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 | 1 | X171659.57-624913.8 | chandra | ccd7 | 234.802 | 139.231 | 3416.31 | 60.1724 | 0.349157 | 0.0061498 | 512.299 | 1 | 0.468978 | 0.468978 | 0 | 0.28073 | F | F | 7.79e+20 | 1.23856e-11 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf rmf | 6 | X171648.23-624923.7 | chandra | ccd7 | 392.732 | 118.895 | 131.824 | 11.6192 | 0.0134728 | 0.00118751 | 19.7679 | 1 | 0.457423 | 0.457423 | 0 | 1.5611 | F | F | 7.81e+20 | 1.01651e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf rmf | 3 | X171705.43-624910.4 | chandra | ccd7 | 153.17 | 146.079 | 114.818 | 11.0631 | 0.0117347 | 0.00113068 | 17.2178 | 1 | 0.418384 | 0.418384 | 0 | 0.448893 | F | F | 7.77e+20 | 8.89104e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X171706.10-624923.3 | chandra | ccd7 | 143.77 | 119.857 | 43.0112 | 6.55829 | 0.00439588 | 0.000670278 | 6.44983 | 1 | 0.402918 | 0.402918 | 0 | 0.604106 | F | F | 7.77e+20 | 3.3287e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X171802.29-624914.0 | chandra | ccd6 | 405.761 | 129.5 | 19.9468 | 4.79587 | 0.00203862 | 0.000490152 | 18.5672 | 1 | 2.03724 | 1.59061 | 120.634 | 6.9332 | F | F | 7.66e+20 | 2.29765e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X171652.75-624900.7 | chandra | ccd7 | 329.704 | 165.715 | 15.43 | 4.75589 | 0.00157699 | 0.000486065 | 2.31383 | 0.984837 | 0.396735 | 0.396735 | 0 | 1.01045 | F | F | 7.8e+20 | 1.18783e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 5 | X171604.32-624925.3 | chandra | ccd7 | 1003.6 | 113.85 | 14.2404 | 4.47222 | 0.00145541 | 0.000457075 | 2.13545 | 0.9788 | 1.77177 | 1.30267 | 161.515 | 6.55033 | F | F | 7.92e+20 | 1.20396e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X171719.95-624846.8 | chandra | ccd6 | 995.333 | 186.333 | 5.88715 | 2.44949 | 0.000601684 | 0.000250346 | 5.47997 | 0.999972 | 0.492 | 0.492 | 45 | 2.11639 | F | F | 7.74e+20 | 6.13824e-15 | 1 | dx | ||||
| Report | 3 | X171729.06-624859.3 | chandra | ccd6 | 868.5 | 160.75 | 3.81548 | 2.00001 | 0.000389953 | 0.000204407 | 3.55158 | 0.993385 | 0.492 | 0.492 | 10.4272 | 3.13752 | F | F | 7.73e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 4 | X171722.08-624901.5 | chandra | ccd6 | 965.75 | 156.5 | 3.84055 | 2 | 0.000392516 | 0.000204407 | 3.57493 | 0.993385 | 0.492 | 0.492 | 34.722 | 2.33948 | F | F | 7.74e+20 | 4.02014e-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