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 | X175233.33-293945.3 | chandra | ccd3 | 932.248 | 764.486 | 53.8914 | 7.34108 | 0.0276638 | 0.00376836 | 109.548 | 1 | 1.74045 | 0.703626 | 130.619 | 5.60635 | 37.8288 | 11.8631 | -0.522535 | 0.184857 | A | F | 6.37e+21 | 3.85482e-13 | 1 | dscx |
| Report | srcpi bgdpi arf | 3 | X175233.41-293946.7 | chandra | ccd3 | 929.567 | 761.1 | 16.3894 | 5.21307 | 0.00841307 | 0.00267599 | 20.9751 | 1 | 0.492 | 0.492 | 55.7065 | 5.5757 | 11.6947 | 4.69472 | -0.427104 | 0.347833 | F | F | 6.37e+21 | 1.17198e-13 | 1 | dcx |
| Report | srcpi bgdpi arf | 1 | X175156.13-295115.6 | chandra | ccd0 | 766.143 | 300.876 | 16.0534 | 4.70787 | 0.00824135 | 0.00241688 | 6.49418 | 1 | 4.35712 | 4.35712 | 0 | 9.34481 | 9.13724 | 9.47592 | 0.018196 | 0.311435 | F | F | 6.65e+21 | 1.29806e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X175259.97-294018.4 | chandra | ccd3 | 226.167 | 696.389 | 8.85054 | 4.1225 | 0.00454318 | 0.00211617 | 22.8931 | 1 | 0.853962 | 0.502446 | 71.0802 | 8.31565 | 9 | -0.149462 | -1 | 0.654039 | A | F | 6.01e+21 | 6.96901e-14 | 1 | dx |
| Report | 5 | X175241.87-294158.9 | chandra | ccd3 | 705.7 | 492.3 | 4.96459 | 2.23607 | 0.00254843 | 0.00114782 | 10.0918 | 1 | 0.497649 | 0.492 | 121.121 | 4.28393 | F | F | 6.21e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 1 | X175212.48-293717.4 | chandra | ccd1 | 458.3 | 957.5 | 4.93882 | 3.39792 | 0.00253531 | 0.0017443 | 19.9676 | 1 | 0.833252 | 0.601914 | 110.505 | 8.78565 | 3 | 1.93882 | -0.214865 | 0.714384 | F | F | 6.71e+21 | 4.1235e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X175217.50-294016.3 | chandra | ccd1 | 325 | 594 | 3.91531 | 3.17945 | 0.0020099 | 0.00163215 | 13.4537 | 1 | 0.492 | 0.492 | 45 | 5.62561 | 2.91531 | 2 | -0.186216 | 0.713849 | F | F | 6.58e+21 | 2.78277e-14 | 1 | dx |
| Report | 4 | X175229.80-294012.5 | chandra | ccd3 | 1025.25 | 708.75 | 3.91061 | 2 | 0.0020074 | 0.00102665 | 7.94932 | 0.999994 | 0.58781 | 0.492 | 153.014 | 5.075 | F | F | 6.41e+21 | 0 | 1 | d | |||||
| Report | 6 | X175239.58-294508.4 | chandra | ccd3 | 766.5 | 107.167 | 2.97243 | 1.73205 | 0.00152582 | 0.0008891 | 6.04223 | 0.999882 | 0.492 | 0.492 | 90 | 2.23893 | F | F | 6.18e+21 | 0 | 1 | d | |||||
| Report | 3 | X175224.08-294301.2 | chandra | ccd1 | 150.833 | 258.833 | 2.9663 | 1.73205 | 0.00152273 | 0.000889138 | 5.72223 | 0.999825 | 0.492 | 0.492 | 45 | 2.5285 | F | F | 6.44e+21 | 0 | 1 | d | |||||
| Report | 1 | X175227.01-294702.1 | chandra | ccd2 | 998.167 | 911.167 | 2.95888 | 1.73205 | 0.00151889 | 0.000889119 | 6.727 | 0.99995 | 0.492 | 0.492 | 45 | 1.82152 | F | F | 6.31e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X175227.52-294714.6 | chandra | ccd2 | 984.5 | 885.833 | 2.91531 | 2.93649 | 0.00149652 | 0.0015074 | 10.0175 | 0.999998 | 0.492 | 0.492 | 90 | 1.99789 | 2.91531 | 0 | -1 | 1.4553 | F | F | 6.3e+21 | 1.9619e-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