5XMM J011416.9-731851
5XMM-DR15 stacked source · SRCID 3001145010100462
Position:
01h14m16.97s -73d18m51.5s
(18.57073°, -73.31432°)
EP flux
4.80e-14
± 7.3e-15
erg cm-2 s-1
CLASSX
AGN
(0.937)
Detections
10
| SRCID | 3001145010100462 |
|---|---|
| IAUNAME | 5XMM J011416.9-731851 |
| SC_RA | 01h14m16.97s (18.57073°) |
| SC_DEC | -73d18m51.5s (-73.31432°) |
| RADEC_ERR | 0.39 arcsec |
| LII / BII | 300.6664° / -43.7133° |
| N_CONTRIB | 10 (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): 4.80e-14 ± 7.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.85
± 0.11
0.2-0.5 / 0.5-1.0 keV
HR2
0.65
± 0.05
0.5-1.0 / 1.0-2.0 keV
HR3
-0.19
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.42
± 0.12
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.7)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.527
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 | 3.65e-14 (+4.3e-14 / −3.1e-14) erg cm−2 s−1 |
|---|---|
| NH | 4.45e+21 (+5.5e+21 / −3.2e+21) cm−2 |
| Photon index (Γ) | 1.85 (+2.12 / −1.58) |
| DoF | 204 |
| p-value | 0.901 |
| Inter-instrument norm. | 1.06 (0.87–1.28) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 9.100 (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.