5XMM J132659.8-620149
5XMM-DR15 stacked source · SRCID 3003614020100009
Position:
13h26m59.82s -62d01m49.4s
(201.74926°, -62.03038°)
EP flux
4.26e-14
± 4.4e-15
erg cm-2 s-1
CLASSX
Star
(0.992)
Detections
2
| SRCID | 3003614020100009 |
|---|---|
| IAUNAME | 5XMM J132659.8-620149 |
| SC_RA | 13h26m59.82s (201.74926°) |
| SC_DEC | -62d01m49.4s (-62.03038°) |
| RADEC_ERR | 0.34 arcsec |
| LII / BII | 307.0884° / 0.5541° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 4 (observations covering the position) |
| MJD_FIRST | 52138.332 (2001-08-17 07:57:32.000 UTC) |
| MJD_LAST | 52668.955 (2003-01-29 22:55:00.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.26e-14 ± 4.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.79
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.71
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.55
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.83
± 0.10
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.0)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 4.17
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
- 3484818
- Match probability
- 0.99
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 17.390 | 0.046 |
| UVM2 | — | — |
| UVW1 | 14.634 | 0.007 |
| U | — | — |
| B | — | — |
| V | 11.603 | 0.001 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.33e-14 (+5.9e-14 / −4.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 7.52e+21 (+8.4e+21 / −6.6e+21) cm−2 |
| Photon index (Γ) | 2.91 (+2.98 / −2.78) |
| DoF | 167 |
| p-value | 0.138 |
| 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.