5XMM J022150.6-035246

5XMM-DR15 stacked source · SRCID 3003798010106154
Position: 02h21m50.69s -03d52m46.9s (35.46120°, -3.87969°)
EP flux
3.27e-15 ± 9.6e-16 erg cm-2 s-1
CLASSX
Bkg_AGN (0.661)
Detections
4

SRCID 3003798010106154
IAUNAME 5XMM J022150.6-035246
SC_RA 02h21m50.69s (35.46120°)
SC_DEC -03d52m46.9s (-3.87969°)
RADEC_ERR 1.10 arcsec
LII / BII 169.7554° / -58.2776°
N_CONTRIB 4 (detections)
N_OBS 372 (observations covering the position)
MJD_FIRST 52285.186 (2002-01-11 04:27:23.000 UTC)
MJD_LAST 57757.972 (2017-01-04 23:19:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 3.27e-15 ± 9.6e-16 erg cm-2 s-1

Hardness ratios
HR1
0.43 ± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
-0.29 ± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.82 ± 0.17
1.0-2.0 / 2.0-4.5 keV
HR4
-0.87 ± 1.34
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.7) SUM_FLAG: 1
Long-term lightcurve

Bkg_AGN

CLASSX outlier: 2.01

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
790394
Match probability
0.959
FilterMag (AB)Err
UVW2
UVM2 18.348 0.033
UVW1 18.217 0.010
U 18.100 0.014
B
V
Gaia DR3
Source ID
2489904421094963072
Match probability
0.987
Magnitudes
G=20.03, BP=17.63, RP=16.98
AllWISE
Name
J022150.80-035248.8
Match probability
0.995
BandMagErr
W1 14.499 0.030
W2 14.157 0.040
W3 10.267 0.060
W4 7.702 0.141
CLASSOPT
Class
Galaxy
Star
0.00
AGN
0.11
Galaxy
0.89

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 4.92e-15 (+7.5e-15 / −3.2e-15) erg cm−2 s−1
NH 6.19e+20 (+2.0e+21 / −4.2e+19) cm−2
Photon index (Γ) 2.28 (+2.77 / −1.74)
DoF 313
p-value 0.279
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.