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 | 6 | X141429.96-002310.2 | chandra | ccd7 | 466.148 | 220.177 | 622.029 | 25.4886 | 0.0471174 | 0.00193071 | 151.819 | 1 | 0.455987 | 0.372995 | 107.272 | 1.30283 | 429.515 | 150.654 | -0.480656 | 0.0480485 | F | F | 3.32e+20 | 3.6349e-13 | 1 | dsxf |
Report | srcpi bgdpi arf | 1 | X141337.59-001725.6 | chandra | ccd3 | 754.307 | 516.064 | 67.3891 | 9.8176 | 0.00510457 | 0.00074366 | 21.7374 | 1 | 4.82654 | 3.60433 | 146.787 | 12.9992 | 25.2179 | 41.3609 | 0.242465 | 0.151072 | F | F | 3.41e+20 | 7.34265e-14 | 1 | dx |
Report | srcpi bgdpi arf rmf | 1 | X141341.57-002812.2 | chandra | ccd2 | 460.519 | 227.154 | 102.116 | 12.1062 | 0.00773505 | 0.000917019 | 15.3173 | 1 | 7.53061 | 5.4775 | 355.503 | 12.1397 | 49.7036 | 72.5888 | 0.187135 | 0.107801 | F | F | 3.45e+20 | 1.41113e-13 | 1 | dsxf |
Report | srcpi bgdpi arf | 3 | X141356.89-001958.3 | chandra | ccd3 | 165.767 | 205.667 | 29.0679 | 6.54527 | 0.00220183 | 0.000495789 | 30.1088 | 1 | 1.53817 | 1.12881 | 11.4153 | 7.56207 | 21.9379 | 7.13008 | -0.50942 | 0.253573 | F | F | 3.37e+20 | 3.01543e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X141346.39-001736.9 | chandra | ccd3 | 486.121 | 492.914 | 25.5946 | 6.54527 | 0.00193873 | 0.000495789 | 12.1942 | 1 | 4.57317 | 1.77569 | 175.292 | 10.9394 | 17.0795 | 8.64661 | -0.327794 | 0.268662 | A | F | 3.39e+20 | 2.73525e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X141424.08-002239.4 | chandra | ccd7 | 645.617 | 282.771 | 19.3218 | 5.02574 | 0.00146359 | 0.00038069 | 4.71587 | 0.999986 | 0.856251 | 0.856251 | 0 | 0.252404 | 20.7126 | 0.237533 | -0.977324 | 0.400457 | F | F | 3.33e+20 | 1.09488e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 6 | X141422.45-002517.0 | chandra | ccd6 | 537.297 | 995.392 | 17.5312 | 4.18703 | 0.00132796 | 0.000317159 | 19.7963 | 1 | 0.492312 | 0.492312 | 0 | 2.61584 | 13.9154 | 3.91535 | -0.56083 | 0.344582 | F | F | 3.33e+20 | 1.42642e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X141435.27-002621.8 | chandra | ccd6 | 146.367 | 863.743 | 18.5138 | 4.30277 | 0.00140238 | 0.000325926 | 20.9059 | 1 | 0.929335 | 0.929335 | 0 | 4.42837 | 11.6614 | 5.15339 | -0.387039 | 0.34174 | F | F | 3.31e+20 | 1.62635e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 4 | X141419.57-003146.0 | chandra | ccd6 | 624.5 | 204.167 | 14.5563 | 5.09268 | 0.00110261 | 0.000385758 | 12.1149 | 1 | 2.12332 | 0.952721 | 134.759 | 9.12139 | 7.50611 | 7.05022 | -0.0313193 | 0.352123 | A | F | 3.36e+20 | 1.361e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X141431.09-002852.2 | chandra | ccd6 | 273.143 | 557.5 | 13.3434 | 4.84057 | 0.00101073 | 0.000366662 | 16.4677 | 1 | 1.66323 | 0.716481 | 92.4765 | 6.30619 | 8.81762 | 5.52582 | -0.229499 | 0.357654 | A | F | 3.32e+20 | 1.20347e-14 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X141412.56-002716.7 | chandra | ccd6 | 838.3 | 751.5 | 4.79022 | 3.39792 | 0.000362848 | 0.000257384 | 10.4586 | 1 | 0.595809 | 0.492 | 58.7372 | 5.50002 | 2.86015 | 1.93007 | -0.194161 | 0.733559 | F | F | 3.36e+20 | 4.17139e-15 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X141437.36-002802.6 | chandra | ccd6 | 82 | 658.25 | 3.54905 | 3.17945 | 0.000268833 | 0.000240836 | 5.28506 | 0.999893 | 0.748517 | 0.498175 | 129.498 | 6.12738 | 1.77453 | 1.77453 | 0 | 0.630046 | A | F | 3.31e+20 | 3.51189e-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