5XMM J001354.8-302040
5XMM-DR15 stacked source · SRCID 3004234010100069
Position:
00h13m54.89s -30d20m40.9s
(3.47870°, -30.34470°)
EP flux
7.20e-15
± 2.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.948)
Detections
2
| SRCID | 3004234010100069 |
|---|---|
| IAUNAME | 5XMM J001354.8-302040 |
| SC_RA | 00h13m54.89s (3.47870°) |
| SC_DEC | -30d20m40.9s (-30.34470°) |
| RADEC_ERR | 0.71 arcsec |
| LII / BII | 9.3608° / -81.1719° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52059.831 (2001-05-30 19:57:00.000 UTC) |
| MJD_LAST | 57011.090 (2014-12-20 02:09:28.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 7.20e-15 ± 2.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.31
± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.11
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.54
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
0.01
± 0.26
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.426
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
- 20259
- Match probability
- 0.956
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 21.590 | 0.145 |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.68e-15 (+8.3e-15 / −5.3e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.30e+20 (+8.3e+20 / −2.4e+19) cm−2 |
| Photon index (Γ) | 1.96 (+2.32 / −1.70) |
| DoF | 222 |
| p-value | 0.759 |
| 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.