5XMM J034053.9-012305
5XMM-DR15 stacked source · SRCID 3000294040100001
Position:
03h40m53.90s -01d23m05.9s
(55.22460°, -1.38498°)
EP flux
3.56e-13
± 2.5e-14
erg cm-2 s-1
CLASSX
AGN
(0.888)
Detections
2
| SRCID | 3000294040100001 |
|---|---|
| IAUNAME | 5XMM J034053.9-012305 |
| SC_RA | 03h40m53.90s (55.22460°) |
| SC_DEC | -01d23m05.9s (-1.38498°) |
| RADEC_ERR | 0.23 arcsec |
| LII / BII | 187.8502° / -41.9445° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52302.856 (2002-01-28 20:33:21.000 UTC) |
| MJD_LAST | 53026.876 (2004-01-22 21:00:55.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.56e-13 ± 2.5e-14 erg cm-2 s-1
Hardness ratios
HR1
0.28
± 0.04
0.2-0.5 / 0.5-1.0 keV
HR2
0.03
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.47
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.28
± 0.08
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.841
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
- 997507
- Match probability
- 0.999
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 20.452 | 0.198 |
| UVM2 | — | — |
| UVW1 | 19.931 | 0.067 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.58e-13 (+2.8e-13 / −2.4e-13) erg cm−2 s−1 |
|---|---|
| NH | 3.62e+20 (+6.1e+20 / −1.0e+20) cm−2 |
| Photon index (Γ) | 1.95 (+2.07 / −1.82) |
| DoF | 614 |
| p-value | 0.704 |
| Inter-instrument norm. | 1.03 (0.95–1.11) |
| 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.