5XMM J034009.9-352454
5XMM-DR15 stacked source · SRCID 3005514010100663
Position:
03h40m09.91s -35d24m54.3s
(55.04130°, -35.41508°)
EP flux
8.11e-15
± 3.3e-15
erg cm-2 s-1
CLASSX
AGN
(0.896)
Detections
1
| SRCID | 3005514010100663 |
|---|---|
| IAUNAME | 5XMM J034009.9-352454 |
| SC_RA | 03h40m09.91s (55.04130°) |
| SC_DEC | -35d24m54.3s (-35.41508°) |
| RADEC_ERR | 1.42 arcsec |
| LII / BII | 236.6448° / -53.2941° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 17 (observations covering the position) |
| MJD_FIRST | 51916.608 (2001-01-07 14:34:55.000 UTC) |
| MJD_LAST | 51917.169 (2001-01-08 04:04:01.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.11e-15 ± 3.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.10
± 0.19
0.2-0.5 / 0.5-1.0 keV
HR2
-0.22
± 0.23
0.5-1.0 / 1.0-2.0 keV
HR3
-0.48
± 0.22
1.0-2.0 / 2.0-4.5 keV
HR4
-0.04
± 0.39
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.14
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
- 995472
- Match probability
- 0.911
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 21.197 | 0.160 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 4.12e-15 (+5.9e-15 / −3.0e-15) erg cm−2 s−1 |
|---|---|
| NH | 6.69e+19 (+2.8e+20 / −1.8e+19) cm−2 |
| Photon index (Γ) | 2.65 (+2.89 / −2.28) |
| DoF | 121 |
| p-value | 0.656 |
| 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.