Observation details report
Detailed source parameters (including errors) in a comma-separated values file
Click on source number for detailed analysis, including spectral fits if applicable
| data | idnum | idradec | telescope | instrument | x | y | cnts | cntserr | rate | rateerr | SNR | poisprob | sigmaj | sigmin | incang | offax | cnts_soft | cnts_hard | hr | hr_err | ext | var | N_H | flux | vign | flags | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Report | srcpi bgdpi arf rmf | 1 | X080335.14-400010.8 | xmm | mos1 | 306.639 | 281.924 | 30982.3 | 197.123 | 1.41956 | 0.0090319 | 349.125 | 1 | 5.76293 | 5.61642 | 356.831 | 1.33865 | F | T | 4.70544 | 1.01687e-11 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 1 | X080335.14-400010.6 | xmm | mos2 | 306.644 | 281.972 | 32924.8 | 204.782 | 1.42069 | 0.00883626 | 346.849 | 1 | 5.74766 | 5.31165 | 340.776 | 1.33417 | F | T | 4.70533 | 1.11503e-11 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 1 | X080347.52-395758.8 | xmm | pn | 273.943 | 312.28 | 200.766 | 25.5823 | 0.006736 | 0.000858324 | 2.63065 | 0.995627 | 5.63756 | 5.63756 | 0 | 2.02011 | F | T | 4.65253 | 1.91099e-14 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 2 | X080335.14-400011.2 | xmm | pn | 306.647 | 281.833 | 125888 | 389.215 | 4.22373 | 0.0130587 | 1649.52 | 1 | 5.99404 | 5.99404 | 0 | 1.34016 | F | F | 4.70545 | 1.35215e-11 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 3 | X080341.44-395724.0 | xmm | pn | 290.004 | 320.274 | 237.087 | 31.1399 | 0.00795463 | 0.00104479 | 3.10657 | 0.998992 | 10.8575 | 10.8575 | 0 | 1.66787 | F | F | 4.66425 | 3.28965e-14 | 1 | dscx | ||||
| Report | srcpi bgdpi arf rmf | 4 | X080340.53-395748.7 | xmm | pn | 292.404 | 314.591 | 398.883 | 30.8293 | 0.0133831 | 0.00103437 | 5.22659 | 1 | 14.525 | 14.525 | 0 | 1.27962 | T | F | 4.66919 | 5.14742e-14 | 1 | dscx | ||||
| Report | srcpi bgdpi arf rmf | 5 | X080338.04-395858.1 | xmm | pn | 298.996 | 298.649 | 725.961 | 50.1025 | 0.0243571 | 0.00168102 | 9.51232 | 1 | 14.9002 | 14.9002 | 0 | 0.891184 | T | F | 4.67437 | 8.98287e-14 | 1 | dsbx | ||||
| Report | srcpi bgdpi arf | 7 | X080342.21-395702.0 | xmm | pn | 287.957 | 324.596 | 173.634 | 18.1991 | 0.0104561 | 0.00109593 | 2.27514 | 0.98845 | 10.875 | 10.875 | 0 | 2.04305 | F | F | 4.65841 | 5.53414e-14 | 1 | dpcbx |
counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 10.00 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), A = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters,
b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters,
i = psf spatial fitting parameters, f = spectral fitting parameters,
c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest