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 | X120612.97-145031.9 | chandra | ccd0 | 1106.28 | 456.167 | 7.40965 | 3.00004 | 0.00348468 | 0.00141089 | 18.0463 | 1 | 2.58469 | 1.14051 | 146.905 | 10.6832 | A | F | 4.06e+20 | 5.32379e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X120655.76-144118.9 | chandra | ccd1 | 274.333 | 631.5 | 5.88097 | 2.44949 | 0.00276576 | 0.00115197 | 14.743 | 1 | 0.709439 | 0.535897 | 61.4279 | 5.73286 | F | F | 4.14e+20 | 3.36752e-14 | 1 | dx | ||||
| Report | 2 | X120716.67-144454.6 | chandra | ccd3 | 624.7 | 632.1 | 4.95783 | 2.23607 | 0.00233162 | 0.0010516 | 11.8964 | 1 | 0.525047 | 0.492 | 109.547 | 5.71273 | F | F | 4.13e+20 | 0 | 1 | d | |||||
| Report | 1 | X120704.50-144415.6 | chandra | ccd3 | 983.5 | 711.3 | 4.95127 | 2.23607 | 0.00232853 | 0.0010516 | 11.8806 | 1 | 0.636184 | 0.492 | 124.099 | 3.64675 | F | F | 4.13e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X120702.45-145313.2 | chandra | ccd2 | 621.3 | 552.7 | 4.87926 | 2.23607 | 0.00229466 | 0.0010516 | 11.8367 | 1 | 0.902675 | 0.513394 | 120.198 | 6.45072 | A | F | 4.08e+20 | 3.36309e-14 | 1 | dx | ||||
| Report | 2 | X120646.68-145020.1 | chandra | ccd2 | 1086 | 904.5 | 3.99009 | 2 | 0.0018765 | 0.000940579 | 9.67963 | 0.999999 | 0.492 | 0.492 | 180 | 3.82727 | F | F | 4.08e+20 | 0 | 1 | d | |||||
| Report | 3 | X120707.07-144518.3 | chandra | ccd3 | 908 | 584 | 3.96493 | 2 | 0.00186466 | 0.000940579 | 9.5139 | 0.999999 | 0.492 | 0.492 | 90 | 3.44705 | F | F | 4.12e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X120648.81-145037.2 | chandra | ccd2 | 1023.25 | 869.75 | 3.96482 | 2 | 0.00186461 | 0.000940579 | 9.61831 | 0.999999 | 0.600805 | 0.492 | 129.056 | 3.8551 | F | F | 4.08e+20 | 2.21212e-14 | 1 | dx | ||||
| Report | 2 | X120623.09-145001.7 | chandra | ccd0 | 808.25 | 517.75 | 3.91122 | 2 | 0.00183941 | 0.00094058 | 9.52582 | 0.999999 | 0.794785 | 0.492 | 62.2961 | 8.21488 | A | F | 4.07e+20 | 0 | 1 | d | |||||
| Report | 3 | X120639.95-144945.5 | chandra | ccd0 | 311.3 | 550.9 | 4.95184 | 2.23607 | 0.0023288 | 0.0010516 | 12.0603 | 1 | 0.502717 | 0.492 | 97.6276 | 4.49121 | F | F | 4.08e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X120621.75-145131.3 | chandra | ccd0 | 847.667 | 335.5 | 5.51535 | 2.4495 | 0.00259381 | 0.00115198 | 13.4327 | 1 | 1.97319 | 0.492 | 170.401 | 9.14858 | A | F | 4.06e+20 | 3.65368e-14 | 1 | dx | ||||
| Report | 5 | X120710.81-144519.0 | chandra | ccd3 | 797.5 | 582.5 | 2.98031 | 1.73205 | 0.00140161 | 0.000814566 | 7.1513 | 0.999967 | 0.492 | 0.492 | 90 | 4.24909 | F | F | 4.12e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X120717.30-144917.7 | chandra | ccd3 | 606.5 | 97.1667 | 2.95553 | 1.73205 | 0.00138995 | 0.000814566 | 7.09183 | 0.999967 | 0.492 | 0.492 | 49.7312 | 5.89656 | F | F | 4.1e+20 | 1.83408e-14 | 1 | dx | ||||
| Report | 2 | X120633.17-144201.3 | chandra | ccd1 | 940.5 | 545.167 | 2.94984 | 1.73205 | 0.00138728 | 0.000814566 | 7.39494 | 0.999976 | 0.492 | 0.492 | 28.155 | 7.24149 | F | F | 4.13e+20 | 0 | 1 | d |
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