5XMM J011915.1-733053
5XMM-DR15 stacked source · SRCID 3001145010100771
Position:
01h19m15.10s -73d30m53.8s
(19.81291°, -73.51495°)
EP flux
2.06e-14
± 3.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.963)
Detections
16
| SRCID | 3001145010100771 |
|---|---|
| IAUNAME | 5XMM J011915.1-733053 |
| SC_RA | 01h19m15.10s (19.81291°) |
| SC_DEC | -73d30m53.8s (-73.51495°) |
| RADEC_ERR | 0.48 arcsec |
| LII / BII | 300.2189° / -43.4665° |
| N_CONTRIB | 16 (detections) |
| N_OBS | 182 (observations covering the position) |
| MJD_FIRST | 52060.097 (2001-05-31 02:20:10.000 UTC) |
| MJD_LAST | 59708.768 (2022-05-09 18:26:09.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.06e-14 ± 3.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.71
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.33
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.34
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.47
± 0.15
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.0204
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.
No multi-wavelength counterpart data available for this source.
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.98e-14 (+2.8e-14 / −1.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.08e+21 (+3.1e+21 / −6.5e+19) cm−2 |
| Photon index (Γ) | 1.70 (+2.37 / −1.31) |
| DoF | 393 |
| p-value | 0.604 |
| Inter-instrument norm. | 0.85 (0.63–1.15) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 6.700 (approximate flux variability amplitude) |
|---|
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.