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 | 3 | X174535.58-290134.4 | chandra | ccd3 | 189.11 | 810.928 | 369.199 | 31.3273 | 0.0741693 | 0.00629341 | 19.3679 | 1 | 1.53274 | 1.53274 | 0 | 1.82145 | T | F | 1.2e+22 | 2.36952e-12 | 1 | dscxf | ||||
| Report | srcpi bgdpi arf rmf | 1 | X174535.50-290133.8 | chandra | ccd3 | 191.147 | 812.256 | 124.895 | 30.5891 | 0.0250905 | 0.00614512 | 6.55189 | 1 | 0.766372 | 0.766372 | 0 | 1.81548 | F | F | 1.2e+22 | 3.84206e-13 | 1 | dscx | ||||
| Report | srcpi bgdpi arf | 11 | X174529.97-290703.8 | chandra | ccd3 | 338.45 | 141.388 | 38.1558 | 7.45901 | 0.00766521 | 0.00149846 | 2.00162 | 0.975866 | 1.10894 | 1.10894 | 0 | 7.39398 | F | F | 1.2e+22 | 1.29647e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X174535.60-290124.1 | chandra | ccd3 | 187.878 | 831.456 | 46.7075 | 8.12418 | 0.00938317 | 0.00163208 | 2.45024 | 0.992448 | 0.671524 | 0.61612 | 172.012 | 1.67739 | T | F | 1.2e+22 | 1.43752e-13 | 1 | dbx | ||||
| Report | srcpi bgdpi arf | 6 | X174539.80-290021.7 | chandra | ccd3 | 76.5208 | 958.741 | 71.3557 | 9.18613 | 0.0143348 | 0.00184542 | 3.74326 | 0.999857 | 1.4719 | 1.4719 | 0 | 0.354328 | T | F | 1.19e+22 | 2.17797e-13 | 1 | dsbx | ||||
| Report | srcpi bgdpi arf | 1 | X174545.43-285828.8 | chandra | ccd0 | 1136.34 | 372.204 | 28.2731 | 5.31725 | 0.00567984 | 0.00106819 | 19.9959 | 1 | 1.71238 | 0.849667 | 1.69571 | 1.96116 | T | F | 1.19e+22 | 1.11829e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 7 | X174543.94-290457.0 | chandra | ccd1 | 973.203 | 592.255 | 16.9234 | 4.11381 | 0.00339979 | 0.000826433 | 13.9252 | 1 | 2.17248 | 0.428671 | 338.913 | 5.04131 | A | F | 1.19e+22 | 5.37652e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X174532.30-285611.8 | chandra | ccd2 | 465.1 | 458.2 | 9.56918 | 3.16229 | 0.00192237 | 0.000635278 | 8.28389 | 1 | 0.623151 | 0.494804 | 130.358 | 4.12349 | F | F | 1.19e+22 | 3.11099e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X174536.10-285638.9 | chandra | ccd2 | 363.7 | 403.1 | 9.48953 | 3.16229 | 0.00190637 | 0.000635278 | 8.21494 | 1 | 0.794811 | 0.492 | 171.303 | 3.4311 | A | F | 1.19e+22 | 3.03446e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X174542.49-285817.5 | chandra | ccd2 | 193.3 | 202.6 | 8.99393 | 3.1623 | 0.00180681 | 0.00063528 | 7.78591 | 1 | 0.681672 | 0.492 | 138.263 | 1.79869 | T | F | 1.19e+22 | 2.83704e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X174614.10-290222.3 | chandra | ccd1 | 168.7 | 905.6 | 8.80006 | 3.1623 | 0.00176786 | 0.00063528 | 7.24103 | 1 | 1.12684 | 0.88287 | 118.795 | 7.88446 | F | F | 1.18e+22 | 3.0159e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X174558.89-290723.3 | chandra | ccd1 | 574.6 | 294.1 | 7.69045 | 3.16233 | 0.00154495 | 0.000635286 | 6.328 | 0.999996 | 1.5343 | 0.96513 | 71.5267 | 8.50485 | A | F | 1.19e+22 | 2.84599e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X174552.53-285709.2 | chandra | ccd0 | 946.5 | 533.5 | 4.54688 | 2.23608 | 0.000913431 | 0.00044921 | 3.21574 | 0.995475 | 0.492 | 0.492 | 45 | 3.98348 | F | F | 1.19e+22 | 1.4491e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X174540.22-285624.7 | chandra | ccd2 | 253.75 | 432 | 3.90022 | 2 | 0.000783523 | 0.000401784 | 3.37636 | 0.997465 | 0.492 | 0.492 | 52.0181 | 3.57685 | F | F | 1.19e+22 | 1.34759e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X174516.07-285756.8 | chandra | ccd2 | 898 | 244.5 | 3.73898 | 2.00001 | 0.000751131 | 0.000401785 | 3.23678 | 0.997465 | 0.598734 | 0.492 | 75.1276 | 5.56099 | F | F | 1.19e+22 | 1.2734e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X174550.73-285626.3 | chandra | ccd0 | 994.25 | 620.75 | 3.60537 | 2.00001 | 0.00072429 | 0.000401786 | 2.54987 | 0.983464 | 0.492 | 0.492 | 45 | 4.28886 | F | F | 1.19e+22 | 1.15936e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X174551.99-285311.4 | chandra | ccd0 | 960.7 | 1016.7 | 4.12734 | 2.23609 | 0.00082915 | 0.000449213 | 2.91903 | 0.995475 | 0.720338 | 0.492 | 138.102 | 7.30615 | F | F | 1.19e+22 | 1.55846e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X174548.94-285751.9 | chandra | ccd0 | 1042.17 | 446.667 | 5.72247 | 2.4495 | 0.0011496 | 0.000492084 | 4.04717 | 0.998906 | 0.492 | 0.492 | 4.21348 | 2.92617 | F | F | 1.19e+22 | 1.89673e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X174533.90-285749.2 | chandra | ccd2 | 422.25 | 260.25 | 3.56381 | 2.00001 | 0.000715941 | 0.000401787 | 3.08514 | 0.988182 | 0.492 | 0.492 | 59.8724 | 2.51314 | F | F | 1.19e+22 | 1.2871e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X174553.27-290709.2 | chandra | ccd1 | 724.167 | 322.833 | 3.53428 | 2.00002 | 0.000710009 | 0.000401787 | 2.90814 | 0.995861 | 0.749069 | 0.492 | 55.278 | 7.75483 | A | F | 1.19e+22 | 1.24786e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X174544.72-290025.1 | chandra | ccd1 | 951.9 | 1144.3 | 3.12068 | 2.23613 | 0.00062692 | 0.00044922 | 2.56782 | 0.982487 | 0.693255 | 0.492 | 52.8543 | 1.17386 | T | F | 1.19e+22 | 9.85549e-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