| LCO Swope | Direct CCD | CCD | 0 43 |
(9) |
| VST | OmegaCam | CCD | 0 21 |
(10) |
| Subaru | HSC | CCD | 0 17 |
(11) |
| VISTA | VIRCAM | IR | 0 34 |
(12) |
References. (1) Flaugher et al. (2010); (2) Wolfe et al. (2000); (3) Autry et al. (2003); (4) Boulade et al. (2003); (5) Cuillandre et al. (2000); (6) Metzger et al. (1995); (7) Ives (1998); (8) Casali et al. (2007); (9) Rheault et al. (2014); (10) Kuijken et al. (2002); (11) Miyazaki et al. (2018); (12) Dalton et al. (2006).
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