5XMM J105247.9+572116
5XMM-DR15 stacked source · SRCID 3002274010100021
Position:
10h52m47.94s +57d21m16.5s
(163.19973°, 57.35459°)
EP flux
3.04e-14
± 1.5e-15
erg cm-2 s-1
CLASSX
Bkg_AGN
(0.406)
Detections
16
| SRCID | 3002274010100021 |
|---|---|
| IAUNAME | 5XMM J105247.9+572116 |
| SC_RA | 10h52m47.94s (163.19973°) |
| SC_DEC | +57d21m16.5s (57.35459°) |
| RADEC_ERR | 0.11 arcsec |
| LII / BII | 149.4214° / 53.2392° |
| N_CONTRIB | 16 (detections) |
| N_OBS | 21 (observations covering the position) |
| MJD_FIRST | 51661.158 (2000-04-27 03:47:47.000 UTC) |
| MJD_LAST | 52615.196 (2002-12-07 04:41:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 3.04e-14 ± 1.5e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.19
± 0.02
0.2-0.5 / 0.5-1.0 keV
HR2
-0.11
± 0.02
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37
± 0.03
1.0-2.0 / 2.0-4.5 keV
HR4
-0.57
± 0.07
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML 141.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Bkg_AGN
CLASSX outlier: 1.25
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
- 2958473
- Match probability
- 0.999
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | 20.690 | 0.040 |
| UVM2 | 20.613 | 0.036 |
| UVW1 | 20.653 | 0.025 |
| U | 20.700 | 0.022 |
| B | 20.421 | 0.030 |
| V | 20.145 | 0.088 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 3.29e-14 (+3.6e-14 / −3.0e-14) erg cm−2 s−1 |
|---|---|
| NH | 3.46e+19 (+1.1e+20 / −1.5e+19) cm−2 |
| Photon index (Γ) | 2.28 (+2.40 / −2.17) |
| DoF | 230 |
| p-value | 0.085 |
| Quality flag | 0 |
| APPROX_SOURCE_VAR | 14.800 (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.