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Table 5.

Reshifted absorber at z = 0.09017.

Parameter SIMULT. FIT RGS1 1st RGS1 2nd RGS2 2nd LETG ACIS LETG HRC MEG ACIS
Ne IX
log NNeIX(cm−2) < 15.8 < 15.6 < 15.9
WHeα (mÅ) 2.7 ± 0.9 3.4 ± 1.8
σ 2.9 1.8 1.4 1.4
c-stat/d.o.f 3691/3451 642/557 266/220 231/197 548/539 546/539 1434/1379

O VIII
log NOVIII(cm−2) 15.5 ± 0.2 n/a n/a < 15.6
WLyα (mÅ) 4.3 ± 1.6 n/a n/a
σ 2.6 2.1 n/a n/a 1.3 1.5 -
c-stat/d.o.f 3178/3026 641/557 n/a n/a 549/539 544/539 1436/1379

O VII
log NOVII(cm−2) < 15.5 (a)
WHeα (mÅ) < 8.6 (a)
c-stat/d.o.f 3146/2982

CIE
kT (keV) 0.26 ± 0.03
NH (Z/Z × 1019 cm−2)
log NNeIX(cm−2) 14.9 ± 0.2
log NOVIII(cm−2) 15.4 ± 0.2
log NOVII(cm−2) 14.8 ± 0.2
log NOVI(cm−2) 12.2 ± 0.2
c-stat/d.o.f 5156/4850

Notes. Spectral modeling of the z = 0.09017 X-ray absorber. The results of the “slab” modeling of Ne IX (λ0 = 13.447 Å), O VIII (blend at λ0 ≈ 18.97 Å) and O VII (λ0 = 21.602 Å) are shown in the three uppermost panels; The rest-frame line equivalent widths of the most important absorption lines are denoted by W, while the σ refers to the statistical detection significance level of the ion as yielded by the slab modeling. The first column reports the results obtained from a simultaneous fit to the individual, co-added data sets, whereas the last 6 columns list the results when these co-added data sets are modeled separately. 1σ upper limits for “slab” column densities are quoted if the line was not detected in individual spectra. The z = 0.09017 CIE modeling results are listed in the bottom panel. The n/a refers to zero effective area around the wavelengths of interest. The RGS2 first-order data was not included in the fits as it misses the data around the wavelengths of all the examined line features. All the quoted uncertainties correspond to 1σ confidence levels.

(a)

Due to the spectral line blending with Galactic O I lines, the O VII upper limits were derived excluding the band of the O VII Heα line.

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