5XMM J043643.1+004029
5XMM-DR15 stacked source · SRCID 3004234160100026
Position:
04h36m43.10s +00d40m29.9s
(69.17960°, 0.67498°)
EP flux
1.45e-14
± 1.2e-14
erg cm-2 s-1
CLASSX
Star
(0.997)
Detections
2
| SRCID | 3004234160100026 |
|---|---|
| IAUNAME | 5XMM J043643.1+004029 |
| SC_RA | 04h36m43.10s (69.17960°) |
| SC_DEC | +00d40m29.9s (0.67498°) |
| RADEC_ERR | 1.48 arcsec |
| LII / BII | 195.3708° / -29.2183° |
| 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): 1.45e-14 ± 1.2e-14 erg cm-2 s-1
Hardness ratios
HR1
0.05
± 0.19
0.2-0.5 / 0.5-1.0 keV
HR2
-0.78
± 0.24
0.5-1.0 / 1.0-2.0 keV
HR3
-0.26
± 0.79
1.0-2.0 / 2.0-4.5 keV
HR4
0.04
± 1.20
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.7)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 3.91
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
- 1078171
- Match probability
- 0.982
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 19.794 | 0.085 |
| U | — | — |
| B | — | — |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 2.16e-14 (+3.1e-14 / −1.5e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.29e+20 (+1.0e+21 / −2.9e+19) cm−2 |
| Photon index (Γ) | 2.36 (+2.78 / −1.92) |
| DoF | 47 |
| p-value | 0.91 |
| 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.