Table 1.
Instruments used in this study.
| Telescope | Instrument | Filters | Platescale | Field of view | Epoch Min./Max. | Ref. |
|---|---|---|---|---|---|---|
| [pixel−1] | ||||||
| CTIO (Blanco) | Flaugher+10 | g, r, i, z, y | 0 27 |
1.1° radius | 2014–2018 | (1) |
| KPNO (Mayall) | NEWFIRM | J, H, Ks | 0 4 |
28′ × 28′ | 2015 | (2) |
| CFHT | MegaCam | r, i | 0 18 |
1° × 1° | 2005–2015 | (3) |
| CFHT | WIRCam | y, J, H, Ks | 0 3 |
20′ × 20′ | 2007–2008 | (4) |
| CFHT | CFH12K | I, z | 0 21 |
42′ × 28′ | 1999–2002 | (5) |
| INT | WFC | u, v, b, β, y (Strömgren), U, B, V, Z, g, r, i(a) | 0 33 |
34′ × 34′ | 2000–2015 | (6) |
| UKIRT | WFCAM | J, Ks | 0 4 |
40′ × 40′(b) | 2006–2012 | (7) |
| LCO Swope | Direct CCD | i | 0 43 |
15′ × 14′ | 2013 | (8) |
| VST | OmegaCam | r | 0 21 |
1° × 1° | 2014 | (9) |
| ESO (2.2 m) | WFI | R, I(a) | 0 24 |
34′ × 33′ | 2002 | (10) |
| Subaru | HSC | y | 0 17 |
1.8° radius | 2015 | (11) |
| Palomar 48″ | PTF | g, r | 1 0 |
3 3 × 2 2 (c) |
2010–2012 | (12) |
| OMM (1.6 m) | CPAPIR | I, J, H | 0 89 |
30′ × 30′ | 2012–2015 | (13) |
Notes.
The chip layout has large gaps between detectors, and the coverage of the focal plane is only partial
References. (1) Flaugher et al. (2010); (2) Autry et al. (2003); (3) Boulade et al. (2003); (4) Thibault et al. (2003); (5) Cuillandre et al. (2000); (6) Ives (1998); (7) Casali et al. (2007); (8) Rheault et al. (2014); (10) Baade et al. (1999); (11) Miyazaki et al. (2018); (12) Rahmer et al. (2008); (13) Thibault et al. (2002).
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