Table B.1.
Results of fitting the BLR model to the line profiles.
ID | Model | Tied? | HαRBLR [ld] | β | ϵ | i [°] | θ0 [°] | κ | γ | ξ | fflow | fellip | θe [°] | Δϕpeak |
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× 10−3 | ||||||||||||||
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) | (14) | (15) |
1 | F | - |
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2 | C | - |
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3 | C | - |
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4 | C | - |
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5 | F | - |
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6 | C | Y |
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7 | C | - |
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8 | C | - |
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9 | C | Y |
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10 | C | Y |
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11 | C | - |
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12 | C | - |
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13 | C | N |
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14 | C | - |
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15 | C | Y |
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16 | C | Y |
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17 | C | Y |
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18 | C | Y |
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19 | C | - |
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20 | C | Y |
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21 | C | Y |
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22 | C | Y |
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23 | C | Y |
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24 | C | Y |
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25 | C | Y |
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26 | C | - |
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27 | C | Y |
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28 | C | Y |
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29 | C | N |
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Note: The columns show (1) the ID number, (2) the model used (C for circular, F for full), (3) whether the central wavelength of Hβ and Hγ was tied to that of Hα whenever the other Balmer lines are available, (4) the Hα BLR size in ld, (5) the shape parameter of the radial cloud distribution, (6) the amount of shift on the central wavelength of the Balmer line(s), (7) inclination angle, (8) position angle, (9) anisotropy parameter, (10) vertical distribution of clouds, (11) midplane obscuration, (12) binary switch for inflowing (fflow < 0.5) and outflowing (fflow > 0.5) radial motion, (13) fraction of clouds in circular/bound orbits, (14) angular location for radial orbit distribution, and (15) the peak expected differential phase. All errors are 1σ uncertainties. More details about the BLR model parameters are discussed in Sect. 5, while the calculation of the peak expected differential phase is shown in Sect. 6.
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