5XMM J001347.3-302146
5XMM-DR15 stacked source · SRCID 3004234010100021
Position:
00h13m47.33s -30d21m46.4s
(3.44721°, -30.36288°)
EP flux
5.14e-14
± 4.4e-15
erg cm-2 s-1
CLASSX
AGN
(0.918)
Detections
2
| SRCID | 3004234010100021 |
|---|---|
| IAUNAME | 5XMM J001347.3-302146 |
| SC_RA | 00h13m47.33s (3.44721°) |
| SC_DEC | -30d21m46.4s (-30.36288°) |
| RADEC_ERR | 0.26 arcsec |
| LII / BII | 9.3068° / -81.1403° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52059.831 (2001-05-30 19:57:00.000 UTC) |
| MJD_LAST | 57011.090 (2014-12-20 02:09:28.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 5.14e-14 ± 4.4e-15 erg cm-2 s-1
Hardness ratios
HR1
0.53
± 0.05
0.2-0.5 / 0.5-1.0 keV
HR2
0.11
± 0.04
0.5-1.0 / 1.0-2.0 keV
HR3
-0.20
± 0.04
1.0-2.0 / 2.0-4.5 keV
HR4
-0.28
± 0.08
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -3.3)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.0212
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 | 3.80e-14 (+4.1e-14 / −3.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 6.02e+20 (+9.1e+20 / −2.8e+20) cm−2 |
| Photon index (Γ) | 1.74 (+1.87 / −1.61) |
| DoF | 692 |
| p-value | 0.968 |
| Inter-instrument norm. | 1.01 (0.92–1.10) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 7.300 (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.