5XMM J163250.2-475506
5XMM-DR15 stacked source · SRCID 3002214010100184
Position:
16h32m50.21s -47d55m06.4s
(248.20919°, -47.91845°)
EP flux
2.53e-15
± 2.7e-15
erg cm-2 s-1
CLASSX
Star
(0.98)
Detections
13
| SRCID | 3002214010100184 |
|---|---|
| IAUNAME | 5XMM J163250.2-475506 |
| SC_RA | 16h32m50.21s (248.20919°) |
| SC_DEC | -47d55m06.4s (-47.91845°) |
| RADEC_ERR | 1.90 arcsec |
| LII / BII | 336.3897° / 0.0400° |
| N_CONTRIB | 13 (detections) |
| N_OBS | 17 (observations covering the position) |
| MJD_FIRST | 51965.565 (2001-02-25 13:33:07.000 UTC) |
| MJD_LAST | 54726.150 (2008-09-17 03:35:25.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 2.53e-15 ± 2.7e-15 erg cm-2 s-1
Hardness ratios
HR1
0.84
± 1.25
0.2-0.5 / 0.5-1.0 keV
HR2
0.60
± 0.50
0.5-1.0 / 1.0-2.0 keV
HR3
-0.10
± 0.43
1.0-2.0 / 2.0-4.5 keV
HR4
0.32
± 0.40
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 1.2)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 6.19
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
- 4228965
- Match probability
- 0.805
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 20.926 | 0.102 |
| B | 18.981 | 0.033 |
| V | 19.334 | 0.149 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 9.81e-14 (+1.2e-13 / −8.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 8.66e+22 (+1.1e+23 / −6.7e+22) cm−2 |
| Photon index (Γ) | 2.44 (+2.85 / −1.83) |
| DoF | 90 |
| p-value | 0.66 |
| 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.