5XMM J104028.4+091057
5XMM-DR15 stacked source · SRCID 3003854040100003
Position:
10h40m28.43s +09d10m57.7s
(160.11846°, 9.18268°)
EP flux
2.24e-14
± 3.4e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.85)
Detections
2
| SRCID | 3003854040100003 |
|---|---|
| IAUNAME | 5XMM J104028.4+091057 |
| SC_RA | 10h40m28.43s (160.11846°) |
| SC_DEC | +09d10m57.7s (9.18268°) |
| RADEC_ERR | 0.68 arcsec |
| LII / BII | 236.8319° / 54.2686° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52238.172 (2001-11-25 04:08:12.000 UTC) |
| MJD_LAST | 53350.123 (2004-12-11 02:57:37.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.24e-14 ± 3.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.34
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.07
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.71
± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.67
± 0.23
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 10.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 3.88
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
- 2920731
- Match probability
- 0.999
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | 20.066 | 0.073 |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.06e-14 (+2.4e-14 / −1.7e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.49e+20 (+7.6e+20 / −3.1e+19) cm−2 |
| Photon index (Γ) | 2.22 (+2.56 / −2.02) |
| DoF | 321 |
| p-value | 0.082 |
| Inter-instrument norm. | 1.47 (1.19–1.77) |
| 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.