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Table 1.

VLTI/PIONIER observations of the target stars and the corresponding angular diameters obtained in this work.

Object J H Ks Night Configuration UD χ2 LDD χ2
[mag] [mag] [mag] [mas] [mas]
AG Peg 5.0 4.4 3.9 2012-08-13 A1-G1-I1-K0 1.023±0.009 0.745 1.062±0.009 0.744
FG Ser 5.9 4.9 4.4 2012-07-03 A1-G1-I1-K0 0.813±0.009 1.358 0.845±0.009 1.358
2012-08-13 A1-G1-I1-K0 0.941±0.015 0.206 0.978±0.016 0.206
2012-08-20 A1-I1-K0 0.892±0.011 0.548 0.927±0.012 0.549
2014-08-27 A1-G1-J3-K0 0.853±0.004 0.571 0.887±0.005 0.571
2014-09-22 A1-G1-J3-K0 0.857±0.002 0.439 0.891±0.002 0.438
2019-04-29 A0-D0-G1-J3 0.887±0.008 0.745 0.922±0.009 0.744
2019-05-02 A0-G1-J2-J3 0.885±0.004 0.252 0.920±0.004 0.252
2019-05-03 A0-G1-J2-J3 0.894±0.003 0.310 0.929±0.003 0.309
ER Del 6.2 5.3 5.0 2012-08-13 A1-G1-I1-K0 0.613±0.009 0.150 0.636±0.009 0.150
V1261 Ori 3.3 2.4 2.1 2012-03-02 A1-G1-I1-K0 2.292±0.003 0.531 2.383±0.003 0.533
RW Hya 5.7 4.9 4.6 2014-08-27 A1-G1-J3-K0 0.619±0.010 0.317 0.642±0.010 0.317
V399 Pav 6.7 5.8 5.4 2014-08-27 A1-G1-J3-K0 0.517±0.016 0.501 0.536±0.017 0.501
2014-10-06 A1-G1-J3-K0 0.493±0.031 0.581 0.511±0.033 0.581

Notes. Angular diameters are provided for both the uniform disk (UD) and limb-darkened disk (LDD) models. The infrared magnitudes for the analyzed stars shown in the Table are from 2MASS (Skrutskie et al. 2006).

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