5XMM J173320.0+433838
5XMM-DR15 stacked source · SRCID 3002114050100027
Position:
17h33m20.00s +43d38m38.2s
(263.33331°, 43.64396°)
EP flux
2.09e-14
± 9.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.908)
Detections
7
| SRCID | 3002114050100027 |
|---|---|
| IAUNAME | 5XMM J173320.0+433838 |
| SC_RA | 17h33m20.00s (263.33331°) |
| SC_DEC | +43d38m38.2s (43.64396°) |
| RADEC_ERR | 0.64 arcsec |
| LII / BII | 69.3932° / 32.0033° |
| N_CONTRIB | 7 (detections) |
| N_OBS | 11 (observations covering the position) |
| MJD_FIRST | 52579.434 (2002-11-01 10:24:27.000 UTC) |
| MJD_LAST | 57689.145 (2016-10-28 03:29:31.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.09e-14 ± 9.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.24
± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
-0.03
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.31
± 0.17
1.0-2.0 / 2.0-4.5 keV
HR4
-0.29
± 0.40
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.839
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
Optical Monitor (OM)
- OM Source ID
- 4710740
- Match probability
- 0.991
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.573 | 0.160 |
| B | 21.588 | 0.204 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.72e-13 (+2.3e-13 / −1.2e-13) erg cm−2 s−1 |
|---|---|
| NH | 3.05e+20 (+1.4e+21 / −3.8e+19) cm−2 |
| Photon index (Γ) | 1.46 (+1.92 / −1.17) |
| DoF | 238 |
| p-value | 0.649 |
| Quality flag | 0 |
No variability data available for this source.
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.