5XMM J162743.9+393417
5XMM-DR15 stacked source · SRCID 3000803020100249
Position:
16h27m43.96s +39d34m17.7s
(246.93317°, 39.57158°)
EP flux
6.54e-15
± 2.3e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
6
| SRCID | 3000803020100249 |
|---|---|
| IAUNAME | 5XMM J162743.9+393417 |
| SC_RA | 16h27m43.96s (246.93317°) |
| SC_DEC | +39d34m17.7s (39.57158°) |
| RADEC_ERR | 0.70 arcsec |
| LII / BII | 62.9558° / 43.8684° |
| N_CONTRIB | 6 (detections) |
| N_OBS | 15 (observations covering the position) |
| MJD_FIRST | 52459.655 (2002-07-04 15:43:08.000 UTC) |
| MJD_LAST | 57815.752 (2017-03-03 18:02:28.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.54e-15 ± 2.3e-15 erg cm-2 s-1
Hardness ratios
HR1
0.71
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
-0.77
± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.71
± 0.31
1.0-2.0 / 2.0-4.5 keV
HR4
0.24
± 0.47
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.0)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 1.02
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
- 4193379
- Match probability
- 0.961
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 15.257 | 0.008 |
| U | — | — |
| B | 12.875 | 0.001 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.53e-14 (+1.9e-14 / −1.2e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.69e+20 (+1.1e+21 / −3.2e+19) cm−2 |
| Photon index (Γ) | 2.49 (+2.81 / −2.14) |
| DoF | 59 |
| p-value | 0.311 |
| 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.