A systematic study of the ultra-fast outflow responses to luminosity variations in active galactic nuclei

Home

All issues

Volume 687 (July 2024)

A&A, 687 (2024) A179

Full HTML

Open Access

Table 1.

Six sources in this sample plus four previously studied sources.

Source	Type	Redshift	log(M_BH/M_⊙)	Exposure	RGS counts	L_bol	λ_Edd	i
		z		(ks)	(10⁵)	(10⁴⁴ erg s⁻¹)	(≡L_bol/L_Edd)	(deg)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)
This work

1H 1934-063	NLS1	0.0102	$6 . 46_{- 0.20}^{+ 0.20}$ $6.46^{+0.20}_{-0.20}$ ^(a)^(b)	492	4.2	1.73 ^(m)⁽ⁿ⁾	0.47 ± 0.22	$42_{- 2}^{+ 14}$ $42^{+14}_{-2}$ ⁽ⁿ⁾
RE J1034+396	NLS1	0.042	$6 . 40_{- 0.4}^{+ 0.2}$ $6.40^{+0.2}_{-0.4}$ ^(c)	1417	3.7	2.7 − 5.4 ⁽ⁿ⁾^(o)	1.29 ± 0.43	$30_{- 28}^{+ 28}$ $30^{+28}_{-28}$ ^(w)
PG 1244+026	NLS1	0.048	$7 . 11_{- 0.41}^{+ 0.14}$ $7.11^{+0.14}_{-0.41}$ ^(b)^(d)^(e)	764	2.8	14 − 17 ⁽ⁿ⁾^(p)	1.04 ± 0.59	$31_{- 1}^{+ 1}$ $31^{+1}_{-1}$ ⁽ⁿ⁾
PG 1211+143	NLS1/quasar	0.0809	$8 . 16_{- 0.15}^{+ 0.12}$ $8.16^{+0.12}_{-0.15}$ ^(f)	876	2.3	31 − 53 ⁽ⁿ⁾^(q)	0.23 ± 0.08	$30_{- 1}^{+ 1}$ $30^{+1}_{-1}$ ⁽ⁿ⁾
I ZW 1	NLS1	0.061	$7 . 45_{- 0.12}^{+ 0.08}$ $7.45^{+0.08}_{-0.12}$ ^(g)	528	1.8	22 − 39 ⁽ⁿ⁾^(r)	0.88 ± 0.21	$39_{- 2}^{+ 4}$ $39^{+4}_{-2}$ ⁽ⁿ⁾
IRAS 17020+4544	NLS1	0.0604	$6 . 72_{- 0.10}^{+ 0.10}$ $6.72^{+0.10}_{-0.10}$ ^(b)^(h)	209	0.8	7.8 − 9.9 ⁽ⁿ⁾^(s)	1.33 ± 0.31	$55_{- 4}^{+ 4}$ $55^{+4}_{-4}$ ⁽ⁿ⁾

Published work

Mrk 1044	NLS1	0.016	$6 . 45_{- 0.13}^{+ 0.12}$ $6.45^{+0.12}_{-0.13}$ ⁽ⁱ⁾	733	9.8	1.3 − 1.6 ^(t)	0.40 ± 0.12	$34_{- 2}^{+ 1}$ $34^{+1}_{-2}$ ^(x)
1H 0707-495	NLS1	0.0406	$6 . 30_{- 0.30}^{+ 0.30}$ $6.30^{+0.30}_{-0.30}$ ^(j)	1385	4.1	2 − 55 ^(u)	9.05 ± 5.43	$43_{- 2}^{+ 2}$ $43^{+2}_{-2}$ ^(y)
IRAS 13224−3809	NLS1	0.0658	$6 . 54_{- 0.08}^{+ 0.41}$ $6.54^{+0.41}_{-0.08}$ ^(k)	2131	3.3	4 − 13 ^(v)	1.13 ± 0.58	$59_{- 1}^{+ 1}$ $59^{+1}_{-1}$ ^(y)
PDS 456	Quasar	0.184	$9 . 3_{- 0.4}^{+ 0.4}$ $9.3^{+0.4}_{-0.4}$ ^(l)	1146	1.1	1800 ^(l)	0.72 ± 0.66	$65_{- 2}^{+ 2}$ $65^{+2}_{-2}$ ^(l)

Notes. The table includes the source name (1), AGN type (2), redshift (3), black hole mass (4), total on-axis XMM-Newton exposure time without solar flare correction (5), total counts in the RGS band with solar flare correction (6), bolometric luminosity (7), Eddington ratio (8) and disk inclination angle (9). See more details in Sect. 2.

References.

^(a)

Malizia et al. (2008);

^(b)

Ponti et al. (2012);

^(c)

Bian & Huang (2010);

^(d)

Kara et al. (2014);

^(e)

Marconi et al. (2008);

^(f)

Peterson et al. (2004);

^(g)

Vestergaard & Peterson (2006);

^(h)

Wang & Lu (2001);

⁽ⁱ⁾

Du et al. (2015);

^(j)

Done & Jin (2016);

^(k)

Chiang et al. (2015);

^(l)

Reeves et al. (2009);

^(m)

Xu et al. (2022);

⁽ⁿ⁾

This work;

^(o)

Czerny et al. (2016);

^(p)

Jin et al. (2013);

^(q)

Kriss et al. (2018);

^(r)

Porquet et al. (2004);

^(s)

Gonzalez et al. (2020);

^(t)

Husemann et al. (2022);

^(u)

Xu et al. (2021b);

^(v)

Buisson et al. (2018);

^(w)

Hu et al. (2014);

^(x)

Xu et al. (2023);

^(y)

Parker et al. (2018).

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.