5XMM J101901.8+412141

5XMM-DR15 stacked source · SRCID 3002874030100020
Position: 10h19m01.85s +41d21m41.9s (154.75771°, 41.36165°)
EP flux
3.41e-14 ± 6.4e-15 erg cm-2 s-1
CLASSX
AGN (0.934)
Detections
1

SRCID 3002874030100020
IAUNAME 5XMM J101901.8+412141
SC_RA 10h19m01.85s (154.75771°)
SC_DEC +41d21m41.9s (41.36165°)
RADEC_ERR 0.75 arcsec
LII / BII 178.3905° / 55.7883°
N_CONTRIB 1 (detections)
N_OBS 1 (observations covering the position)
MJD_FIRST 52215.969 (2001-11-02 23:15:02.000 UTC)
MJD_LAST 52216.312 (2001-11-03 07:28:39.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.41e-14 ± 6.4e-15 erg cm-2 s-1

Hardness ratios
HR1
0.36 ± 0.12
0.2-0.5 / 0.5-1.0 keV
HR2
0.11 ± 0.10
0.5-1.0 / 1.0-2.0 keV
HR3
-0.40 ± 0.11
1.0-2.0 / 2.0-4.5 keV
HR4
-0.39 ± 0.17
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.4) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: -0.539

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
2866193
Match probability
0.988
FilterMag (AB)Err
UVW2
UVM2
UVW1
U 20.769 0.133
B
V 19.789 0.200

Spectroscopic (zsp) 0.14900
Photometric (TPZ) 1.5756 (conf 0.45)
Photometric (Le Phare) 1.4920 (conf 0.67)

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

Stacked power-law fit
Unabsorbed flux 2.71e-14 (+3.3e-14 / −2.3e-14) erg cm−2 s−1
NH 1.99e+21 (+3.0e+21 / −8.6e+20) cm−2
Photon index (Γ) 2.50 (+2.83 / −2.05)
DoF 94
p-value 0.789
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

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