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Table 1.

Optical photometry of the local sequence for AT 2014ej in the “standard” system.

ID α(2000) δ(2000) B V u g r i
1 349.073883 −42.532539
2 349.146027 −42.515438
3 348.886597 −42.615513 14.807(010) 14.145(007) 15.940(034) 14.434(007) 13.949(005) 13.805(007)
4 349.104828 −42.476219 15.332(013) 14.847(011) 16.056(036) 15.053(009) 14.713(007) 14.605(011)
5 348.940552 −42.641197 15.983(037) 15.050(030) 17.578(091) 15.504(031) 14.689(029) 14.316(014)
6 349.160797 −42.579163 15.729(022) 15.144(010) 16.608(051) 15.402(011) 14.974(008) 14.828(007)
7 349.018341 −42.487396 15.825(007) 15.114(011) 16.957(050) 15.434(012) 14.883(008) 14.683(010)
8 349.177582 −42.494061 16.206(039) 15.209(009) 18.097(048) 15.689(015) 14.782(010) 14.447(009)
9 349.201538 −42.602962 15.843(024) 15.269(010) 16.636(050) 15.515(009) 15.114(009) 14.967(011)
10 348.887085 −42.535305 16.070(021) 15.241(010) 17.454(089) 15.626(013) 14.936(008) 14.675(008)
11 349.011200 −42.468658 15.985(017) 15.422(008) 16.833(051) 15.671(012) 15.273(011) 15.141(012)
12 348.950928 −42.493233 16.349(015) 15.528(011) 17.800(063) 15.903(011) 15.248(013) 15.027(011)
13 349.079193 −42.577908 16.528(029) 15.614(012) 17.847(229) 16.049(013) 15.289(008) 14.948(010)
14 348.948059 −42.539196 16.196(030) 15.621(013) 17.028(082) 15.875(015) 15.465(016) 15.316(011)
15 349.177124 −42.531296 16.463(027) 15.645(015) 17.914(059) 16.018(015) 15.356(012) 15.141(009)
16 349.107941 −42.547867 16.849(022) 16.196(028) 17.786(073) 16.488(034) 15.999(016) 15.842(022)
17 349.041046 −42.637428 18.129(070) 17.004(051) 19.990(061) 17.570(043) 16.477(030) 16.051(021)
18 349.142731 −42.624664 17.243(031) 16.379(035) 18.671(075) 16.785(021) 16.065(016) 15.824(018)
19 349.086792 −42.654221 17.109(047) 16.521(032) 17.911(083) 16.773(014) 16.358(019) 16.216(036)
20 349.004547 −42.548927 17.406(080) 16.513(033) 18.663(085) 16.931(037) 16.227(014) 15.914(024)
21 349.021851 −42.545380 17.152(040) 16.558(030) 17.871(092) 16.843(046) 16.377(019) 16.174(017)
22 349.063202 −42.463596 17.234(067) 16.593(036) 18.179(051) 16.868(033) 16.405(032) 16.243(030)
23 349.155212 −42.636612 17.182(050) 16.607(023) 17.946(056) 16.847(031) 16.477(013) 16.358(019)
24 348.945343 −42.460548 17.043(035) 16.618(040) 17.523(170) 16.811(024) 16.502(037) 16.415(061)
25 349.102997 −42.480492 17.794(058) 16.606(041) 19.879(052) 17.199(042) 16.088(015) 15.623(015)
26 349.023193 −42.670746 17.517(080) 16.726(046) 18.875(074) 17.077(049) 16.433(016) 16.205(022)
27 349.009583 −42.517628 17.768(078) 16.937(036) 19.021(070) 17.327(021) 16.621(039) 16.345(027)
28 348.988068 −42.467167 17.582(100) 16.962(035) 18.510(044) 17.236(044) 16.762(023) 16.626(037)

Notes. Values in parenthesis are 1-σ uncertainties that correspond to the rms of the instrumental errors of the photometry obtained over a minimum of three nights observed relative to standard star fields.

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