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 | X175356.86-290110.7 | chandra | ccd0 | 1026.61 | 532.426 | 26.5307 | 6.26783 | 0.0136204 | 0.0032178 | 38.7282 | 1 | 2.93642 | 2.03441 | 50.8792 | 10.2032 | 23.648 | 2.88268 | -0.782691 | 0.301141 | F | F | 6.24e+21 | 2.20855e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X175424.43-284915.8 | chandra | ccd1 | 367.5 | 938.147 | 17.5096 | 5.33013 | 0.00898895 | 0.00273635 | 25.0026 | 1 | 2.28747 | 1.47217 | 25.5697 | 8.42051 | 4.67305 | 12.8365 | 0.46623 | 0.337685 | A | F | 6.34e+21 | 1.37827e-13 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X175446.69-285126.5 | chandra | ccd3 | 801 | 751.5 | 7.8834 | 3.95804 | 0.00404696 | 0.00203187 | 23.0872 | 1 | 0.714565 | 0.492 | 90 | 5.7923 | 0.941702 | 6.9417 | 0.761093 | 0.637637 | F | F | 5.94e+21 | 5.61718e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X175412.69-285448.5 | chandra | ccd1 | 680.5 | 261.786 | 6.89543 | 3.78388 | 0.00353993 | 0.00194255 | 21.3232 | 1 | 1.37355 | 0.56545 | 48.3609 | 6.25975 | 4 | 2.89543 | -0.160189 | 0.562291 | A | F | 6.32e+21 | 4.97496e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X175509.72-285145.0 | chandra | ccd3 | 185.928 | 713.643 | 6.7368 | 3.78388 | 0.00345835 | 0.00194246 | 13.1313 | 1 | 1.45775 | 0.755247 | 49.0071 | 8.46105 | 3.95613 | 2.78066 | -0.174485 | 0.576872 | A | F | 5.66e+21 | 5.48841e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X175454.25-285921.6 | chandra | ccd2 | 552.667 | 833.833 | 5.9368 | 3.59808 | 0.00304774 | 0.00184712 | 23.6162 | 1 | 0.659691 | 0.492 | 171.622 | 3.99526 | -0.0631952 | 6 | 1 | 0.859312 | F | F | 5.52e+21 | 4.16652e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X175442.17-284950.6 | chandra | ccd3 | 921.5 | 946.5 | 4.89693 | 3.39792 | 0.00251385 | 0.00174433 | 15.2532 | 1 | 1.21266 | 0.492 | 56.3099 | 7.1955 | 3.96564 | 0.965644 | -0.60836 | 0.818787 | A | F | 6.05e+21 | 3.62091e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X175405.10-285314.1 | chandra | ccd1 | 883.1 | 453.3 | 4.90469 | 3.39792 | 0.00251794 | 0.0017444 | 15.8868 | 1 | 1.18587 | 0.667454 | 73.5153 | 8.41429 | 1.95234 | 2.95234 | 0.203887 | 0.717774 | A | F | 6.46e+21 | 3.76226e-14 | 1 | dx |
| Report | 2 | X175446.16-290116.5 | chandra | ccd2 | 768.25 | 600.5 | 3.96978 | 2 | 0.00203794 | 0.00102673 | 8.99649 | 0.999998 | 0.492 | 0.492 | 79.5728 | 4.50502 | F | F | 5.6e+21 | 0 | 1 | d | |||||
| Report | 5 | X175450.15-290035.3 | chandra | ccd2 | 661.833 | 684.167 | 2.97187 | 1.73205 | 0.00152565 | 0.000889171 | 6.73497 | 0.999949 | 0.492 | 0.492 | 90 | 4.27086 | F | F | 5.55e+21 | 0 | 1 | d | |||||
| Report | 4 | X175442.59-285919.0 | chandra | ccd2 | 863.5 | 839.167 | 2.96568 | 1.73205 | 0.00152247 | 0.000889171 | 6.72094 | 0.999949 | 0.550073 | 0.492 | 18.4349 | 2.40247 | F | F | 5.69e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 3 | X175440.30-290243.6 | chandra | ccd2 | 924.5 | 423.5 | 2.93818 | 2.93649 | 0.00150835 | 0.00150749 | 11.8175 | 0.999999 | 0.673699 | 0.492 | 26.5651 | 5.71428 | 1.93818 | 1 | -0.319307 | 1.07183 | F | F | 5.66e+21 | 2.15712e-14 | 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