5XMM J043730.8+005305
5XMM-DR15 stacked source · SRCID 3004234160100006
Position:
04h37m30.85s +00d53m05.9s
(69.37853°, 0.88497°)
EP flux
2.12e-13
± 3.2e-14
erg cm-2 s-1
CLASSX
AGN
(0.801)
Detections
2
| SRCID | 3004234160100006 |
|---|---|
| IAUNAME | 5XMM J043730.8+005305 |
| SC_RA | 04h37m30.85s (69.37853°) |
| SC_DEC | +00d53m05.9s (0.88497°) |
| RADEC_ERR | 0.39 arcsec |
| LII / BII | 195.2874° / -28.9384° |
| N_CONTRIB | 2 (detections) |
| N_OBS | 2 (observations covering the position) |
| MJD_FIRST | 52524.666 (2002-09-07 15:59:45.000 UTC) |
| MJD_LAST | 53069.965 (2004-03-05 23:09:19.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.12e-13 ± 3.2e-14 erg cm-2 s-1
Hardness ratios
HR1
0.38
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
0.15
± 0.06
0.5-1.0 / 1.0-2.0 keV
HR3
-0.39
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.26
± 0.15
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.9)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.729
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 | 1.28e-13 (+1.5e-13 / −1.1e-13) erg cm−2 s−1 |
|---|---|
| NH | 1.00e+21 (+1.6e+21 / −3.8e+20) cm−2 |
| Photon index (Γ) | 2.24 (+2.58 / −1.90) |
| DoF | 319 |
| p-value | 0.952 |
| Inter-instrument norm. | 0.95 (0.83–1.10) |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 31.400 (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.