5XMM J004051.4-092817
5XMM-DR15 stacked source · SRCID 3006514010100104
Position:
00h40m51.44s -09d28m17.0s
(10.21433°, -9.47139°)
EP flux
1.77e-14
± 3.5e-15
erg cm-2 s-1
CLASSX
AGN
(0.947)
Detections
2
| SRCID | 3006514010100104 |
|---|---|
| IAUNAME | 5XMM J004051.4-092817 |
| SC_RA | 00h40m51.44s (10.21433°) |
| SC_DEC | -09d28m17.0s (-9.47139°) |
| RADEC_ERR | 0.62 arcsec |
| LII / BII | 114.3835° / -72.1673° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 8 (observations covering the position) |
| MJD_FIRST | 52281.557 (2002-01-07 13:21:35.000 UTC) |
| MJD_LAST | 57179.777 (2015-06-06 18:39:02.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.77e-14 ± 3.5e-15 erg cm-2 s-1
Hardness ratios
HR1
0.31
± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.10
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.45
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.43
± 0.20
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.642
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
- 111613
- Match probability
- 0.975
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 22.304 | 0.287 |
| U | — | — |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.63e-14 (+3.0e-14 / −2.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.46e+20 (+5.6e+20 / −3.1e+19) cm−2 |
| Photon index (Γ) | 1.77 (+1.96 / −1.62) |
| DoF | 210 |
| p-value | 0.889 |
| Inter-instrument norm. | 0.92 (0.76–1.10) |
| 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.