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 | X144107.34+045506.3 | chandra | ccd7 | 265.652 | 831.413 | 181.49 | 13.8302 | 0.00845719 | 0.000644467 | 75.5131 | 1 | 0.379954 | 0.379954 | 0 | 0.523785 | 123.915 | 57.576 | -0.365523 | 0.0852264 | F | F | 2.75e+20 | 6.75608e-14 | 1 | dsxf |
| Report | srcpi bgdpi arf | 2 | X144105.53+045455.2 | chandra | ccd7 | 320.451 | 808.955 | 77.2094 | 9.23793 | 0.00359786 | 0.000430475 | 32.1247 | 1 | 0.406465 | 0.305437 | 23.2584 | 0.184249 | 47.7453 | 28.8727 | -0.246322 | 0.132157 | F | F | 2.75e+20 | 2.69512e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X144059.28+045345.8 | chandra | ccd7 | 510.191 | 667.893 | 16.3179 | 4.03954 | 0.000760392 | 0.000188237 | 6.78943 | 1 | 0.645747 | 0.310298 | 90.5702 | 1.9879 | 3.83713 | 12.9186 | 0.541991 | 0.355888 | F | F | 2.75e+20 | 5.73398e-15 | 1 | dsx |
| Report | srcpi bgdpi arf | 4 | X144111.60+045426.3 | chandra | ccd7 | 136.007 | 750.213 | 8.93633 | 3.60801 | 0.000416421 | 0.000168129 | 3.71816 | 0.999029 | 0.292986 | 0.292986 | 0 | 1.71264 | 8 | -0.0848312 | -1 | 0.707107 | F | F | 2.74e+20 | 3.15557e-15 | 1 | dsx |
| Report | srcpi bgdpi arf | 5 | X144110.63+045437.5 | chandra | ccd7 | 165.2 | 772.5 | 9.32245 | 4.27872 | 0.000434414 | 0.000199382 | 11.3256 | 1 | 0.492 | 0.492 | 94.7702 | 1.42082 | 7.83061 | 0.74592 | -0.826056 | 0.629477 | F | F | 2.74e+20 | 3.28232e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 6 | X144114.42+045448.2 | chandra | ccd7 | 49.875 | 794.25 | 8.23776 | 4.1225 | 0.000383868 | 0.000192103 | 9.43547 | 1 | 0.492 | 0.492 | 6.62026 | 2.30649 | 7.91531 | 0.661227 | -0.845806 | 0.635624 | F | F | 2.74e+20 | 2.96383e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 7 | X144058.78+045455.2 | chandra | ccd7 | 525.1 | 808.5 | 4.23776 | 3.39792 | 0.000197474 | 0.000158338 | 4.8539 | 0.999858 | 0.492 | 0.492 | 36.6504 | 1.61678 | -0.169387 | 4.74592 | 1 | 1.0279 | F | F | 2.76e+20 | 1.48811e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 8 | X144100.87+045649.1 | chandra | ccd7 | 461.667 | 1040 | 5.40715 | 3.59808 | 0.000251966 | 0.000167665 | 7.02255 | 0.999997 | 0.492 | 0.492 | 147.732 | 2.04378 | 4 | 1.57653 | -0.434583 | 0.712834 | F | F | 2.77e+20 | 2.72191e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 9 | X144104.99+045653.9 | chandra | ccd7 | 336.3 | 1049.7 | 8.62276 | 4.27872 | 0.000401809 | 0.000199382 | 7.34752 | 1 | 0.60557 | 0.492 | 156.323 | 1.81073 | 5.72455 | 1.38024 | -0.611462 | 0.659909 | F | F | 2.76e+20 | 3.08049e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 11 | X144045.18+045036.8 | chandra | ccd7 | 938.778 | 283.82 | 18.8239 | 6.33637 | 0.000877168 | 0.000295266 | 7.83211 | 1 | 3.9896 | 1.11781 | 99.0937 | 6.68296 | 12.0784 | 17.0144 | 0.169665 | 0.244048 | A | F | 2.75e+20 | 7.22008e-15 | 1 | dsx |
| Report | srcpi bgdpi arf | 12 | X144105.77+045206.2 | chandra | ccd7 | 313.102 | 465.438 | 29.913 | 5.47515 | 0.00139391 | 0.000255135 | 12.446 | 1 | 0.534429 | 0.299513 | 320.524 | 2.98956 | 18.8577 | 9.85766 | -0.313421 | 0.236386 | F | F | 2.73e+20 | 1.07376e-14 | 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 - 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