Table 3
X-ray properties of AGN candidates.
| Object | Obs. ID | Obs. date | Exp. | Counts | N H | L 2−10 keV,obs | L 2−10 keV,exp |
|
|
|||||||
| J0045+1339 | 10294 | 2009 May 28 | 11562 | <4.6 | 5.3 | <5.3 × 1041 | 6.0 × 1042 |
| J1025+1402 | 10295 | 2009 Jan. 14 | 4937 | <4.6 | 3.6 | <1.1 × 1041 | 7.3 × 1042 |
| J1047+0739 | 10296 | 2009 Jun. 23 | 4782 | 3.0 |
2.4 | 2.2 × 1041 | 3.9 × 1043 |
| J1222+3602 | 10297 | 2009 Feb. 26 | 10718 | <4.6 | 1.2 | <5.5 × 1041 | 3.0 × 1042 |
| J1536+3122 | 11476 | 2010 Apr. 05 | 1822 | 2.0 |
2.1 | 4.1 × 1040 | 9.1 × 1041 |
| J0840+4707 | 17039 | 2015 Jan. 05 | 12892 | 4.0 |
2.8 | 7.9 × 1039 | 1.8 × 1042 |
| J1404+5423 | 2779 | 2002 Oct. 31 | 14276 | 9.0 |
1.8 | 1.5 × 1037 | 2.7 × 1039 |
Notes. Column 1: shortened SDSS object name. Column 2: Chandra observation identification number. Column 3: Chandra observation date (UT). Column 4: Chandra net exposure after cleaning in seconds. Column 5: Chandra 0.5−7.0 keV net counts derived from a 2′′ radius aperture. For detected sources, we quote Poisson errors derived from Gehrels (1986) at 1σ confidence level. For undetected sources, we derive 99% confidence upper limits based on the Bayesian technique of Kraft et al. (1991). Column 6: galactic Hi column density from Kalberla et al. (2005) in 1020 cm-2. Column 7: observed 2−10 keV luminosity or limit assuming a Γ = 1.8 powerlaw spectrum absorbed by Galactic NH, in erg s-1. Column 8: expected 2−10 keV luminosity based on the LX–LHα relation of P06, in erg s-1.
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