5XMM J132722.2-615555
5XMM-DR15 stacked source · SRCID 3003614020100038
Position:
13h27m22.21s -61d55m55.2s
(201.84253°, -61.93199°)
EP flux
1.22e-14
± 4.8e-15
erg cm-2 s-1
CLASSX
Star
(0.999)
Detections
2
| SRCID | 3003614020100038 |
|---|---|
| IAUNAME | 5XMM J132722.2-615555 |
| SC_RA | 13h27m22.21s (201.84253°) |
| SC_DEC | -61d55m55.2s (-61.93199°) |
| RADEC_ERR | 0.86 arcsec |
| LII / BII | 307.1454° / 0.6454° |
| 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): 1.22e-14 ± 4.8e-15 erg cm-2 s-1
Hardness ratios
HR1
0.93
± 0.10
0.2-0.5 / 0.5-1.0 keV
HR2
0.10
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.60
± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.85
± 0.43
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.
Star
CLASSX outlier: 3.79
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
- 3487216
- Match probability
- 0.975
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 19.717 | 0.233 |
| UVM2 | — | — |
| UVW1 | 17.489 | 0.024 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.11e-14 (+2.7e-14 / −1.6e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.85e+21 (+4.2e+21 / −1.4e+21) cm−2 |
| Photon index (Γ) | 2.47 (+2.85 / −1.92) |
| DoF | 68 |
| p-value | 0.373 |
| 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.