Table 4.

SDSS spectral fitting results.

No.Object|$\rm FWHM_{H\alpha ^b}$||$\rm FWHM_{H\beta ^b}$||$\log L_{\rm H\alpha ^b}$||$\log L_{\rm H\beta ^b}$|log L5100|$L_{\rm H\alpha ^b}/L_{\rm H\beta ^b}$|log (MBH/M|$\odot$|)
(1)(2)(3)(4)(5)(6)(7)(8)(9)
1Mrk 10184152601142.1741.7443.862.678.40
2MCG 04-22-0422062298942.3441.9743.692.337.71
3Mrk 7052062203942.0341.5743.382.887.22
4RX J1007.1 + 22032092240742.1741.6743.663.177.50
5CBS 1262639291443.0042.5344.182.947.93
6Mrk 1413624667241.9141.3943.513.318.31
7Mrk 1421494165042.0041.5843.602.647.15
8Ton 13882966400444.1143.6045.273.258.75
9SBS 1136 + 5942637324942.7242.2443.862.997.86
10PG 1138 + 2222246224642.5542.0243.953.347.59
11KUG 1141 + 3716795904941.8241.3643.282.838.46
12Mrk 13102252271741.3140.9242.752.467.16
13RX J1209.8 + 32172019203842.5442.0844.092.897.57
14Mrk 504838583741.7841.3343.072.837.98
15Mrk 7712800335842.6642.1943.912.927.92
16PG 1307 + 0853650461243.6743.1844.783.138.63
17Ton 7303009352042.4942.1243.952.337.98
18RX J1355.2 + 56121141119242.6742.1644.163.227.14
19Mrk 13924183537142.2941.8343.602.918.17
20Mrk 2903612453342.2241.8243.582.538.01
21Mrk 4931095109541.7141.2943.412.637.51
22KUG 1618 + 4102045241841.2240.7542.902.927.13
23RX J1702.5 + 32472330244243.2742.8244.702.828.03
No.Object|$\rm FWHM_{H\alpha ^b}$||$\rm FWHM_{H\beta ^b}$||$\log L_{\rm H\alpha ^b}$||$\log L_{\rm H\beta ^b}$|log L5100|$L_{\rm H\alpha ^b}/L_{\rm H\beta ^b}$|log (MBH/M|$\odot$|)
(1)(2)(3)(4)(5)(6)(7)(8)(9)
1Mrk 10184152601142.1741.7443.862.678.40
2MCG 04-22-0422062298942.3441.9743.692.337.71
3Mrk 7052062203942.0341.5743.382.887.22
4RX J1007.1 + 22032092240742.1741.6743.663.177.50
5CBS 1262639291443.0042.5344.182.947.93
6Mrk 1413624667241.9141.3943.513.318.31
7Mrk 1421494165042.0041.5843.602.647.15
8Ton 13882966400444.1143.6045.273.258.75
9SBS 1136 + 5942637324942.7242.2443.862.997.86
10PG 1138 + 2222246224642.5542.0243.953.347.59
11KUG 1141 + 3716795904941.8241.3643.282.838.46
12Mrk 13102252271741.3140.9242.752.467.16
13RX J1209.8 + 32172019203842.5442.0844.092.897.57
14Mrk 504838583741.7841.3343.072.837.98
15Mrk 7712800335842.6642.1943.912.927.92
16PG 1307 + 0853650461243.6743.1844.783.138.63
17Ton 7303009352042.4942.1243.952.337.98
18RX J1355.2 + 56121141119242.6742.1644.163.227.14
19Mrk 13924183537142.2941.8343.602.918.17
20Mrk 2903612453342.2241.8243.582.538.01
21Mrk 4931095109541.7141.2943.412.637.51
22KUG 1618 + 4102045241841.2240.7542.902.927.13
23RX J1702.5 + 32472330244243.2742.8244.702.828.03

Notes: Column (1): identification number assigned in this paper. Column (2): NED name of the sample objects. Column (3): FWHM of the |$\rm H\alpha$| broad component. Column (4): FWHM of the |$\rm H\beta$| broad component. Column (5): logarithmic of the luminosity of the |$\rm H\alpha$| broad component in units of erg s−1. Column (6): logarithmic of the luminosity of the |$\rm H\beta$| broad component in units of erg s−1. Column (7): logarithmic of the 5100 Å monochromatic luminosity in units of erg s−1. Column (8): broad-line Balmer decrement derived from |$L_{\rm H\alpha ^b}$|/|$L_{\rm H\beta ^b}$|⁠. Column (9): logarithmic of Black hole mass MBH derived from |$\rm FWHM({H\beta ^b})$| and L5100 (Vestergaard & Peterson 2006) in units of M|$\odot$|.

Table 4.

SDSS spectral fitting results.

No.Object|$\rm FWHM_{H\alpha ^b}$||$\rm FWHM_{H\beta ^b}$||$\log L_{\rm H\alpha ^b}$||$\log L_{\rm H\beta ^b}$|log L5100|$L_{\rm H\alpha ^b}/L_{\rm H\beta ^b}$|log (MBH/M|$\odot$|)
(1)(2)(3)(4)(5)(6)(7)(8)(9)
1Mrk 10184152601142.1741.7443.862.678.40
2MCG 04-22-0422062298942.3441.9743.692.337.71
3Mrk 7052062203942.0341.5743.382.887.22
4RX J1007.1 + 22032092240742.1741.6743.663.177.50
5CBS 1262639291443.0042.5344.182.947.93
6Mrk 1413624667241.9141.3943.513.318.31
7Mrk 1421494165042.0041.5843.602.647.15
8Ton 13882966400444.1143.6045.273.258.75
9SBS 1136 + 5942637324942.7242.2443.862.997.86
10PG 1138 + 2222246224642.5542.0243.953.347.59
11KUG 1141 + 3716795904941.8241.3643.282.838.46
12Mrk 13102252271741.3140.9242.752.467.16
13RX J1209.8 + 32172019203842.5442.0844.092.897.57
14Mrk 504838583741.7841.3343.072.837.98
15Mrk 7712800335842.6642.1943.912.927.92
16PG 1307 + 0853650461243.6743.1844.783.138.63
17Ton 7303009352042.4942.1243.952.337.98
18RX J1355.2 + 56121141119242.6742.1644.163.227.14
19Mrk 13924183537142.2941.8343.602.918.17
20Mrk 2903612453342.2241.8243.582.538.01
21Mrk 4931095109541.7141.2943.412.637.51
22KUG 1618 + 4102045241841.2240.7542.902.927.13
23RX J1702.5 + 32472330244243.2742.8244.702.828.03
No.Object|$\rm FWHM_{H\alpha ^b}$||$\rm FWHM_{H\beta ^b}$||$\log L_{\rm H\alpha ^b}$||$\log L_{\rm H\beta ^b}$|log L5100|$L_{\rm H\alpha ^b}/L_{\rm H\beta ^b}$|log (MBH/M|$\odot$|)
(1)(2)(3)(4)(5)(6)(7)(8)(9)
1Mrk 10184152601142.1741.7443.862.678.40
2MCG 04-22-0422062298942.3441.9743.692.337.71
3Mrk 7052062203942.0341.5743.382.887.22
4RX J1007.1 + 22032092240742.1741.6743.663.177.50
5CBS 1262639291443.0042.5344.182.947.93
6Mrk 1413624667241.9141.3943.513.318.31
7Mrk 1421494165042.0041.5843.602.647.15
8Ton 13882966400444.1143.6045.273.258.75
9SBS 1136 + 5942637324942.7242.2443.862.997.86
10PG 1138 + 2222246224642.5542.0243.953.347.59
11KUG 1141 + 3716795904941.8241.3643.282.838.46
12Mrk 13102252271741.3140.9242.752.467.16
13RX J1209.8 + 32172019203842.5442.0844.092.897.57
14Mrk 504838583741.7841.3343.072.837.98
15Mrk 7712800335842.6642.1943.912.927.92
16PG 1307 + 0853650461243.6743.1844.783.138.63
17Ton 7303009352042.4942.1243.952.337.98
18RX J1355.2 + 56121141119242.6742.1644.163.227.14
19Mrk 13924183537142.2941.8343.602.918.17
20Mrk 2903612453342.2241.8243.582.538.01
21Mrk 4931095109541.7141.2943.412.637.51
22KUG 1618 + 4102045241841.2240.7542.902.927.13
23RX J1702.5 + 32472330244243.2742.8244.702.828.03

Notes: Column (1): identification number assigned in this paper. Column (2): NED name of the sample objects. Column (3): FWHM of the |$\rm H\alpha$| broad component. Column (4): FWHM of the |$\rm H\beta$| broad component. Column (5): logarithmic of the luminosity of the |$\rm H\alpha$| broad component in units of erg s−1. Column (6): logarithmic of the luminosity of the |$\rm H\beta$| broad component in units of erg s−1. Column (7): logarithmic of the 5100 Å monochromatic luminosity in units of erg s−1. Column (8): broad-line Balmer decrement derived from |$L_{\rm H\alpha ^b}$|/|$L_{\rm H\beta ^b}$|⁠. Column (9): logarithmic of Black hole mass MBH derived from |$\rm FWHM({H\beta ^b})$| and L5100 (Vestergaard & Peterson 2006) in units of M|$\odot$|.

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