5XMM J182722.4-120731
5XMM-DR15 stacked source · SRCID 3005194020100178
Position:
18h27m22.48s -12d07m31.6s
(276.84368°, -12.12544°)
EP flux
5.77e-14
± 1.3e-14
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.353)
Detections
1
| SRCID | 3005194020100178 |
|---|---|
| IAUNAME | 5XMM J182722.4-120731 |
| SC_RA | 18h27m22.48s (276.84368°) |
| SC_DEC | -12d07m31.6s (-12.12544°) |
| RADEC_ERR | 0.78 arcsec |
| LII / BII | 19.4187° / -0.2629° |
| N_CONTRIB | 1 (detections) |
| N_OBS | 71 (observations covering the position) |
| MJD_FIRST | 51978.813 (2001-03-10 19:30:19.000 UTC) |
| MJD_LAST | 51978.919 (2001-03-10 22:02:48.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.77e-14 ± 1.3e-14 erg cm-2 s-1
Hardness ratios
HR1
0.96
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.48
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.44
± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.45
± 0.21
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 5.75
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
- 5411283
- Match probability
- 0.606
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 15.617 | 0.015 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 5.50e-14 (+6.8e-14 / −4.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.36e+21 (+6.0e+21 / −2.7e+21) cm−2 |
| Photon index (Γ) | 2.29 (+2.72 / −1.82) |
| DoF | 64 |
| p-value | 0.998 |
| 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.