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ERRATUM: "INFRARED DIAGNOSTICS FOR THE EXTENDED 12 μm SAMPLE OF SEYFERTS" (2010, ApJ, 710, 289)

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Published 2010 March 24 © 2010. The American Astronomical Society. All rights reserved.
, , Citation Stefi A. Baum et al 2010 ApJ 713 708 DOI 10.1088/0004-637X/713/1/708

0004-637X/713/1/708

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Due to an error at the publisher's end, the values of Rows 1–13 of Columns 3 and 4 of Table 10 were not printed. Also, the units of "μm" in Rows 2–13 of Column 2 were incorrectly represented as "m." The correct version of the table appears below. IOP Publishing sincerely regrets this error.

Table 10. Tests for Correlations in Seyfert Properties

First Property Second Property z p(%)
(1) (2) (3) (4)
EW(PAH 6.2 μm) Distance −2.058 4.0
EW(PAH 6.2 μm) Sil 10 μm −2.311 2.1
EW(PAH 6.2 μm) α(20–30 μm) 7.691 <0.1
EW(PAH 6.2 μm) α(55–90 μm) 5.663 <0.1
EW(PAH 6.2 μm) EW(H2 S(1) λ17 μm) 4.888 <0.1
EW(PAH 6.2 μm) EW(Ne v λ14 μm) 2.220 2.6
EW(PAH 6.2 μm) log L(Ne v λ14 μm) −0.668 50.4
PAH 6.2 μm Flux Ne v λ14 μm Flux 1.933 5.3
log L(PAH 6.2 μm) log L(Ne v λ14 μm) 4.205 <0.1
PAH 6.2 μm Flux H2 S(1) λ17 μm Flux 4.969 <0.1
log L(PAH 6.2 μm) log L(H2 S(1) λ17 μm) 5.333 <0.1
log L(PAH 6.2 μm) α(20–30 μm) 2.671 0.8
log L(PAH 6.2 μm) α(55–90 μm) 1.370 17.1
PAH 6.2 μm Flux IRAS Sν(60 μm) 7.260 <0.1
log L(PAH 6.2 μm) IRAS log νLν(60 μm) 7.491 <0.1
PAH 6.2 μm Flux O iv λ26 μm Flux 1.029 30.3
log L(PAH 6.2 μm) log L(O iv λ26 μm) 2.744 0.6
α(20–30 μm) α(55–90 μm) 4.288 <0.1
α(20–30 μm) EW(H2 S(1) λ17 μm) 4.292 <0.1
α(20–30 μm) IRAS log νLν(60 μm) 2.788 0.5
α(20–30 μm) EW(Ne v λ14 μm) 2.933 0.3
α(20–30 μm) log L(Ne v λ14 μm) −0.317 75.2
α(20–30 μm) log L(S iii λ18 μm) 2.861 0.4
α(20–30 μm) Sil 10 μm −4.674 <0.1
Sν(6.7 μm) Ne v λ14 μm Flux 3.228 0.1
log νLν(6.7 μm) log L(Ne v λ14 μm) 5.136 <0.1
Sν(6.7 μm) PAH 6.2 μm Flux −0.690 49.0
log νLν(6.7 μm) log L(PAH 6.2 μm) 2.884 0.4
EW(Ne v λ14 μm) Sil 10 μm −2.997 0.3
Ne v λ14 μm Flux Sν(8.4 GHz) 3.118 0.2
log L(Ne v λ14 μm) log νLν(8.4 GHz) 4.371 <0.1
Ne v λ14 μm Flux IRAS Sν(60 μm) 2.724 0.6
log L(Ne v λ14 μm) IRAS log νLν(60 μm) 4.808 <0.1
log L(Ne v λ14 μm) Sil 10 μm −0.410 68.1
Ne v 14 μm/24 μm S iii 18 μm/33 μm −0.171 86.4
Ne v 14 μm/24 μm Sil 10 μm −0.914 36.1
PAH 6.2 μm/11.3 μm log L(Ne v λ14 μm) 0.501 61.7
PAH 6.2 μm/11.3 μm Sil 10 μm −0.006 99.5
X-ray Flux (2−10 keV) Ne v λ14 μm Flux 1.685 9.2
O iii Flux Ne v λ14 μm Flux 1.811 7.0
Ne v 14 μm/[Ne ii] EW(PAH 6.2 μm) −5.261 <0.1
O iii/Ne v (14 μm) Sil 10 μm 4.197 <0.1
O iii/O iv (26 μm) Sil 10 μm 4.121 <0.1
log L(O iv λ26 μm) log L(O iii) 4.847 <0.1
O iv λ26 μm Flux O iii Flux 2.564 1.0
log L(Ne v λ14 μm) log L(O iii) 4.655 <0.1
Ne v λ14 μm Flux O iii Flux 1.811 7.0
log L(Ne v λ14 μm) Sil 10 μm −0.410 68.1
NH (cm−2) Sil 10 μm −2.372 1.8

Notes. The results of non-parametric rank tests to look for correlations among the properties of the combined sample. Columns 1 and 2: properties tested for correlation. Column 3: Kendall's generalized rank correlation coefficient, adjusted to account for upper and lower limits. Reported is the z-score, following the method outlined by Isobe et al. (1986). Column 4: two-sided significance, giving the probability of no correlation; small values (p < 1%) indicate evidence for correlation.

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10.1088/0004-637X/713/1/708