Table 1.

Emission line fluxes of the three main components identified in Section 4.1 from both the PRISM and R2700 grating data. The fluxes are in the units of |$10^{-19}$| erg s|$^{-1}$| cm|$^{-2}$|⁠. The upper limits are set as |$3\sigma$|⁠. For H α and [N ii]|$\lambda $||$\lambda $|6550,6585 and [O ii]|$\lambda $||$\lambda $|3727,3729 we only report the combined flux for the PRISM as we are unable to deblend the emission lines.

ObjectMainNorthEast
lineF|$_{\rm PRISM}$|F|$_{\rm F290LP}$|F|$_{\rm PRISM}$|F|$_{\rm F290LP}$|F|$_{\rm PRISM}$|F|$_{\rm F290LP}$|
H α + [N ii]|$\lambda $||$\lambda $|6550,6585272.5|$\pm$|5.9248.0|$\pm$| 1.756.6|$\pm$|1.358.3|$\pm$| 0.96.1|$\pm$|0.44.3|$\pm$| 0.2
H α-234.4|$\pm$|1.9-51.5|$\pm$| 0.9-3.9|$\pm$| 0.2
[N ii]|$\lambda $||$\lambda $|6550,6585-14.2|$\pm$|1.1-5.1|$\pm$| 0.8-<0.8
[O iii]|$\lambda $||$\lambda $|5007,4959528.7|$\pm$|6.2538.5|$\pm$|2.288.6|$\pm$|1.190.9|$\pm$| 0.812.2|$\pm$|0.38.6|$\pm$| 0.2
H β76.6|$\pm$|3.265.9|$\pm$|1.014.1|$\pm$|0.914.6|$\pm$| 0.42.4|$\pm$|0.31.4|$\pm$| 0.2
He ii|$\lambda $|4686<8.7<2.4<2.3<0.4<0.8<0.9
H |$\gamma$|27.5|$\pm$|3.229.2|$\pm$|1.06.5|$\pm$|0.86.5|$\pm$| 0.4<0.90.6|$\pm$| 0.1
[O iii]|$\lambda $|436310.8|$\pm$|3.07.0|$\pm$|0.9<2.22.0|$\pm$| 0.4<0.9<1.5
H |$\delta$|15.3|$\pm$|2.914.9|$\pm$|1.84.4|$\pm$|0.83.5|$\pm$| 0.6<0.9<1.1
[Ne iii]|$\lambda $|386935.7|$\pm$|3.336.4|$\pm$|1.26.6|$\pm$|0.96.4|$\pm$| 0.5<1.1<1.6
[O ii]|$\lambda $||$\lambda $|3727,372981.3|$\pm$|3.785.7|$\pm$|2.726.1|$\pm$|1.026.8|$\pm$|1.22.4|$\pm$|0.4<2.5
[O ii]|$\lambda $|3727-48.4|$\pm$|2.1-13.9|$\pm$| 0.7-<1.4
[O ii]|$\lambda $|3729-37.4|$\pm$|2.0-12.9|$\pm$| 0.8-<1.1
C iii]|$\lambda $|1906<23.1-<29.7-<16.8-
N iii]|$\lambda $|1750<36.1-<33.1-<19.5-
He ii|$\lambda $|1640  + [O iii]|$\lambda $|1660<28.8-<39.0-<22.8-
C iv]|$\lambda $|1550<33-<42.1-<24.9-
N iv]|$\lambda $|1497<26.1-<45.0-<27.6-
ObjectMainNorthEast
lineF|$_{\rm PRISM}$|F|$_{\rm F290LP}$|F|$_{\rm PRISM}$|F|$_{\rm F290LP}$|F|$_{\rm PRISM}$|F|$_{\rm F290LP}$|
H α + [N ii]|$\lambda $||$\lambda $|6550,6585272.5|$\pm$|5.9248.0|$\pm$| 1.756.6|$\pm$|1.358.3|$\pm$| 0.96.1|$\pm$|0.44.3|$\pm$| 0.2
H α-234.4|$\pm$|1.9-51.5|$\pm$| 0.9-3.9|$\pm$| 0.2
[N ii]|$\lambda $||$\lambda $|6550,6585-14.2|$\pm$|1.1-5.1|$\pm$| 0.8-<0.8
[O iii]|$\lambda $||$\lambda $|5007,4959528.7|$\pm$|6.2538.5|$\pm$|2.288.6|$\pm$|1.190.9|$\pm$| 0.812.2|$\pm$|0.38.6|$\pm$| 0.2
H β76.6|$\pm$|3.265.9|$\pm$|1.014.1|$\pm$|0.914.6|$\pm$| 0.42.4|$\pm$|0.31.4|$\pm$| 0.2
He ii|$\lambda $|4686<8.7<2.4<2.3<0.4<0.8<0.9
H |$\gamma$|27.5|$\pm$|3.229.2|$\pm$|1.06.5|$\pm$|0.86.5|$\pm$| 0.4<0.90.6|$\pm$| 0.1
[O iii]|$\lambda $|436310.8|$\pm$|3.07.0|$\pm$|0.9<2.22.0|$\pm$| 0.4<0.9<1.5
H |$\delta$|15.3|$\pm$|2.914.9|$\pm$|1.84.4|$\pm$|0.83.5|$\pm$| 0.6<0.9<1.1
[Ne iii]|$\lambda $|386935.7|$\pm$|3.336.4|$\pm$|1.26.6|$\pm$|0.96.4|$\pm$| 0.5<1.1<1.6
[O ii]|$\lambda $||$\lambda $|3727,372981.3|$\pm$|3.785.7|$\pm$|2.726.1|$\pm$|1.026.8|$\pm$|1.22.4|$\pm$|0.4<2.5
[O ii]|$\lambda $|3727-48.4|$\pm$|2.1-13.9|$\pm$| 0.7-<1.4
[O ii]|$\lambda $|3729-37.4|$\pm$|2.0-12.9|$\pm$| 0.8-<1.1
C iii]|$\lambda $|1906<23.1-<29.7-<16.8-
N iii]|$\lambda $|1750<36.1-<33.1-<19.5-
He ii|$\lambda $|1640  + [O iii]|$\lambda $|1660<28.8-<39.0-<22.8-
C iv]|$\lambda $|1550<33-<42.1-<24.9-
N iv]|$\lambda $|1497<26.1-<45.0-<27.6-
Table 1.

Emission line fluxes of the three main components identified in Section 4.1 from both the PRISM and R2700 grating data. The fluxes are in the units of |$10^{-19}$| erg s|$^{-1}$| cm|$^{-2}$|⁠. The upper limits are set as |$3\sigma$|⁠. For H α and [N ii]|$\lambda $||$\lambda $|6550,6585 and [O ii]|$\lambda $||$\lambda $|3727,3729 we only report the combined flux for the PRISM as we are unable to deblend the emission lines.

ObjectMainNorthEast
lineF|$_{\rm PRISM}$|F|$_{\rm F290LP}$|F|$_{\rm PRISM}$|F|$_{\rm F290LP}$|F|$_{\rm PRISM}$|F|$_{\rm F290LP}$|
H α + [N ii]|$\lambda $||$\lambda $|6550,6585272.5|$\pm$|5.9248.0|$\pm$| 1.756.6|$\pm$|1.358.3|$\pm$| 0.96.1|$\pm$|0.44.3|$\pm$| 0.2
H α-234.4|$\pm$|1.9-51.5|$\pm$| 0.9-3.9|$\pm$| 0.2
[N ii]|$\lambda $||$\lambda $|6550,6585-14.2|$\pm$|1.1-5.1|$\pm$| 0.8-<0.8
[O iii]|$\lambda $||$\lambda $|5007,4959528.7|$\pm$|6.2538.5|$\pm$|2.288.6|$\pm$|1.190.9|$\pm$| 0.812.2|$\pm$|0.38.6|$\pm$| 0.2
H β76.6|$\pm$|3.265.9|$\pm$|1.014.1|$\pm$|0.914.6|$\pm$| 0.42.4|$\pm$|0.31.4|$\pm$| 0.2
He ii|$\lambda $|4686<8.7<2.4<2.3<0.4<0.8<0.9
H |$\gamma$|27.5|$\pm$|3.229.2|$\pm$|1.06.5|$\pm$|0.86.5|$\pm$| 0.4<0.90.6|$\pm$| 0.1
[O iii]|$\lambda $|436310.8|$\pm$|3.07.0|$\pm$|0.9<2.22.0|$\pm$| 0.4<0.9<1.5
H |$\delta$|15.3|$\pm$|2.914.9|$\pm$|1.84.4|$\pm$|0.83.5|$\pm$| 0.6<0.9<1.1
[Ne iii]|$\lambda $|386935.7|$\pm$|3.336.4|$\pm$|1.26.6|$\pm$|0.96.4|$\pm$| 0.5<1.1<1.6
[O ii]|$\lambda $||$\lambda $|3727,372981.3|$\pm$|3.785.7|$\pm$|2.726.1|$\pm$|1.026.8|$\pm$|1.22.4|$\pm$|0.4<2.5
[O ii]|$\lambda $|3727-48.4|$\pm$|2.1-13.9|$\pm$| 0.7-<1.4
[O ii]|$\lambda $|3729-37.4|$\pm$|2.0-12.9|$\pm$| 0.8-<1.1
C iii]|$\lambda $|1906<23.1-<29.7-<16.8-
N iii]|$\lambda $|1750<36.1-<33.1-<19.5-
He ii|$\lambda $|1640  + [O iii]|$\lambda $|1660<28.8-<39.0-<22.8-
C iv]|$\lambda $|1550<33-<42.1-<24.9-
N iv]|$\lambda $|1497<26.1-<45.0-<27.6-
ObjectMainNorthEast
lineF|$_{\rm PRISM}$|F|$_{\rm F290LP}$|F|$_{\rm PRISM}$|F|$_{\rm F290LP}$|F|$_{\rm PRISM}$|F|$_{\rm F290LP}$|
H α + [N ii]|$\lambda $||$\lambda $|6550,6585272.5|$\pm$|5.9248.0|$\pm$| 1.756.6|$\pm$|1.358.3|$\pm$| 0.96.1|$\pm$|0.44.3|$\pm$| 0.2
H α-234.4|$\pm$|1.9-51.5|$\pm$| 0.9-3.9|$\pm$| 0.2
[N ii]|$\lambda $||$\lambda $|6550,6585-14.2|$\pm$|1.1-5.1|$\pm$| 0.8-<0.8
[O iii]|$\lambda $||$\lambda $|5007,4959528.7|$\pm$|6.2538.5|$\pm$|2.288.6|$\pm$|1.190.9|$\pm$| 0.812.2|$\pm$|0.38.6|$\pm$| 0.2
H β76.6|$\pm$|3.265.9|$\pm$|1.014.1|$\pm$|0.914.6|$\pm$| 0.42.4|$\pm$|0.31.4|$\pm$| 0.2
He ii|$\lambda $|4686<8.7<2.4<2.3<0.4<0.8<0.9
H |$\gamma$|27.5|$\pm$|3.229.2|$\pm$|1.06.5|$\pm$|0.86.5|$\pm$| 0.4<0.90.6|$\pm$| 0.1
[O iii]|$\lambda $|436310.8|$\pm$|3.07.0|$\pm$|0.9<2.22.0|$\pm$| 0.4<0.9<1.5
H |$\delta$|15.3|$\pm$|2.914.9|$\pm$|1.84.4|$\pm$|0.83.5|$\pm$| 0.6<0.9<1.1
[Ne iii]|$\lambda $|386935.7|$\pm$|3.336.4|$\pm$|1.26.6|$\pm$|0.96.4|$\pm$| 0.5<1.1<1.6
[O ii]|$\lambda $||$\lambda $|3727,372981.3|$\pm$|3.785.7|$\pm$|2.726.1|$\pm$|1.026.8|$\pm$|1.22.4|$\pm$|0.4<2.5
[O ii]|$\lambda $|3727-48.4|$\pm$|2.1-13.9|$\pm$| 0.7-<1.4
[O ii]|$\lambda $|3729-37.4|$\pm$|2.0-12.9|$\pm$| 0.8-<1.1
C iii]|$\lambda $|1906<23.1-<29.7-<16.8-
N iii]|$\lambda $|1750<36.1-<33.1-<19.5-
He ii|$\lambda $|1640  + [O iii]|$\lambda $|1660<28.8-<39.0-<22.8-
C iv]|$\lambda $|1550<33-<42.1-<24.9-
N iv]|$\lambda $|1497<26.1-<45.0-<27.6-
Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close