5XMM J031818.1-030054
5XMM-DR15 stacked source · SRCID 3005602220100001
Position:
03h18m18.14s -03d00m54.9s
(49.57559°, -3.01526°)
EP flux
3.36e-13
± 1.6e-14
erg cm-2 s-1
CLASSX
AGN
(0.743)
Detections
1
| SRCID | 3005602220100001 |
|---|---|
| IAUNAME | 5XMM J031818.1-030054 |
| SC_RA | 03h18m18.14s (49.57559°) |
| SC_DEC | -03d00m54.9s (-3.01526°) |
| RADEC_ERR | 0.21 arcsec |
| LII / BII | 184.8754° / -47.4273° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52503.423 (2002-08-17 10:08:51.000 UTC) |
| MJD_LAST | 52503.706 (2002-08-17 16:56:53.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.36e-13 ± 1.6e-14 erg cm-2 s-1
Hardness ratios
HR1
0.17
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.05
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.32
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.55
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.355
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
- 928560
- Match probability
- 0.967
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.474 | 0.090 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.50e-13 (+3.7e-13 / −3.3e-13) erg cm−2 s−1 |
|---|---|
| NH | 3.97e+19 (+1.2e+20 / −1.5e+19) cm−2 |
| Photon index (Γ) | 1.78 (+1.83 / −1.74) |
| DoF | 1379 |
| p-value | 0.994 |
| Inter-instrument norm. | 0.82 (0.77–0.87) |
| 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.