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 | 2 | X004744.97-112754.5 | chandra | ccd7 | 919.218 | 977.958 | 21.5934 | 4.64687 | 0.00460235 | 0.000990418 | 22.675 | 1 | 0.445345 | 0.445345 | 0 | 0.31359 | F | F | 2.48e+20 | 3.31239e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X004729.62-112717.1 | chandra | ccd6 | 820.911 | 155.847 | 24.4426 | 4.94395 | 0.00520961 | 0.00105374 | 40.0636 | 1 | 1.27631 | 1.27631 | 0 | 4.12372 | F | F | 2.45e+20 | 5.77937e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X004737.11-112539.2 | chandra | ccd6 | 597.006 | 354.971 | 12.3256 | 3.51078 | 0.00262705 | 0.000748279 | 20.2028 | 1 | 0.64827 | 0.64827 | 0 | 3.23016 | F | F | 2.47e+20 | 2.80918e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X004831.51-111735.1 | chandra | ccd2 | 201.318 | 786.045 | 8.25893 | 3.31669 | 0.00176028 | 0.000706907 | 14.0731 | 1 | 4.08974 | 1.96246 | 141.696 | 15.2212 | A | F | 2.65e+20 | 2.58348e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X004749.21-112954.9 | chandra | ccd7 | 792.214 | 732.786 | 6.78809 | 2.64576 | 0.00144679 | 0.000563907 | 7.12811 | 0.999995 | 0.511856 | 0.492 | 4.06505 | 2.05684 | F | F | 2.49e+20 | 1.06046e-14 | 1 | dx | ||||
| Report | 4 | X004745.84-112915.5 | chandra | ccd7 | 892.833 | 812.833 | 5.83907 | 2.44949 | 0.00124452 | 0.000522077 | 6.13156 | 0.999954 | 0.492 | 0.492 | 16.845 | 1.26728 | F | F | 2.48e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X004810.25-113155.7 | chandra | ccd7 | 163.667 | 487.167 | 4.88982 | 2.44952 | 0.0010422 | 0.000522082 | 5.13475 | 0.999643 | 1.72027 | 0.492 | 34.6126 | 7.0836 | A | F | 2.53e+20 | 8.88466e-15 | 1 | dx | ||||
| Report | 6 | X004745.10-112048.9 | chandra | ccd6 | 357.9 | 944.5 | 4.73497 | 2.23607 | 0.0010092 | 0.000476589 | 7.76105 | 0.999997 | 0.804406 | 0.558126 | 27.1231 | 7.18417 | F | F | 2.51e+20 | 0 | 1 | d | |||||
| Report | 4 | X004726.76-112255.9 | chandra | ccd6 | 906 | 686.25 | 3.92155 | 2 | 0.000835825 | 0.000426274 | 6.42777 | 0.999956 | 0.492 | 0.492 | 37.9819 | 6.95096 | F | F | 2.45e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X004730.92-112307.9 | chandra | ccd6 | 781.75 | 662 | 3.77833 | 2.00001 | 0.000805301 | 0.000426275 | 6.19303 | 0.999956 | 0.492 | 0.492 | 52.0181 | 6.13779 | F | F | 2.46e+20 | 9.09529e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X004744.70-112522.0 | chandra | ccd6 | 369.833 | 389.5 | 2.9717 | 1.73205 | 0.000633377 | 0.000369164 | 4.87088 | 0.999405 | 0.492 | 0.492 | 180 | 2.65369 | F | F | 2.49e+20 | 6.69022e-15 | 1 | dx | ||||
| Report | 5 | X004731.39-112742.7 | chandra | ccd6 | 767.5 | 103.5 | 2.95897 | 1.73205 | 0.000630666 | 0.000369164 | 4.85003 | 0.999405 | 0.492 | 0.492 | 180 | 3.63951 | F | F | 2.45e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X004744.40-113246.4 | chandra | ccd7 | 935.833 | 384.167 | 2.93971 | 1.73205 | 0.000626559 | 0.000369164 | 3.08696 | 0.986199 | 0.492 | 0.492 | 90 | 4.79958 | F | F | 2.44e+20 | 5.05937e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X004747.19-112407.2 | chandra | ccd6 | 295.5 | 541.5 | 2.91659 | 1.73205 | 0.000621631 | 0.000369164 | 4.78055 | 0.999405 | 0.492 | 0.492 | 45 | 3.88204 | F | F | 2.5e+20 | 6.78121e-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