5XMM J052451.4-333648
5XMM-DR15 stacked source · SRCID 3005015010100035
Position:
05h24m51.48s -33d36m48.0s
(81.21451°, -33.61334°)
EP flux
9.07e-15
± 3.3e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.478)
Detections
10
| SRCID | 3005015010100035 |
|---|---|
| IAUNAME | 5XMM J052451.4-333648 |
| SC_RA | 05h24m51.48s (81.21451°) |
| SC_DEC | -33d36m48.0s (-33.61334°) |
| RADEC_ERR | 0.66 arcsec |
| LII / BII | 237.4228° / -31.7229° |
| N_CONTRIB | 10 (detections) |
| N_OBS | 10 (observations covering the position) |
| MJD_FIRST | 51951.717 (2001-02-11 17:11:57.000 UTC) |
| MJD_LAST | 59974.211 (2023-01-30 05:03:40.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 9.07e-15 ± 3.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.40
± 0.31
0.2-0.5 / 0.5-1.0 keV
HR2
0.57
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.30
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
-0.48
± 0.33
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.
Bkg_AGN
CLASSX outlier: 1.97
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
- 1610118
- Match probability
- 0.995
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 21.813 | 0.322 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.99e-14 (+3.0e-14 / −1.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.34e+21 (+1.2e+22 / −2.8e+20) cm−2 |
| Photon index (Γ) | 1.56 (+2.35 / −1.13) |
| DoF | 49 |
| p-value | 0.38 |
| 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.