Chemical enrichment and accretion of nitrogen-loud quasars

K. Matsuoka; T. Nagao; R. Maiolino; A. Marconi; D. Park; Y. Taniguchi

doi:10.1051/0004-6361/201629878

Home

All issues

Volume 608 (December 2017)

A&A, 608 (2017) A90

Full HTML

Free Access

Table 3

Estimates of 3σ flux upper limits of undetected emission lines.

Object	F_{[Ne v]}	F_{[O ii]}	F_{[Ne iii]}
	[10^-17 erg s^-1 cm^-2]

SDSS J0357−0528	–^a	<16.47	<9.41
SDSS J0931+3439	–^a	<10.43	<6.40
SDSS J1211+0449	–^a	–^a	–^a
SDSS J0756+2054	<17.23	<12.57	<14.52
SDSS J0803+1742	<17.89	<13.29	<12.95
SDSS J0857+2636	<11.75	<7.15	<10.77
SDSS J0938+0900	<28.46	<18.74	<24.54
SDSS J1036+1247	<21.31	<15.20	<14.71
SDSS J1110+0456^b	<14.39	<8.80	<11.52
SDSS J1130+1512	<16.26	<9.87	<14.31
SDSS J1134+1500	<49.02	<46.02	<42.98
SDSS J1308+1136	<29.67	<29.45	<16.50

Notes.

^(a)

Out of the wavelength coverage;

^(b)

based on the averaged FWHM_[O iii] value of 24.2 Å, due to the lack of the [O iii]λ5007 line detection.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.