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Table 3

Distances and absolute magnitudes for the LMC Cepheids calculated using the precepts given in Paper I, using the new p-factor relation.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14) (15) (16)
ID log (P) d σ(d) (m − M)0 σ (m − M) MV    MI    MJ    MH    MK    WVI    WJK    E(B − V) Δφ Δ(m − M)
(kpc) (kpc) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag) (mag)
HV 12199 0.421469 49.7 1.8 18.48 0.08  −2.41  −3.01  −3.13  −3.80  −3.94  −4.26 0.060 0.035  −0.058
HV 12203 0.470427 53.4 2.1 18.64 0.09  −2.71  −3.31  −3.66  −4.08  −4.24  −4.37 0.060 0.050  −0.058
HV 12202 0.491519 47.8 1.7 18.40 0.08  −2.53  −3.14  −3.60  −4.02  −4.09  −4.30 0.060 0.030  −0.058
HV 12197 0.497456 46.1 1.3 18.32 0.06  −2.42  −3.07  −3.44  −3.87  −4.07  −4.17 0.060  −0.015  −0.057
HV 12204 0.536402 45.6 1.0 18.30 0.05  −2.79  −3.33  −3.67  −4.07  −4.17  −4.34 0.060 0.015  −0.059
HV 12198 0.546887 47.5 0.7 18.38 0.03  −2.63  −3.27  −3.69  −4.09  −4.26  −4.36 0.060 0.020  −0.059
HV 6093 0.679885 47.2 1.4 18.37 0.06  −3.25  −3.86  −4.21  −4.60  −4.79  −4.87 0.058  −0.015  −0.048
HV 914 0.837489 57.6 1.1 18.80 0.04  −4.10  −4.79  −5.18  −5.54  −5.59  −5.84  −5.88 0.070  −0.035 0.013
HV 2405 0.840331 39.5 0.9 17.98 0.05  −3.06  −3.77  −4.14  −4.52  −4.57  −4.86  −4.86 0.070  −0.015 0.046
HV 12452 0.941457 45.9 1.9 18.31 0.09  −3.74  −4.48  −4.94  −5.32  −5.37  −5.62  −5.67 0.058 0.030 0.058
HV 12717 0.946628 42.9 2.0 18.16 0.10  −3.62  −4.33  −4.77  −5.14  −5.21  −5.42  −5.51 0.058  −0.005 0.065
HV 12816 0.959466 52.0 2.3 18.58 0.09  −4.29  −4.88  −5.24  −5.56  −5.62  −5.79  −5.88 0.070 0.015  −0.075
HV 2527 1.112251 55.8 1.3 18.73 0.05  −4.36  −5.21  −5.66  −6.09  −6.15  −6.51  −6.49 0.070 0.005 0.041
HV 2538 1.142118 51.2 1.3 18.55 0.06  −4.39  −5.28  −5.70  −6.14  −6.19  −6.64  −6.53 0.100  −0.040  −0.019
HV 5655 1.152657 60.7 1.7 18.91 0.06  −4.69  −5.53  −5.96  −6.41  −6.47  −6.84  −6.81 0.100  −0.015 0.046
HV 1006 1.152786 44.1 2.0 18.22 0.10  −4.17  −4.95  −5.48  −5.90  −5.95  −6.15  −6.28 0.100 0.005  −0.010
HV 12505 1.158115 53.9 0.8 18.66 0.03  −4.14  −5.04  −5.63  −6.11  −6.17  −6.43  −6.55 0.100  −0.005 0.031
HV 2282 1.166636 48.2 0.9 18.42 0.04  −4.41  −5.19  −5.66  −6.07  −6.12  −6.38  −6.44 0.100 0.015 0.051
HV 2549 1.210289 41.8 1.3 18.10 0.07  −4.50  −5.31  −5.69  −6.06  −6.13  −6.56  −6.43 0.058 0.020 0.052
HV 1005 1.272209 49.9 0.9 18.49 0.04  −4.72  −5.47  −5.98  −6.41  −6.45  −6.62  −6.77 0.100 0.015  −0.023
U1 1.353098 52.8 0.6 18.61 0.02  −4.82  −5.70  −6.28  −6.74  −6.80  −7.07  −7.16 0.100 0.010 0.060
HV 876 1.356342 47.6 0.5 18.39 0.02  −5.06  −5.86  −6.27  −6.67  −6.71  −7.10  −7.02 0.100 0.005 0.005
HV 878 1.367445 49.2 1.1 18.46 0.05  −5.11  −5.66  −6.35  −6.75  −6.80  −6.52  −7.12 0.058  −0.010 0.055
HV 12815 1.416910 46.5 0.8 18.34 0.04  −5.08  −5.96  −6.48  −6.94  −6.99  −7.32  −7.35 0.070  −0.030  −0.075
HV 1023 1.424235 46.3 0.7 18.33 0.03  −4.77  −6.28  −6.75  −6.79  −7.15 0.070 0.025  −0.049
HV 899 1.492039 56.2 0.4 18.75 0.01  −5.71  −6.52  −7.02  −7.45  −7.50  −7.78  −7.82 0.110 0.025 0.018
HV 873 1.537311 49.7 1.2 18.48 0.05  −5.87  −7.08  −7.46  −7.50  −7.79 0.130  −0.010 0.080
HV 881 1.552820 51.2 2.5 18.55 0.10  −5.55  −6.97  −7.41  −7.50  −7.85 0.030  −0.065 0.062
HV 879 1.566167 48.9 1.0 18.45 0.05  −5.27  −6.25  −6.84  −7.32  −7.39  −7.75  −7.78 0.060 0.015 0.044
HV 909 1.574986 46.1 0.8 18.32 0.04  −5.75  −6.52  −6.97  −7.36  −7.43  −7.70  −7.74 0.058  −0.065 0.048
HV 2257 1.595153 55.6 0.8 18.73 0.03  −5.90  −6.80  −7.35  −7.81  −7.87  −8.19  −8.22 0.060  −0.005 0.054
HV 2338 1.625350 51.8 0.5 18.57 0.02  −5.95  −6.83  −7.36  −7.80  −7.86  −8.19  −8.21 0.040  −0.015 0.070
HV 877 1.655215 44.2 0.3 18.23 0.02  −5.21  −6.80  −7.31  −7.36  −7.74 0.100 0.070 0.017
HV 900 1.675637 60.0 2.0 18.89 0.07  −6.32  −7.72  −8.17  −8.25  −8.62 0.058  −0.060 0.042
HV 2369 1.684646 47.5 1.6 18.39 0.07  −6.02  −7.46  −7.90  −7.96  −8.29 0.095 0.005  −0.029
HV 2827 1.896354 44.3 1.4 18.23 0.07  −6.18  −7.20  −7.81  −8.29  −8.36  −8.75  −8.73 0.080 0.035  −0.079

Notes. In Cols. 3 and 4 we give the IRSB distance and the associated error estimate. In Cols. 5 and 6 follows the distance modulus, and in Cols. 7 through 13, we give the absolute magnitudes in the different bands as well as the Wesenheits indices. Finally in Col. 14 we give the adopted reddening and in Col. 15 the adopted phase shift between spectroscopic and photometric angular diameters. Column 16 gives the magnitude correction to refer the distance moduli to the LMC barycenter.

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