5XMM J073913.3+703138
5XMM-DR15 stacked source · SRCID 3002854020100019
Position:
07h39m13.38s +70d31m38.4s
(114.80575°, 70.52733°)
EP flux
1.21e-14
± 2.9e-15
erg cm-2 s-1
CLASSX
Star
(1)
Detections
3
| SRCID | 3002854020100019 |
|---|---|
| IAUNAME | 5XMM J073913.3+703138 |
| SC_RA | 07h39m13.38s (114.80575°) |
| SC_DEC | +70d31m38.4s (70.52733°) |
| RADEC_ERR | 0.62 arcsec |
| LII / BII | 144.9221° / 29.4270° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52171.579 (2001-09-19 13:53:26.000 UTC) |
| MJD_LAST | 52578.796 (2002-10-31 19:06:04.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 1.21e-14 ± 2.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.66
± 0.07
0.2-0.5 / 0.5-1.0 keV
HR2
-0.32
± 0.08
0.5-1.0 / 1.0-2.0 keV
HR3
-0.88
± 0.08
1.0-2.0 / 2.0-4.5 keV
HR4
-0.12
± 0.49
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.5)
SUM_FLAG:
0
Long-term lightcurve
No light-curve points available.
Star
CLASSX outlier: 1.56
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
- 2403621
- Match probability
- 0.957
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | 14.622 | 0.002 |
| U | — | — |
| B | — | — |
| V | 12.309 | 0.001 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.09e-14 (+1.3e-14 / −9.2e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.30e+21 (+1.8e+21 / −6.8e+20) cm−2 |
| Photon index (Γ) | 2.84 (+2.95 / −2.59) |
| DoF | 507 |
| p-value | 0.476 |
| Inter-instrument norm. | 1.23 (0.96–1.52) |
| 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.