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 | 2 | X033358.34-391916.2 | chandra | ccd7 | 440.646 | 857.892 | 121.209 | 11.2386 | 0.0243868 | 0.00226116 | 92.9903 | 1 | 0.809424 | 0.809424 | 0 | 3.9845 | F | F | 1.52e+20 | 1.95061e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X033339.51-391841.5 | chandra | ccd7 | 884.742 | 928.631 | 58.1368 | 7.62475 | 0.0116969 | 0.00153407 | 44.602 | 1 | 0.409866 | 0.409866 | 0 | 0.298344 | F | F | 1.53e+20 | 8.70347e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X033326.48-391624.9 | chandra | ccd6 | 517.16 | 402.311 | 14.0967 | 3.75457 | 0.00283627 | 0.000755423 | 24.4625 | 1 | 0.855928 | 0.445702 | 104.708 | 3.12855 | F | F | 1.55e+20 | 3.11793e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X033347.50-392051.3 | chandra | ccd7 | 696.438 | 664.77 | 10.0351 | 3.16782 | 0.00201902 | 0.000637354 | 7.69883 | 1 | 0.470796 | 0.470796 | 0 | 2.90145 | F | F | 1.52e+20 | 1.53881e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X033339.82-391642.7 | chandra | ccd7 | 876.944 | 1169.72 | 8.88781 | 3 | 0.0017882 | 0.00060359 | 6.81864 | 0.999998 | 0.492 | 0.492 | 19.9028 | 1.92309 | F | F | 1.54e+20 | 1.36044e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X033301.10-391414.0 | chandra | ccd6 | 1116.07 | 667.214 | 6.27176 | 2.64577 | 0.00126188 | 0.000532327 | 10.8836 | 1 | 1.64359 | 1.39653 | 21.4505 | 8.3775 | F | F | 1.57e+20 | 1.67325e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X033343.93-391643.9 | chandra | ccd7 | 779.833 | 1167.17 | 5.88888 | 2.44949 | 0.00118482 | 0.000492829 | 4.51789 | 0.999614 | 0.492 | 0.492 | 90 | 2.19152 | F | F | 1.54e+20 | 9.03686e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X033357.02-391659.2 | chandra | ccd7 | 471 | 1135.83 | 5.85512 | 2.44949 | 0.00117803 | 0.000492829 | 4.49199 | 0.999614 | 0.492 | 0.492 | 21.3547 | 4.01254 | F | F | 1.53e+20 | 1.04456e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X033314.29-391813.2 | chandra | ccd6 | 804.1 | 181.5 | 4.91398 | 2.23607 | 0.000988691 | 0.000449896 | 8.52741 | 0.999999 | 0.492 | 0.492 | 55.9007 | 4.60862 | F | F | 1.55e+20 | 1.18134e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 10 | X033345.43-392112.7 | chandra | ccd7 | 744.7 | 620.9 | 4.90623 | 2.23607 | 0.000987116 | 0.000449889 | 3.76401 | 0.998131 | 0.492 | 0.492 | 21.4395 | 2.97433 | F | F | 1.52e+20 | 7.52263e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X033333.42-391551.5 | chandra | ccd6 | 352.9 | 469.7 | 4.87433 | 2.23607 | 0.000980713 | 0.000449897 | 8.45861 | 0.999999 | 0.639127 | 0.492 | 98.1301 | 2.88616 | F | F | 1.55e+20 | 1.06972e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X033430.39-391915.8 | chandra | ccd3 | 852.1 | 123.9 | 4.26633 | 2.23609 | 0.000858927 | 0.000450185 | 7.6961 | 0.999982 | 2.70927 | 0.492 | 77.5308 | 10.1485 | A | F | 1.49e+20 | 1.32135e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X033436.14-391436.9 | chandra | ccd3 | 715.1 | 690.5 | 8.16517 | 3.16232 | 0.00164387 | 0.000636661 | 14.7293 | 1 | 4.13172 | 1.50638 | 56.8111 | 11.9305 | A | F | 1.5e+20 | 2.86693e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X033431.45-391152.5 | chandra | ccd3 | 825.039 | 1024.96 | 9.77857 | 3.60562 | 0.00196869 | 0.000725908 | 17.6397 | 1 | 3.58316 | 2.89586 | 8.16493 | 12.3361 | F | F | 1.51e+20 | 2.81858e-14 | 1 | dcx | ||||
| Report | srcpi bgdpi arf | 4 | X033432.37-391141.1 | chandra | ccd3 | 803.1 | 1048.1 | 13.7692 | 4.47225 | 0.0027721 | 0.000900384 | 24.8384 | 1 | 6.52291 | 4.87714 | 175.002 | 12.5905 | F | F | 1.51e+20 | 4.21378e-14 | 1 | dcx | ||||
| Report | srcpi bgdpi arf | 5 | X033417.90-391450.1 | chandra | ccd3 | 1145.72 | 664.722 | 16.463 | 4.24266 | 0.00331445 | 0.000854162 | 29.698 | 1 | 2.4164 | 1.53215 | 160.235 | 8.58627 | A | F | 1.51e+20 | 4.63278e-14 | 1 | dx | ||||
| Report | 3 | X033313.87-391842.7 | chandra | ccd6 | 814 | 121.5 | 3.90796 | 2 | 0.000786279 | 0.0004024 | 6.78162 | 0.999974 | 0.492 | 0.492 | 63.4349 | 4.67531 | F | F | 1.55e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 7 | X033327.94-391928.7 | chandra | ccd7 | 1157 | 832.25 | 3.90531 | 2 | 0.000785735 | 0.000402393 | 2.99612 | 0.992022 | 0.504692 | 0.492 | 52.0181 | 2.13892 | F | F | 1.54e+20 | 6.04685e-15 | 1 | dx | ||||
| Report | 2 | X033316.55-391535.9 | chandra | ccd6 | 751.167 | 501.167 | 2.96783 | 1.73205 | 0.000597126 | 0.000348488 | 5.15018 | 0.999611 | 0.492 | 0.492 | 153.435 | 5.1294 | F | F | 1.56e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 9 | X033358.82-392243.3 | chandra | ccd7 | 429.167 | 436.5 | 2.9068 | 1.73205 | 0.000584838 | 0.000348483 | 2.23007 | 0.970449 | 0.492 | 0.492 | 180 | 5.75429 | F | F | 1.51e+20 | 4.65056e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 8 | X033338.66-392213.9 | chandra | ccd7 | 904.167 | 496.5 | 2.86279 | 1.73205 | 0.000575983 | 0.000348483 | 2.1963 | 0.970449 | 0.510281 | 0.492 | 28.155 | 3.63054 | F | F | 1.52e+20 | 4.51883e-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