5XMM J011537.4-733808
5XMM-DR15 stacked source · SRCID 3001145010101044
Position:
01h15m37.45s -73d38m08.5s
(18.90605°, -73.63570°)
EP flux
1.50e-14
± 2.6e-15
erg cm-2 s-1
CLASSX
AGN
(0.929)
Detections
16
| SRCID | 3001145010101044 |
|---|---|
| IAUNAME | 5XMM J011537.4-733808 |
| SC_RA | 01h15m37.45s (18.90605°) |
| SC_DEC | -73d38m08.5s (-73.63570°) |
| RADEC_ERR | 0.58 arcsec |
| LII / BII | 300.5916° / -43.3825° |
| 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): 1.50e-14 ± 2.6e-15 erg cm-2 s-1
Hardness ratios
HR1
0.74
± 0.09
0.2-0.5 / 0.5-1.0 keV
HR2
0.35
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.36
± 0.09
1.0-2.0 / 2.0-4.5 keV
HR4
-0.49
± 0.16
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.
AGN
CLASSX outlier: -0.648
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 | 1.85e-14 (+2.3e-14 / −1.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 1.42e+21 (+2.9e+21 / −2.0e+20) cm−2 |
| Photon index (Γ) | 1.62 (+2.11 / −1.22) |
| DoF | 153 |
| p-value | 0.085 |
| Inter-instrument norm. | 1.85 (1.66–1.97) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 5.600 (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.