5XMM J132639.2-620103
5XMM-DR15 stacked source · SRCID 3003614020100018
Position:
13h26m39.28s -62d01m03.1s
(201.66365°, -62.01753°)
EP flux
1.11e-14
± 3.0e-15
erg cm-2 s-1
CLASSX
Star
(0.999)
Detections
3
| SRCID | 3003614020100018 |
|---|---|
| IAUNAME | 5XMM J132639.2-620103 |
| SC_RA | 13h26m39.28s (201.66365°) |
| SC_DEC | -62d01m03.1s (-62.01753°) |
| RADEC_ERR | 0.60 arcsec |
| LII / BII | 307.0504° / 0.5723° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 52138.332 (2001-08-17 07:57:32.000 UTC) |
| MJD_LAST | 60137.811 (2023-07-12 19:28:20.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.11e-14 ± 3.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.92
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.59
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.87
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.49
± 0.53
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.4)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.72
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
- 3482462
- Match probability
- 0.975
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 17.621 | 0.051 |
| UVM2 | — | — |
| UVW1 | 14.859 | 0.007 |
| U | — | — |
| B | — | — |
| V | 11.806 | 0.001 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.24e-14 (+2.6e-14 / −1.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.93e+21 (+5.0e+21 / −3.0e+21) cm−2 |
| Photon index (Γ) | 2.71 (+2.92 / −2.40) |
| DoF | 362 |
| p-value | 0.555 |
| 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.