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 | 1 | X144016.48-623913.2 | chandra | ccd3 | 656.758 | 683.415 | 86.2737 | 21.7371 | 0.0427999 | 0.0107837 | 5.8038 | 1 | 8.71184 | 8.71184 | 0 | 11.5092 | F | F | 7.26e+21 | 7.04537e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X144151.46-623616.4 | chandra | ccd7 | 550.592 | 459.925 | 37.1225 | 6.09341 | 0.0184163 | 0.00302291 | 35.9809 | 1 | 0.434457 | 0.434457 | 0 | 0.326146 | F | F | 7.07e+21 | 1.95324e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 1 | X144059.64-624300.4 | chandra | ccd2 | 603.678 | 1104.46 | 109.679 | 16.9688 | 0.0544111 | 0.00841811 | 11.1409 | 1 | 7.18167 | 7.18167 | 0 | 9.01353 | T | F | 6.88e+21 | 7.42989e-13 | 1 | dscxf | ||||
Report | srcpi bgdpi arf rmf | 2 | X144102.30-624310.4 | chandra | ccd2 | 566.336 | 1084.26 | 521.744 | 26.2261 | 0.258834 | 0.0130106 | 52.9971 | 1 | 14.3633 | 14.3633 | 0 | 8.97514 | T | F | 6.86e+21 | 4.0356e-12 | 1 | dcsx | ||||
Report | srcpi bgdpi arf | 2 | X144040.93-624000.5 | chandra | ccd3 | 313.876 | 589.088 | 27.7488 | 9.13561 | 0.013766 | 0.00453212 | 1.86672 | 0.966109 | 3.46926 | 2.84362 | 92.9149 | 9.10942 | F | F | 7.11e+21 | 2.12275e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 3 | X144101.73-624305.5 | chandra | ccd2 | 574.404 | 1094.28 | 179.212 | 13.387 | 0.0889063 | 0.00664124 | 18.2038 | 1 | 6.69786 | 6.69786 | 0 | 8.98458 | T | F | 6.87e+21 | 1.39333e-12 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 4 | X144056.91-624222.4 | chandra | ccd2 | 642.048 | 1181.6 | 20.3613 | 10.3189 | 0.0101011 | 0.00511917 | 2.06824 | 0.979265 | 2.15602 | 2.15602 | 0 | 8.82661 | F | F | 6.93e+21 | 1.58667e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 5 | X144048.23-624207.6 | chandra | ccd2 | 763 | 1210.81 | 20.9352 | 6.92847 | 0.0103858 | 0.00343717 | 2.12653 | 0.979265 | 3.08873 | 1.67169 | 126.789 | 9.4425 | A | F | 6.97e+21 | 1.60598e-13 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X144104.61-624322.7 | chandra | ccd2 | 533.486 | 1058.93 | 35.1535 | 8.48556 | 0.0174394 | 0.00420963 | 3.57078 | 0.999706 | 4.02424 | 1.67591 | 57.2116 | 8.95093 | A | F | 6.84e+21 | 2.7062e-13 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 7 | X144115.40-624354.2 | chandra | ccd2 | 383.155 | 995.783 | 18.716 | 8.53645 | 0.00928492 | 0.00423489 | 1.90111 | 0.96769 | 3.01761 | 0.83066 | 324.426 | 8.67156 | F | F | 6.77e+21 | 1.44645e-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 - 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