5XMM J001452.5-391224

5XMM-DR15 stacked source · SRCID 3002874010100173
Position: 00h14m52.56s -39d12m24.2s (3.71900°, -39.20673°)
EP flux
1.91e-15 ± 9.0e-16 erg cm-2 s-1
CLASSX
Extragal_XRB (0.499)
Detections
10

SRCID 3002874010100173
IAUNAME 5XMM J001452.5-391224
SC_RA 00h14m52.56s (3.71900°)
SC_DEC -39d12m24.2s (-39.20673°)
RADEC_ERR 0.77 arcsec
LII / BII 332.8697° / -75.7207°
N_CONTRIB 10 (detections)
N_OBS 10 (observations covering the position)
MJD_FIRST 52227.605 (2001-11-14 14:31:49.000 UTC)
MJD_LAST 59561.812 (2021-12-13 19:29:06.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.91e-15 ± 9.0e-16 erg cm-2 s-1

Hardness ratios
HR1
0.41 ± 0.47
0.2-0.5 / 0.5-1.0 keV
HR2
0.82 ± 0.14
0.5-1.0 / 1.0-2.0 keV
HR3
-0.42 ± 0.14
1.0-2.0 / 2.0-4.5 keV
HR4
-0.50 ± 0.36
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.5) SUM_FLAG: 1
Long-term lightcurve

Extragal_XRB

CLASSX outlier: 4.44

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
22545
Match probability
0.988
FilterMag (AB)Err
UVW2 18.155 0.035
UVM2 17.944 0.015
UVW1 18.072 0.004
U 16.818 0.014
B 18.797 0.048
V 18.201 0.064
Gaia DR3
Source ID
4998160133637833472
Match probability
0.976
Parallax
-0.273 ± 1.041 mas
Proper motion
(-0.61, -0.66) mas/yr
Magnitudes
G=20.47, BP=19.97, RP=19.60
CLASSOPT
Class
QSO
Star
0.01
AGN
0.74
Galaxy
0.25

No redshift estimate available for this source.

Stacked power-law fit
Unabsorbed flux 1.29e-14 (+1.6e-14 / −1.0e-14) erg cm−2 s−1
NH 4.20e+21 (+6.1e+21 / −2.1e+21) cm−2
Photon index (Γ) 2.34 (+2.75 / −1.81)
DoF 80
p-value 0.862
Quality flag 0

APPROX_SOURCE_VAR 13.900 (approximate flux variability amplitude)

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.