5XMM J144202.4+352638
5XMM-DR15 stacked source · SRCID 3000501010100018
Position:
14h42m02.45s +35d26m38.6s
(220.51019°, 35.44407°)
EP flux
6.12e-14
± 7.1e-15
erg cm-2 s-1
CLASSX
Extended
(1)
Detections
5
| SRCID | 3000501010100018 |
|---|---|
| IAUNAME | 5XMM J144202.4+352638 |
| SC_RA | 14h42m02.45s (220.51019°) |
| SC_DEC | +35d26m38.6s (35.44407°) |
| RADEC_ERR | 12.68 arcsec |
| LII / BII | 59.2560° / 65.0504° |
| N_CONTRIB | 5 (detections) |
| N_OBS | 5 (observations covering the position) |
| MJD_FIRST | 52266.013 (2001-12-23 00:19:14.000 UTC) |
| MJD_LAST | 57936.351 (2017-07-02 08:25:53.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.12e-14 ± 7.1e-15 erg cm-2 s-1
Hardness ratios
HR1
-0.10
± 0.08
0.2-0.5 / 0.5-1.0 keV
HR2
0.16
± 0.07
0.5-1.0 / 1.0-2.0 keV
HR3
-0.56
± 0.07
1.0-2.0 / 2.0-4.5 keV
HR4
-0.19
± 0.16
2.0-4.5 / 4.5-12.0 keV
Extent:
22.85
± 1.36
arcsec
(ML 201.9)
SUM_FLAG:
4
Long-term lightcurve
No light-curve points available.
Extended
CLASSX outlier: 1.57
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
- 3750801
- Match probability
- 0.925
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | — | — |
| B | — | — |
| V | 14.316 | 0.006 |
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 1.52e-14 (+1.7e-14 / −1.4e-14) erg cm−2 s−1 |
|---|---|
| NH | 2.60e+19 (+7.3e+19 / −1.3e+19) cm−2 |
| Photon index (Γ) | 2.37 (+2.49 / −2.24) |
| DoF | 527 |
| p-value | 0.08 |
| 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.