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 | 2 | X004911.49-724940.5 | xmm | mos2 | 275.285 | 330.201 | 1499.48 | 43.7808 | 0.215432 | 0.00629003 | 102.314 | 1 | 5.7533 | 4.68934 | 99.3208 | 2.84135 | 507.783 | 1302.35 | 0.438954 | 0.0264339 | F | T | 4.72e+21 | 3.26325e-12 | 1 | dsx |
Report | srcpi bgdpi arf rmf | 1 | X004911.54-724939.6 | xmm | mos1 | 275.232 | 330.425 | 1444.15 | 43.2471 | 0.207645 | 0.00621823 | 103.454 | 1 | 5.69976 | 5.04386 | 77.5159 | 2.84834 | 519.1 | 1253.58 | 0.414332 | 0.0265028 | F | F | 4.72e+21 | 2.85586e-12 | 1 | dsx |
Report | srcpi bgdpi arf rmf | 1 | X004903.55-725055.3 | xmm | pn | 283.392 | 313.035 | 522.744 | 28.7144 | 0.104566 | 0.00574383 | 30.1688 | 1 | 5.08581 | 5.08581 | 0 | 1.52021 | 210.943 | 323.162 | 0.210106 | 0.0473081 | F | F | 4.74e+21 | 5.86936e-13 | 1 | dsx |
Report | srcpi bgdpi arf rmf | 2 | X004911.65-724940.0 | xmm | pn | 275.126 | 330.315 | 2971.66 | 61.145 | 0.594431 | 0.012231 | 171.502 | 1 | 5.7488 | 5.7488 | 0 | 2.84203 | 946.145 | 2489.22 | 0.449174 | 0.0191328 | F | T | 4.72e+21 | 2.8283e-12 | 1 | dsx |
Report | srcpi bgdpi arf rmf | 2 | X004903.61-725054.8 | xmm | mos1 | 283.325 | 313.145 | 289.846 | 20.7531 | 0.0416753 | 0.00298397 | 20.7636 | 1 | 5.43061 | 4.08391 | 91.2791 | 1.51864 | 105.43 | 188.101 | 0.281641 | 0.0654524 | F | T | 4.74e+21 | 7.5332e-13 | 1 | dsx |
Report | srcpi bgdpi arf rmf | 1 | X004903.51-725055.0 | xmm | mos2 | 283.429 | 313.105 | 269.203 | 21.6417 | 0.0386766 | 0.00310927 | 18.3685 | 1 | 5.26653 | 4.34492 | 70.4607 | 1.51391 | 112.773 | 164.813 | 0.187473 | 0.0661896 | F | F | 4.74e+21 | 7.27689e-13 | 1 | dbsx |
Report | srcpi bgdpi arf | 3 | X004908.91-725543.3 | xmm | pn | 278.026 | 246.646 | 32.9405 | 9.47054 | 0.00658918 | 0.00189442 | 5.33947 | 0.999999 | 10.875 | 10.875 | 0 | 4.03591 | 14.0061 | 16.7847 | 0.0902419 | 0.297527 | F | F | 4.9e+21 | 4.41763e-14 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X005000.44-724930.7 | xmm | pn | 225.439 | 332.304 | 96.9132 | 13.0844 | 0.0193858 | 0.00261732 | 5.5931 | 1 | 5.55566 | 5.55566 | 0 | 5.82629 | 37.2881 | 63.5041 | 0.2601 | 0.118743 | F | F | 4.84e+21 | 1.33192e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 3 | X004736.14-724537.4 | xmm | mos2 | 372.638 | 385.934 | 36.4139 | 8.02121 | 0.00523161 | 0.00115241 | 2.48463 | 0.992843 | 5.81377 | 5.81377 | 0 | 8.32977 | 21.0407 | 15.0611 | -0.165632 | 0.210035 | F | F | 4.27e+21 | 1.26659e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 6 | X004805.00-725041.1 | xmm | pn | 342.939 | 316.229 | 34.5325 | 9.61023 | 0.00690765 | 0.00192237 | 1.99296 | 0.974474 | 12.2239 | 4.43912 | 104.497 | 3.4268 | 26.8901 | 8.78024 | -0.507701 | 0.258162 | F | F | 4.56e+21 | 5.05316e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 4 | X004718.42-723951.4 | xmm | mos1 | 391.248 | 465.361 | 44.0897 | 7.85322 | 0.00633941 | 0.00112917 | 3.15843 | 0.998779 | 14.2454 | 4.14425 | 33.7238 | 13.8606 | 20.0647 | 4.19291 | -0.654302 | 0.340716 | A | F | 4.01e+21 | 2.44083e-13 | 1 | dsx |
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