5XMM J125325.3-292340
5XMM-DR15 stacked source · SRCID 3005774030100143
Position:
12h53m25.34s -29d23m40.5s
(193.35557°, -29.39459°)
EP flux
8.13e-15
± 2.4e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.937)
Detections
2
| SRCID | 3005774030100143 |
|---|---|
| IAUNAME | 5XMM J125325.3-292340 |
| SC_RA | 12h53m25.34s (193.35557°) |
| SC_DEC | -29d23m40.5s (-29.39459°) |
| RADEC_ERR | 0.91 arcsec |
| LII / BII | 303.4501° / 33.4752° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 14 (observations covering the position) |
| MJD_FIRST | 52642.080 (2003-01-03 01:54:58.000 UTC) |
| MJD_LAST | 52650.824 (2003-01-11 19:46:07.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 8.13e-15 ± 2.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.82
± 0.21
0.2-0.5 / 0.5-1.0 keV
HR2
0.37
± 0.13
0.5-1.0 / 1.0-2.0 keV
HR3
-0.06
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.50
± 0.21
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: 2.35
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
- 3320755
- Match probability
- 0.987
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.547 | 0.091 |
| U | 19.227 | 0.041 |
| B | 17.467 | 0.020 |
| V | 16.163 | 0.021 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.28e-15 (+8.6e-15 / −4.2e-15) erg cm−2 s−1 |
|---|---|
| NH | 2.44e+20 (+1.4e+21 / −2.3e+19) cm−2 |
| Photon index (Γ) | 1.39 (+1.86 / −1.14) |
| DoF | 75 |
| p-value | 0.447 |
| 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.