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 | X182613.17-133446.7 | xmm | pn | 312.115 | 316.892 | 503.505 | 55.8086 | 0.0242727 | 0.0026904 | 9.85353 | 1 | 10.4532 | 5.54176 | 0.0734393 | 1.65667 | 219.047 | 414.246 | 0.308228 | 0.0625209 | F | F | 1.37e+22 | 1.8175e-13 | 1 | dsx |
| Report | srcpi bgdpi arf rmf | 1 | X182613.20-133448.5 | xmm | mos2 | 312.022 | 316.489 | 245.595 | 24.6905 | 0.0128263 | 0.00128947 | 15.3834 | 1 | 9.96575 | 5.86397 | 8.69853 | 1.66463 | 93.3366 | 210.338 | 0.385285 | 0.0725921 | F | F | 1.37e+22 | 2.71437e-13 | 1 | dsx |
| Report | srcpi bgdpi arf rmf | 2 | X182613.16-133447.5 | xmm | mos1 | 312.14 | 316.713 | 230.261 | 23.7336 | 0.0122916 | 0.00126693 | 16.0069 | 1 | 8.68961 | 6.67877 | 13.9512 | 1.6716 | 96.2165 | 171.484 | 0.281164 | 0.0761634 | F | F | 1.37e+22 | 2.33944e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X182603.63-133428.7 | xmm | pn | 344.086 | 321.019 | 32.1177 | 31.1952 | 0.00154832 | 0.00150384 | 1.08338 | 0.864144 | 10.875 | 10.875 | 0 | 3.69239 | 36.9633 | -3.55818 | -1 | 1.157 | F | F | 1.39e+22 | 1.06746e-14 | 1 | dbx |
| Report | srcpi bgdpi arf | 3 | X182640.70-133909.2 | xmm | mos2 | 219.869 | 256.236 | 88.3419 | 14.5554 | 0.00461368 | 0.000760162 | 9.08004 | 1 | 10.875 | 10.875 | 0 | 6.46582 | 83.9486 | 5.03613 | -0.886809 | 0.215978 | F | F | 1.29e+22 | 1.39987e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X182540.01-133132.0 | xmm | mos2 | 423.285 | 361.69 | 83.5547 | 14.2947 | 0.00436367 | 0.000746547 | 8.69017 | 1 | 10.875 | 10.875 | 0 | 10.1469 | 5.26675 | 75.4101 | 0.869436 | 0.229316 | F | F | 1.43e+22 | 1.43582e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X182640.67-133906.0 | xmm | mos1 | 219.971 | 256.964 | 80.3139 | 13.9518 | 0.00428725 | 0.000744766 | 8.62613 | 1 | 10.875 | 10.875 | 0 | 6.43446 | 72.5483 | 7.52107 | -0.812136 | 0.2215 | F | F | 1.29e+22 | 1.34072e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X182540.02-133129.0 | xmm | mos1 | 423.254 | 362.251 | 79.5256 | 13.7574 | 0.00424517 | 0.000734384 | 8.75684 | 1 | 10.875 | 10.875 | 0 | 10.1634 | 10.8862 | 72.2627 | 0.738151 | 0.20462 | F | F | 1.43e+22 | 1.20675e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X182621.11-134426.6 | xmm | mos2 | 285.522 | 183.584 | 38.1556 | 13.5606 | 0.00199268 | 0.000708203 | 2.38996 | 0.991148 | 4.03506 | 4.03506 | 0 | 8.39228 | 28.53 | 10.4885 | -0.462383 | 0.231849 | F | F | 1.3e+22 | 1.04687e-13 | 1 | dbsx |
| Report | srcpi bgdpi arf | 4 | X182630.55-132733.3 | xmm | mos1 | 253.823 | 416.533 | 46.4709 | 11.2832 | 0.00248067 | 0.000602311 | 3.23048 | 0.999147 | 21.9206 | 9.76394 | 134.097 | 9.06344 | 6.36743 | 5.36886 | -0.0850841 | 1.157 | T | F | 1.38e+22 | 7.696e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 5 | X182621.05-134427.7 | xmm | mos1 | 285.714 | 183.528 | 63.029 | 13.0727 | 0.00336456 | 0.000697836 | 6.96161 | 1 | 10.875 | 10.875 | 0 | 8.38182 | 35.9975 | 31.2636 | -0.0703807 | 0.194375 | F | F | 1.3e+22 | 1.16644e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X182614.08-132110.5 | xmm | mos2 | 309.059 | 503.491 | 43.127 | 11.4762 | 0.00225232 | 0.000599346 | 5.31369 | 1 | 10.875 | 10.875 | 0 | 14.8864 | 12.6547 | 33.0616 | 0.446382 | 0.271741 | F | F | 1.42e+22 | 1.44154e-13 | 1 | dpx |
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