5XMM J030511.6-774758
5XMM-DR15 stacked source · SRCID 3004234040100006
Position:
03h05m11.63s -77d47m58.4s
(46.29844°, -77.79956°)
EP flux
9.06e-14
± 4.7e-15
erg cm-2 s-1
CLASSX
AGN
(0.949)
Detections
4
| SRCID | 3004234040100006 |
|---|---|
| IAUNAME | 5XMM J030511.6-774758 |
| SC_RA | 03h05m11.63s (46.29844°) |
| SC_DEC | -77d47m58.4s (-77.79956°) |
| RADEC_ERR | 0.16 arcsec |
| LII / BII | 294.5408° / -37.0589° |
| N_CONTRIB | 4 (detections) |
| N_OBS | 5 (observations covering the position) |
| MJD_FIRST | 52032.765 (2001-05-03 18:21:36.000 UTC) |
| MJD_LAST | 59685.458 (2022-04-16 11:00:04.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.06e-14 ± 4.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.41
± 0.03
0.2-0.5 / 0.5-1.0 keV
HR2
0.03
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.31
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.44
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.8)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 1.37
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
- 908228
- Match probability
- 0.999
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.715 | 0.104 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.78e-14 (+7.3e-14 / −6.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.80e+20 (+1.0e+21 / −5.4e+20) cm−2 |
| Photon index (Γ) | 2.04 (+2.17 / −1.90) |
| DoF | 1102 |
| p-value | 0.805 |
| 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.