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Table 2.
NIR photometry of the local sequences for AT 2014ej in the “standard” system.
| ID | α(2000) | δ(2000) | Y | N | Jrc2 | N | H | N |
|---|---|---|---|---|---|---|---|---|
| 101 | 349.044870 | −42.571004 | 15.64(02) | 3 | 15.38(04) | 3 | 15.07(07) | 3 |
| 102 | 349.018801 | −42.593902 | 16.57(06) | 3 | 16.11(06) | 3 | 15.61(16) | 3 |
| 103 | 349.015365 | −42.595754 | 17.60(07) | 2 | ⋯ | ⋯ | ⋯ | ⋯ |
| 104 | 349.061355 | −42.592496 | 17.52(41) | 2 | 17.08(21) | 3 | 17.01(15) | 1 |
| 106 | 349.068255 | −42.572860 | 18.37(11) | 1 | ⋯ | ⋯ | ⋯ | ⋯ |
| 107 | 349.059690 | −42.570588 | 18.29(10) | 1 | ⋯ | ⋯ | ⋯ | ⋯ |
| 109 | 349.006081 | −42.561110 | 18.54(12) | 1 | ⋯ | ⋯ | ⋯ | ⋯ |
Notes. Uncertainties given in parentheses in thousandths of a magnitude correspond to an rms of the magnitudes obtained on photometric nights.
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