5XMM J010734.2-174013
5XMM-DR15 stacked source · SRCID 3002554010100011
Position:
01h07m34.29s -17d40m13.0s
(16.89289°, -17.67029°)
EP flux
4.19e-14
± 9.7e-15
erg cm-2 s-1
CLASSX
AGN
(0.955)
Detections
2
| SRCID | 3002554010100011 |
|---|---|
| IAUNAME | 5XMM J010734.2-174013 |
| SC_RA | 01h07m34.29s (16.89289°) |
| SC_DEC | -17d40m13.0s (-17.67029°) |
| RADEC_ERR | 0.66 arcsec |
| LII / BII | 145.2520° / -79.8358° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52086.507 (2001-06-26 12:10:14.000 UTC) |
| MJD_LAST | 58494.099 (2019-01-11 02:22:24.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.19e-14 ± 9.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.10
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
-0.01
± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37
± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.39
± 0.24
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.108
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
- 500359
- Match probability
- 0.986
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 19.243 | 0.063 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.75e-14 (+4.9e-14 / −2.9e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.54e+20 (+8.9e+20 / −2.3e+19) cm−2 |
| Photon index (Γ) | 1.94 (+2.25 / −1.69) |
| DoF | 127 |
| p-value | 0.882 |
| Inter-instrument norm. | 0.65 (0.55–0.82) |
| 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.