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Table 1

GTC/OSIRIS astrometry, photometry (or 3σ lower limits), observing information, and photometry for six Y dwarfs and a T9 + Y0 binary.

WISE J...(SpT) RA Dec z Date ExpT J H z − J μα   cosδ μ δ

hh:mm:ss.sss °:′:′′ mag dd/mm/yy s mag mag

0146 + 4234 (Y0) 01:46:56.576  + 42:34:09.80 24.10  ±  0.13 03/09/12 50  ×  50 19.40  ±  0.25 18.71  ±  0.24 5.39  ±  0.27  −0.52  ±  0.08  −0.11  ±  0.08
0410 + 1502 (Y0) 04:10:22.933  + 15:02:42.91 22.66  ±  0.09 15/09/12 40  ×  50 19.44  ±  0.03 20.02  ±  0.05 3.22  ±  0.09  + 1.20  ±  0.08  −2.17  ±  0.08
1405 + 5534 (Y0p)  >23.85 06/08/12 45  ×  50 21.06  ±  0.06 21.41  ±  0.08  >2.79
1738 + 2732 (Y0)a 17:38:35.585  + 27:32:58.28 22.80  ±  0.09 17/06/12 30  ×  50 20.05  ±  0.09 20.45  ±  0.09 2.75  ±  0.13  + 0.32  ±  0.10  −0.39  ±  0.10
1828 + 2650 (≥Y2)  >24.46 09/09/12 40  ×  50 23.48  ±  0.23 22.85  ±  0.24  >0.98
2056 + 1459 (Y0) 20:56:29.028  + 14:59:54.64 23.09  ±  0.08 15/06/12 40  ×  50 19.94  ±  0.04 19.96  ±  0.04 3.66  ±  0.09  + 0.89  ±  0.10  + 0.61  ±  0.10
1217 + 1626 (T9+Y0) 12:17:57.144  + 16:26:35.99 21.60  ±  0.03 15/12/12 15  ×  60 17.83  ±  0.02 18.18  ±  0.05 3.77  ±  0.04  + 1.41  ±  0.10  −1.96  ±  0.10

Notes. The near-infrared photometry is taken from Leggett et al. (2013), except for the H-band magnitude of WISEJ1828 + 2650 (Kirkpatrick et al. 2012).

(a)

We also targeted this object in the i band with OSIRIS. We measured a 3σ lower limit of i > 25.3 mag, translating into i − z > 2.4 mag and i − J > 5.8 mag.

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