Table 1.
Basic information on 1H 0707–495, NGC 1566, and NGC 7679.
Source parameter | 1H 0707–495 | NGC 1566 | Mrk 3 | NGC 7679 |
---|---|---|---|---|
Class of AGN | Sy1, NLS1 (a) | CL-AGN, SAB(s)bc (b) | Sy2, S0, HBLR (c) | Sy2, SB0, SB+AGN |
Mass of BH, M⊙ | 2 × 106–107 (d) | 8.3 × 106 − 1.3 × 107 (e, f) | 5.5× 108 (g) | 5.9× 106 (h) |
Inclination, i, deg | 55-65 (i) | 60 ± 5 (j), | 50 (c) | 30 (k) |
Distance, D, Mpc | 160 (l) | 21.3 (m) | 63.2 (c) | 58.633± 1.910 (k) |
Redshift, z | 0.041(d) | 0.005 (j, m) | 0.013 (c) | 0.017 (d) |
RA (J2000), α | 07h 08m 41.48s (l) | 04h 20m 00.52s (l) | 06h 15m 36.3s (l) | 23h 28m 46.73s (l) |
Dec (J2000), δ | –49° 33′06.4″(l) | –54° 56′17.1″(l) | +71° 2′15″(l) | +03° 30′42.1″(l) |
Mean count rate, ct/s | 0.1975±0.0013 (l) | 0.2984±0.0013 (l) | 0.192±0.012 (l) | 0.192±0.012 (l) |
Mean flux, | 4.533±0.030 (l) | 11.74±0.05 (l) | 9.7±0.7 (l) | 7.9±0.5 (l) |
×10−12 erg/s/cm2 | ||||
Swift name, 2SXPS... | J070841.4–493306 | J0420.0–5457 | J061536.2+710214 | J232846.7+033042 |
Alternative names | 1H 0659–494, | ESO 157–20, | UGC 03426 | Arp 216, Mrk 534, |
4U 0708–49 | IRAS 04189–5503, | PGC 71554, VV 329a, | ||
PGC 14897 | UGC 12618 | |||
NH, Gal, cm−2 | 8.0×1020 (k) | 1.1×1020 (k) | 1.8×1020 (l) | 4.5×1020 (m) |
Notes. NLS1 – Narrowline Seyfert 1 galaxy; SAB(s)bc – barred spiral galaxy; CL-AGN – changing-look AGN; SB0 – early-type barred galaxy; S0 – lenticular galaxy; HBLR – hidden broad-line-region; Mean count rate and flux of the source is measured in 0.3–10 keV range. (a)Zoghbi et al. (2011) ; (b)de Vaucouleurs (1973); (c)Véron-Cetty & Véron (2006), Ricci et al. (2014); (d)Zhou & Wang (2005), Kara et al. (2013), Done & Jin (2016), Zoghbi et al. (2011); (e)Woo & Urry (2002); (f)Elagali et al. (2019); (g)Fabian et al. (2009); (h)Hancock et al. (2023); (i)Aguero et al. (2004); (j)Kewley et al. (2001), Springob et al. (2005); (k)Galactic neutral hydrogen column density along the line of sight from the Leiden/Dwingeloo Survey Hartmann & Burton (1997); (l) https://www.swift.ac.uk/2SXPS/; and (m)Della Ceca et al. (2001).
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