5XMM J172844.3-141834
5XMM-DR15 stacked source · SRCID 3004116010100041
Position:
17h28m44.33s -14d18m34.5s
(262.18470°, -14.30959°)
EP flux
1.56e-14
± 1.0e-15
erg cm-2 s-1
CLASSX
AGN
(0.505)
Detections
13
| SRCID | 3004116010100041 |
|---|---|
| IAUNAME | 5XMM J172844.3-141834 |
| SC_RA | 17h28m44.33s (262.18470°) |
| SC_DEC | -14d18m34.5s (-14.30959°) |
| RADEC_ERR | 0.21 arcsec |
| LII / BII | 10.4075° / 11.0562° |
| N_CONTRIB | 13 (detections) |
| N_OBS | 13 (observations covering the position) |
| MJD_FIRST | 51966.410 (2001-02-26 09:50:20.000 UTC) |
| MJD_LAST | 58751.667 (2019-09-25 16:00:27.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.56e-14 ± 1.0e-15 erg cm-2 s-1
Hardness ratios
HR1
0.93
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.60
± 0.03
0.5-1.0 / 1.0-2.0 keV
HR3
-0.12
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.45
± 0.05
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 3.3)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 2.4
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
- 4675703
- Match probability
- 0.524
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 19.890 | 0.194 |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.21e-14 (+2.5e-14 / −1.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.74e+21 (+6.6e+21 / −3.2e+21) cm−2 |
| Photon index (Γ) | 1.82 (+2.14 / −1.54) |
| DoF | 442 |
| p-value | 0.947 |
| Inter-instrument norm. | 0.90 (0.76–1.09) |
| 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.