5XMM J031817.7-030947
5XMM-DR15 stacked source · SRCID 3005602220100018
Position:
03h18m17.79s -03d09m47.5s
(49.57414°, -3.16319°)
EP flux
3.88e-14
± 1.6e-14
erg cm-2 s-1
CLASSX
AGN
(0.948)
Detections
1
| SRCID | 3005602220100018 |
|---|---|
| IAUNAME | 5XMM J031817.7-030947 |
| SC_RA | 03h18m17.79s (49.57414°) |
| SC_DEC | -03d09m47.5s (-3.16319°) |
| RADEC_ERR | 1.04 arcsec |
| LII / BII | 185.0463° / -47.5196° |
| 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): 3.88e-14 ± 1.6e-14 erg cm-2 s-1
Hardness ratios
HR1
0.19
± 0.18
0.2-0.5 / 0.5-1.0 keV
HR2
0.28
± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.33
± 0.15
1.0-2.0 / 2.0-4.5 keV
HR4
-0.55
± 0.38
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.282
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
- 928504
- Match probability
- 0.863
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.429 | 0.232 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.48e-14 (+3.3e-14 / −1.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.65e+20 (+9.1e+20 / −2.7e+19) cm−2 |
| Photon index (Γ) | 2.02 (+2.48 / −1.74) |
| DoF | 273 |
| p-value | 0.658 |
| Inter-instrument norm. | 1.24 (0.92–1.59) |
| 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.