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 | X213050.01-131800.3 | chandra | ccd1 | 173.256 | 422.637 | 13.9688 | 4.67544 | 0.00223525 | 0.000748153 | 4.97273 | 0.999973 | 2.76387 | 2.76387 | 0 | 8.4924 | F | F | 4.83e+20 | 2.84993e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X213033.10-131255.2 | chandra | ccd0 | 496.269 | 540.5 | 12.3809 | 3.60556 | 0.00198116 | 0.000576953 | 18.132 | 1 | 1.25283 | 0.755198 | 139.921 | 6.71231 | A | F | 4.81e+20 | 2.41501e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X213012.63-132038.0 | chandra | ccd3 | 280.7 | 413.9 | 9.82491 | 3.16228 | 0.00157216 | 0.00050602 | 14.085 | 1 | 0.680116 | 0.492 | 6.62026 | 2.68736 | F | F | 4.86e+20 | 1.75154e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X213007.85-131757.0 | chandra | ccd2 | 258.5 | 267.125 | 7.89406 | 2.82843 | 0.00126319 | 0.000452598 | 11.1222 | 1 | 0.492 | 0.492 | 112.955 | 1.77655 | F | F | 4.83e+20 | 1.53858e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X213011.26-131904.0 | chandra | ccd3 | 321.375 | 605.125 | 7.86765 | 2.82843 | 0.00125896 | 0.000452598 | 11.2791 | 1 | 0.492 | 0.492 | 16.5119 | 1.41229 | F | F | 4.85e+20 | 1.38669e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X213017.92-131333.8 | chandra | ccd0 | 946.667 | 462.167 | 5.85536 | 2.44949 | 0.000936961 | 0.000391962 | 8.57527 | 0.999999 | 0.492 | 0.492 | 78.8469 | 4.50484 | F | F | 4.81e+20 | 1.08589e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X213010.49-132116.6 | chandra | ccd3 | 344.1 | 335.5 | 4.92389 | 2.23607 | 0.000787908 | 0.00035781 | 7.0589 | 0.999988 | 0.492 | 0.492 | 90 | 3.45061 | F | F | 4.87e+20 | 8.9537e-15 | 1 | dx | ||||
Report | 3 | X212948.07-131824.4 | chandra | ccd2 | 845.5 | 211.3 | 4.73577 | 2.23608 | 0.000757807 | 0.000357811 | 6.67237 | 0.999985 | 0.492 | 0.492 | 90 | 6.6003 | F | T | 4.85e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X212957.85-132106.5 | chandra | ccd3 | 719 | 356 | 3.9234 | 2 | 0.000627813 | 0.000320035 | 5.6246 | 0.999848 | 0.492 | 0.492 | 90 | 5.22037 | F | T | 4.87e+20 | 7.62357e-15 | 1 | dx | ||||
Report | 3 | X213035.00-131405.1 | chandra | ccd0 | 439.75 | 398.5 | 3.81525 | 2.00001 | 0.000610506 | 0.000320036 | 5.58748 | 0.999875 | 0.492 | 0.492 | 180 | 6.2295 | F | T | 4.82e+20 | 0 | 1 | d | |||||
Report | 4 | X213025.65-131602.9 | chandra | ccd0 | 717.25 | 159 | 3.89296 | 2 | 0.000622941 | 0.000320036 | 5.70129 | 0.999875 | 0.492231 | 0.492 | 166.224 | 3.22614 | F | F | 4.82e+20 | 0 | 1 | d | |||||
Report | 5 | X213024.73-131518.7 | chandra | ccd0 | 744.7 | 248.9 | 4.93259 | 2.23607 | 0.0007893 | 0.00035781 | 7.22384 | 0.99999 | 0.492 | 0.492 | 18.4349 | 3.5711 | F | T | 4.82e+20 | 0 | 1 | d | |||||
Report | 6 | X213028.81-131335.9 | chandra | ccd0 | 623.5 | 457.833 | 2.93343 | 1.73205 | 0.0004694 | 0.000277159 | 4.29605 | 0.99864 | 0.627179 | 0.492 | 146.31 | 5.52982 | F | F | 4.81e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 7 | X213027.72-131558.8 | chandra | ccd0 | 655.833 | 167.5 | 2.95285 | 1.73205 | 0.000472508 | 0.000277159 | 4.32449 | 0.99864 | 0.492 | 0.492 | 180 | 3.67636 | F | F | 4.82e+20 | 5.33672e-15 | 1 | dx |
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