5XMM J144228.5+352144

5XMM-DR15 stacked source · SRCID 3000501010100091
Position: 14h42m28.57s +35d21m44.0s (220.61905°, 35.36223°)
EP flux
2.50e-15 ± 1.8e-15 erg cm-2 s-1
CLASSX
AGN (0.908)
Detections
5

SRCID 3000501010100091
IAUNAME 5XMM J144228.5+352144
SC_RA 14h42m28.57s (220.61905°)
SC_DEC +35d21m44.0s (35.36223°)
RADEC_ERR 1.25 arcsec
LII / BII 59.0240° / 64.9799°
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): 2.50e-15 ± 1.8e-15 erg cm-2 s-1

Hardness ratios
HR1
0.21 ± 0.24
0.2-0.5 / 0.5-1.0 keV
HR2
0.20 ± 0.18
0.5-1.0 / 1.0-2.0 keV
HR3
-0.52 ± 0.20
1.0-2.0 / 2.0-4.5 keV
HR4
0.18 ± 0.38
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.5) SUM_FLAG: 2
Long-term lightcurve

AGN

CLASSX outlier: -0.524

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
3752292
Match probability
0.997
FilterMag (AB)Err
UVW2 20.525 0.110
UVM2
UVW1
U
B
V
CLASSOPT
Class
QSO
Star
0.00
AGN
1.00
Galaxy
0.00

Photometric (TPZ) 0.8758 (conf 0.36)
Photometric (Le Phare) 0.8066 (conf 0.19)

Spectroscopic redshifts (when present) are the most reliable. Photometric estimates carry a per-algorithm confidence flag.

Automated spectral fits are not yet available for this source. Interactive fitting on individual observations will be available from the contributing detections table soon.

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

The per-observation light curve is shown in the X-ray properties section above.