5XMM J233955.9-121951
5XMM-DR15 stacked source · SRCID 3005599030100008
Position:
23h39m55.90s -12d19m51.3s
(354.98290°, -12.33093°)
EP flux
6.08e-14
± 7.8e-15
erg cm-2 s-1
CLASSX
AGN
(0.841)
Detections
1
| SRCID | 3005599030100008 |
|---|---|
| IAUNAME | 5XMM J233955.9-121951 |
| SC_RA | 23h39m55.90s (354.98290°) |
| SC_DEC | -12d19m51.3s (-12.33093°) |
| RADEC_ERR | 0.49 arcsec |
| LII / BII | 70.8841° / -67.6469° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 1 (observations covering the position) |
| MJD_FIRST | 52241.584 (2001-11-28 14:00:26.000 UTC) |
| MJD_LAST | 52241.750 (2001-11-28 17:59:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.08e-14 ± 7.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.09
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.11
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.22
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.30
± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 2.02
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
- 6612262
- Match probability
- 0.971
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 21.128 | 0.158 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.64e-14 (+4.2e-14 / −3.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.80e+19 (+2.9e+20 / −2.2e+19) cm−2 |
| Photon index (Γ) | 1.97 (+2.16 / −1.81) |
| DoF | 113 |
| p-value | 0.61 |
| 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.