5XMM J144903.1+090235
5XMM-DR15 stacked source · SRCID 3005756030100049
Position:
14h49m03.12s +09d02m35.5s
(222.26300°, 9.04319°)
EP flux
7.34e-15
± 1.9e-15
erg cm-2 s-1
CLASSX
AGN
(0.907)
Detections
3
| SRCID | 3005756030100049 |
|---|---|
| IAUNAME | 5XMM J144903.1+090235 |
| SC_RA | 14h49m03.12s (222.26300°) |
| SC_DEC | +09d02m35.5s (9.04319°) |
| RADEC_ERR | 0.68 arcsec |
| LII / BII | 5.4299° / 56.8641° |
| N_CONTRIB | 3 (detections) |
| N_OBS | 3 (observations covering the position) |
| MJD_FIRST | 52130.132 (2001-08-09 03:10:43.000 UTC) |
| MJD_LAST | 52868.447 (2003-08-17 10:44:11.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 7.34e-15 ± 1.9e-15 erg cm-2 s-1
Hardness ratios
HR1
0.07
± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.21
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.24
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.73
± 0.25
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -2.1)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: -0.858
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
- 3781499
- Match probability
- 0.817
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.168 | 0.164 |
| B | 21.866 | 0.212 |
| V | — | — |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 6.21e-15 (+8.5e-15 / −4.6e-15) erg cm−2 s−1 |
|---|---|
| NH | 1.38e+20 (+7.7e+20 / −2.3e+19) cm−2 |
| Photon index (Γ) | 2.13 (+2.48 / −1.79) |
| DoF | 127 |
| p-value | 0.69 |
| Inter-instrument norm. | 1.23 (0.85–1.62) |
| 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.