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Table 2.

Details of the content of the 1OUSXB table in FITS format.

Column Format Units Description
Blazar name 18A Blazar name as it appears in Table 1
or in the 5BZCAT, 3LAC, or 3HSP catalogue
Source name 22A Catalogue source name formatted as 1OUSXBJhhmm.f+/−ddmm
hhmm = hours, min of RA, f = fraction of minutes
ddmm = deg and min of Dec
Other_name 22A Alternative source name from the literature when available
RA D deg Right Ascension in degrees (J2000.0 epoch)
Dec D deg Declination in degrees (J2000.0 epoch)
MJD_Start D days Modified Julian Day of observation start time
MJD_End D days Modified Julian Day of observation end time
Exposure_time D s Vignetting-corrected exposure time (a)
Ctr_03_10 D cts s−1 Count rate in the full (0.3–10.0 keV) band
Ctr_03_10_error D cts s−1 1σ error on Ctr_03_10
Ctr_03_1 D cts s−1 Count rate in the soft (0.3–1.0 keV) band
Ctr_03_1_error D cts s−1 1σ error on Ctr_03_1
Ctr_03_1_UL D cts s−1 3σ upper limit (b) on Ctr_03_1
Ctr_1_2 D cts s−1 Count rate in the medium (1.0–2.0) keV band
Ctr_1_2_error D cts s−1 1σ error on Ctr_1_2
Ctr_1_2_UL D cts s−1 3σ upper limit (b) on Ctr_1_2
Ctr_2_10 D cts s−1 Count rate in the hard (2.0–10.0 keV) band
Ctr_2_10_error D cts s−1 1σ error on Ctr_2_10
Ctr_2_10_UL D cts s−1 3σ upper limit (b) on Ctr_2_10
Flux_03_10 D erg cm−2 s−1 Observed energy flux in the full band
Flux_03_10_error D erg cm−2 s−1 1σ error on Flux_03_10
Flux_03_1 D erg cm−2 s−1 Observed energy flux in the soft band
Flux_03_1_error D erg cm−2 s−1 1σ error on Flux_03_1
Flux_03_1_UL D erg cm−2 s−1 3σ upper limit (b) on Flux_03_1
Flux_1_2 D erg cm−2 s−1 Observed energy flux in the medium band
Flux_1_2_error D erg cm−2 s−1 1σ error on Flux_1_2
Flux_1_2_UL D erg cm−2 s−1 3σ upper limit (b) on Flux_1_2
Flux_2_10 D erg cm−2 s−1 Observed energy flux in the hard band
Flux_2_10_error D erg cm−2 s−1 1σ error on Flux_2_10
Flux_2_10_UL D erg cm−2 s−1 3σ upper limit (b) on Flux_2_10
Nufnu_3.0keV D erg cm−2 s−1 Absorption-corrected (c)νf(ν) flux at 3.0 keV calculated from Ctr_03_10
Nufnu_3.0 keV_error D erg cm−2 s−1 1σ error on Nufnu_3.0 keV
Nufnu_0.5 keV D erg cm−2 s−1 Absorption-corrected (c)νf(ν) flux at 0.5 keV calculated from Ctr_03_1
Nufnu_0.5 keV_error D erg cm−2 s−1 1σ error or 3σ upper limit (d) on Nufnu_0.5 keV
Nufnu_1.5 keV D erg cm−2 s−1 Absorption-corrected (c)νf(ν) flux at 1.5 keV calculated from Ctr_1_2
Nufnu_1.5 keV_error D erg cm−2 s−1 1σ error or 3σ upper limit (d) on Nufnu_1.5 keV
Nufnu_4.5 keV D erg cm−2 s−1 Absorption-corrected (c)νf(ν) flux at 4.5 keV calculated from Ctr_2_10
Nufnu_4.5 keV_error D erg cm−2 s−1 1σ error or 3σ upper limit (d) on Nufnu_4.5 keV
Nufnu_1.0 keV D erg cm−2 s−1 νf(ν) flux at 1.0 keV interpolated between Nufnu_0.5 keV and Nufnu_1.5 keV
Nufnu_1.0 keV_error D erg cm−2 s−1 1σ error on Nufnu_1.0 keV
Spectral_slope D Power-law energy spectral index
Spectral_slope_error D 1σ error on Spectral_slope
Pileup flag 3A YES if Ctr_03_10 > 0.6 cts s−1, NO otherwise

Notes.

(a)

The vignetting-corrected exposure time is equivalent to the exposure with the source exactly at the centre of the field of view.

(b)

Upper limits are provided when no significant detection is achieved in the energy band considered.

(c)

Galactic absorption-corrected flux in the observer frame.

(d)

In case the source is not detected in this band, the Nufnu flux is set to 0 and the error is set equal to a 3σ upper limit.

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