5XMM J132802.4-620226
5XMM-DR15 stacked source · SRCID 3003614020100051
Position:
13h28m02.40s -62d02m26.3s
(202.01000°, -62.04065°)
EP flux
1.73e-14
± 1.0e-14
erg cm-2 s-1
CLASSX
Extragal_XRB
(0.3)
Detections
2
| SRCID | 3003614020100051 |
|---|---|
| IAUNAME | 5XMM J132802.4-620226 |
| SC_RA | 13h28m02.40s (202.01000°) |
| SC_DEC | -62d02m26.3s (-62.04065°) |
| RADEC_ERR | 1.02 arcsec |
| LII / BII | 307.2080° / 0.5268° |
| 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): 1.73e-14 ± 1.0e-14 erg cm-2 s-1
Hardness ratios
HR1
0.92
± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
0.32
± 0.16
0.5-1.0 / 1.0-2.0 keV
HR3
-0.19
± 0.17
1.0-2.0 / 2.0-4.5 keV
HR4
-0.34
± 0.37
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -1.8)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Extragal_XRB
CLASSX outlier: 5.88
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
- 3489645
- Match probability
- 0.937
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 20.349 | 0.133 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.10e-14 (+4.2e-14 / −2.3e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.16e+21 (+3.2e+21 / −6.0e+19) cm−2 |
| Photon index (Γ) | 1.79 (+2.39 / −1.36) |
| DoF | 63 |
| p-value | 0.857 |
| 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.