5XMM J034102.8-012518
5XMM-DR15 stacked source · SRCID 3000294040100008
Position:
03h41m02.81s -01d25m18.0s
(55.26172°, -1.42167°)
EP flux
2.70e-14
± 9.7e-15
erg cm-2 s-1
CLASSX
AGN
(0.952)
Detections
2
| SRCID | 3000294040100008 |
|---|---|
| IAUNAME | 5XMM J034102.8-012518 |
| SC_RA | 03h41m02.81s (55.26172°) |
| SC_DEC | -01d25m18.0s (-1.42167°) |
| RADEC_ERR | 0.88 arcsec |
| LII / BII | 187.9195° / -41.9363° |
| 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): 2.70e-14 ± 9.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.47
± 0.15
0.2-0.5 / 0.5-1.0 keV
HR2
0.19
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.62
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.27
± 0.40
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.552
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
- 998067
- Match probability
- 0.998
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.152 | 0.256 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.75e-14 (+3.7e-14 / −2.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.86e+20 (+1.4e+21 / −4.0e+19) cm−2 |
| Photon index (Γ) | 1.93 (+2.49 / −1.62) |
| DoF | 201 |
| p-value | 0.631 |
| 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.