5XMM J005946.9-720057
5XMM-DR15 stacked source · SRCID 3001854010100319
Position:
00h59m46.94s -72d00m57.4s
(14.94558°, -72.01593°)
EP flux
2.24e-14
± 2.3e-15
erg cm-2 s-1
CLASSX
AGN
(0.768)
Detections
15
| SRCID | 3001854010100319 |
|---|---|
| IAUNAME | 5XMM J005946.9-720057 |
| SC_RA | 00h59m46.94s (14.94558°) |
| SC_DEC | -72d00m57.4s (-72.01593°) |
| RADEC_ERR | 0.33 arcsec |
| LII / BII | 302.0196° / -45.0975° |
| N_CONTRIB | 15 (detections) |
| N_OBS | 182 (observations covering the position) |
| MJD_FIRST | 51834.632 (2000-10-17 15:10:35.000 UTC) |
| MJD_LAST | 57725.009 (2016-12-03 00:13:40.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.24e-14 ± 2.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.64
± 0.06
0.2-0.5 / 0.5-1.0 keV
HR2
0.18
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.43
± 0.06
1.0-2.0 / 2.0-4.5 keV
HR4
-0.50
± 0.11
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.9)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 0.608
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 | 1.91e-14 (+2.5e-14 / −1.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.61e+20 (+1.2e+21 / −3.4e+19) cm−2 |
| Photon index (Γ) | 1.85 (+2.25 / −1.56) |
| DoF | 164 |
| p-value | 0.719 |
| Inter-instrument norm. | 1.27 (0.97–1.61) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 20.000 (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.