5XMM J103751.9+415414

5XMM-DR15 stacked source · SRCID 3004694010100020
Position: 10h37m51.90s +41d54m14.2s (159.46625°, 41.90394°)
EP flux
1.33e-14 ± 5.5e-15 erg cm-2 s-1
CLASSX
AGN (0.828)
Detections
2

SRCID 3004694010100020
IAUNAME 5XMM J103751.9+415414
SC_RA 10h37m51.90s (159.46625°)
SC_DEC +41d54m14.2s (41.90394°)
RADEC_ERR 0.89 arcsec
LII / BII 175.7199° / 59.0459°
N_CONTRIB 2 (detections)
N_OBS 2 (observations covering the position)
MJD_FIRST 52040.539 (2001-05-11 12:55:30.000 UTC)
MJD_LAST 53119.856 (2004-04-24 20:32:49.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.33e-14 ± 5.5e-15 erg cm-2 s-1

Hardness ratios
HR1
0.14 ± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
-0.12 ± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.37 ± 0.18
1.0-2.0 / 2.0-4.5 keV
HR4
-0.97 ± 0.52
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -2.1) SUM_FLAG: 1
Long-term lightcurve

AGN

CLASSX outlier: 1.02

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
2909858
Match probability
0.996
FilterMag (AB)Err
UVW2 — —
UVM2 — —
UVW1 20.410 0.061
U 20.301 0.067
B 20.164 0.088
V — —

Spectroscopic (zsp) 1.78600
Photometric (TPZ) 1.9255 (conf 0.87)
Photometric (Le Phare) 1.9520 (conf 0.98)

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

Stacked power-law fit
Unabsorbed flux 2.76e-14 (+3.6e-14 / −2.0e-14) erg cm−2 s−1
NH 2.15e+20 (+8.4e+20 / −2.5e+19) cm−2
Photon index (Γ) 2.14 (+2.54 / −1.85)
DoF 298
p-value 0.351
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.