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 | X054332.96-273905.5 | chandra | ccd2 | 302.464 | 952.738 | 191.757 | 14.2762 | 0.0381753 | 0.00284214 | 55.2309 | 1 | 0.606987 | 0.445268 | 323.333 | 2.70638 | 40.8757 | 154.751 | 0.582106 | 0.0889323 | F | F | 2.16e+20 | 1.43886e-12 | 1 | dsxf |
| Report | srcpi bgdpi arf | 1 | X054422.24-273141.6 | chandra | ccd1 | 73.8999 | 881.033 | 15.1564 | 5.09268 | 0.00301738 | 0.00101386 | 16.5022 | 1 | 3.11429 | 1.19334 | 104.445 | 11.1054 | 13.708 | 1.51334 | -0.801156 | 0.431268 | A | F | 2.03e+20 | 4.73672e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X054405.34-274031.9 | chandra | ccd3 | 467.7 | 841.6 | 9.83616 | 4.27872 | 0.00195817 | 0.000851802 | 24.3003 | 1 | 0.508874 | 0.492 | 81.6008 | 4.66717 | 8 | 1.83616 | -0.626652 | 0.517901 | F | F | 2.11e+20 | 2.45272e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X054417.38-274137.8 | chandra | ccd3 | 142.7 | 707.4 | 8.60799 | 4.1225 | 0.00171367 | 0.000820702 | 13.7484 | 1 | 1.52165 | 0.704482 | 135.15 | 7.54241 | 6.9216 | 1.72559 | -0.60089 | 0.56156 | A | F | 2.1e+20 | 2.38277e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X054309.43-273403.7 | chandra | ccd0 | 998.2 | 527.2 | 10.3727 | 4.42783 | 0.00206503 | 0.000881508 | 13.096 | 1 | 2.74831 | 1.69689 | 30.1565 | 9.42349 | 7.84316 | 1.63405 | -0.655162 | 0.544522 | A | F | 2.17e+20 | 3.15725e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X054331.03-273208.4 | chandra | ccd0 | 414.4 | 762.1 | 11.6566 | 4.57071 | 0.00232064 | 0.000909954 | 19.8925 | 1 | 1.51998 | 1.23282 | 103.746 | 7.696 | 7.79398 | 3.86265 | -0.337261 | 0.416967 | F | F | 2.1e+20 | 3.26664e-14 | 1 | dx |
| Report | 4 | X054412.99-273756.4 | chandra | ccd1 | 324.643 | 119.5 | 6.705 | 2.64576 | 0.00133484 | 0.000526723 | 12.0309 | 1 | 1.1925 | 1.07806 | 155.766 | 6.28191 | F | F | 2.09e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X054347.35-273147.3 | chandra | ccd1 | 1017.36 | 870.071 | 9.67577 | 4.27872 | 0.00192627 | 0.000851816 | 16.9925 | 1 | 2.12215 | 1.0158 | 65.8777 | 7.39623 | 6.91894 | 2.83788 | -0.418277 | 0.479564 | A | F | 2.08e+20 | 2.68793e-14 | 1 | dx |
| Report | 1 | X054404.34-274024.6 | chandra | ccd3 | 494.7 | 856.5 | 4.93868 | 2.23607 | 0.000983187 | 0.000445154 | 8.78683 | 0.999999 | 0.575705 | 0.492 | 118.488 | 4.42003 | F | F | 2.11e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X054400.50-273300.9 | chandra | ccd1 | 661.7 | 720.3 | 5.84155 | 3.59808 | 0.00116295 | 0.000716312 | 14.6749 | 1 | 0.788755 | 0.492 | 93.2599 | 7.0281 | 2.89436 | 3.94718 | 0.153886 | 0.566172 | A | F | 2.07e+20 | 1.57387e-14 | 1 | dx |
| Report | 5 | X054344.14-274229.2 | chandra | ccd3 | 1040 | 603.25 | 3.95427 | 2 | 0.00078721 | 0.000398158 | 7.03537 | 0.99998 | 0.492 | 0.492 | 37.9819 | 3.32688 | F | F | 2.16e+20 | 0 | 1 | d | |||||
| Report | 4 | X054410.05-274203.5 | chandra | ccd3 | 340.5 | 655.25 | 3.81592 | 2.00001 | 0.000759668 | 0.000398159 | 6.78922 | 0.99998 | 0.58344 | 0.545758 | 2.35032e-08 | 6.21982 | F | F | 2.11e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X054331.67-273529.4 | chandra | ccd0 | 396.833 | 353.5 | 3.74592 | 3.17945 | 0.000745751 | 0.000632976 | 7.43145 | 0.999993 | 0.492 | 0.492 | 61.845 | 4.74082 | 1.83061 | 1.91531 | 0.0226095 | 0.864112 | F | F | 2.14e+20 | 9.36456e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 4 | X054342.07-273407.3 | chandra | ccd0 | 116 | 520.5 | 3.84526 | 3.17945 | 0.000765527 | 0.000632976 | 9.77501 | 0.999999 | 0.539213 | 0.492 | 130.269 | 5.09389 | 3.92263 | -0.0773723 | -1 | 1.16669 | F | F | 2.11e+20 | 1.0405e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X054310.22-273145.3 | chandra | ccd0 | 977 | 808.5 | 3.95191 | 3.17945 | 0.000786761 | 0.000632976 | 18.0216 | 1 | 1.73261 | 0.492 | 92.6884 | 10.7208 | 1 | 1.95191 | 0.322473 | 1.06783 | A | F | 2.14e+20 | 1.25132e-14 | 1 | dx |
| Report | 6 | X054325.45-273545.7 | chandra | ccd0 | 565 | 320.333 | 5.9071 | 2.44949 | 0.00117601 | 0.000487654 | 10.8197 | 1 | 0.702713 | 0.492 | 41.0053 | 5.54086 | F | F | 2.15e+20 | 0 | 1 | d |
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 - 7.99 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), T = 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