5XMM J163341.5+571411
5XMM-DR15 stacked source · SRCID 3004954010100074
Position:
16h33m41.50s +57d14m11.6s
(248.42291°, 57.23655°)
EP flux
4.73e-14
± 1.1e-14
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
6
| SRCID | 3004954010100074 |
|---|---|
| IAUNAME | 5XMM J163341.5+571411 |
| SC_RA | 16h33m41.50s (248.42291°) |
| SC_DEC | +57d14m11.6s (57.23655°) |
| RADEC_ERR | 1.90 arcsec |
| LII / BII | 86.6880° / 40.9807° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 6 (observations covering the position) |
| MJD_FIRST | 52208.338 (2001-10-26 08:07:10.000 UTC) |
| MJD_LAST | 53674.442 (2005-10-31 10:36:41.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 4.73e-14 ± 1.1e-14 erg cm-2 s-1
Hardness ratios
HR1
0.46
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.39
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.80
± 0.13
1.0-2.0 / 2.0-4.5 keV
HR4
0.71
± 0.20
2.0-4.5 / 4.5-12.0 keV
Extent:
14.88
± 1.17
arcsec
(ML 79.7)
SUM_FLAG:
2
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 2.28
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.
Optical Monitor (OM)
- OM Source ID
- 4236057
- Match probability
- 0.711
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.277 | 0.164 |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.04e-15 (+1.1e-14 / −6.0e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.25e+20 (+6.0e+20 / −2.3e+19) cm−2 |
| Photon index (Γ) | 2.53 (+2.85 / −2.17) |
| DoF | 155 |
| p-value | 0.34 |
| Quality flag | 0 |
No variability data available for this source.
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.