5XMM J174804.5-281457

5XMM-DR15 stacked source · SRCID 3003054010108651
Position: 17h48m04.55s -28d14m57.3s (267.01896°, -28.24924°)
EP flux
1.23e-14 ± 2.0e-15 erg cm-2 s-1
CLASSX
Star (0.41)
Detections
14

SRCID 3003054010108651
IAUNAME 5XMM J174804.5-281457
SC_RA 17h48m04.55s (267.01896°)
SC_DEC -28d14m57.3s (-28.24924°)
RADEC_ERR 0.68 arcsec
LII / BII 0.8669° / -0.1044°
N_CONTRIB 14 (detections)
N_OBS 308 (observations covering the position)
MJD_FIRST 51810.719 (2000-09-23 17:14:57.000 UTC)
MJD_LAST 59127.048 (2020-10-05 01:09:24.000 UTC)

Stacked EPIC flux

EP flux (0.2-12 keV): 1.23e-14 ± 2.0e-15 erg cm-2 s-1

Hardness ratios
HR1
0.60 ± 0.14
0.2-0.5 / 0.5-1.0 keV
HR2
0.45 ± 0.09
0.5-1.0 / 1.0-2.0 keV
HR3
-0.04 ± 0.10
1.0-2.0 / 2.0-4.5 keV
HR4
-0.13 ± 0.14
2.0-4.5 / 4.5-12.0 keV
Extent: 0.00 arcsec (ML -1.9) SUM_FLAG: 3
Long-term lightcurve

Star

CLASSX outlier: 5.53

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
4893659
Match probability
0.732
FilterMag (AB)Err
UVW2
UVM2
UVW1
U
B 20.818 0.149
V
Gaia DR3
Source ID
4057626922187530240
Match probability
0.986
Parallax
0.576 ± 0.116 mas
Proper motion
(-3.67, -1.33) mas/yr
Magnitudes
G=17.26, BP=19.02, RP=15.98
CLASSOPT
Class
Star
Star
1.00
AGN
0.00
Galaxy
0.00

No redshift estimate available for this source.

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.