Table 2.
Comparison of fitted with other research studies.
Objects |
![]() |
![]() |
![]() |
Ref. | Methods |
---|---|---|---|---|---|
Mrk 335 | – |
![]() |
0.7 | Tripathi et al. (2020) | SED fitting |
Fairall 9 | 2.0 |
![]() |
0.2 | Pal et al. (2017) | – |
Ark 120 | 0.06 |
![]() |
1.0 | Porquet et al. (2018) | – |
MCG +08-11-011 | 0.15 |
![]() |
0.54 | Fausnaugh et al. (2018) | Bolometric correction |
NGC 2617 | 0.03 |
![]() |
0.1 | Fausnaugh et al. (2018) | Bolometric correction |
Mrk 110 | 10 |
![]() |
4 | Meyer-Hofmeister & Meyer (2011) | – |
Mrk 817 | 1.5 |
![]() |
2.0 | Kara et al. (2021) | fitting τ |
NGC 4151 | 0.5 |
![]() |
0.6–6 | Edelson et al. (2017) | – |
NGC 4593 | 0.09 |
![]() |
0.081 | McHardy et al. (2018) | SED fitting |
NGC 5548 | 0.3 |
![]() |
1 | Fausnaugh et al. (2016) | – |
Mrk 509 | 0.5 |
![]() |
0.5 | Edelson et al. (2019) | – |
NGC 7469 | 1.1 |
![]() |
0.5 | Pahari et al. (2020) | Bolometric correction |
Notes. is the accretion rates fitted by the present model,
is the
measured by Du & Wang (2019) and
is the
measured by other method, some of the methods are listed in the last column of the table, while ‘–’ represents the methods that are unclear to us. The references are list in the column Ref.
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