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 | X175430.14-292357.2 | chandra | ccd0 | 113.796 | 692.941 | 31.6706 | 5.62766 | 0.0162765 | 0.00289223 | 70.0734 | 1 | 0.844246 | 0.466492 | 50.3608 | 3.3196 | 29.9064 | 1 | -0.935288 | 0.294913 | F | F | 5.16e+21 | 2.19794e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 4 | X175448.27-291940.0 | chandra | ccd3 | 759.832 | 270.664 | 21.5198 | 4.63894 | 0.0110596 | 0.00238409 | 47.7709 | 1 | 0.633273 | 0.633273 | 0 | 2.6271 | 5 | 17.8306 | 0.561992 | 0.296387 | F | F | 5.02e+21 | 1.41909e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 4 | X175502.52-292227.5 | chandra | ccd2 | 284.056 | 973.389 | 8.85934 | 4.1225 | 0.00455296 | 0.00211862 | 23.6218 | 1 | 0.592153 | 0.492 | 112.795 | 5.42224 | 1.92967 | 6.92967 | 0.564376 | 0.539477 | F | F | 4.83e+21 | 6.31086e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X175410.25-291404.3 | chandra | ccd1 | 717.643 | 843.071 | 6.53361 | 3.78388 | 0.00335773 | 0.0019446 | 9.56707 | 1 | 1.84001 | 1.26692 | 93.496 | 9.36952 | 3.65021 | 2.8834 | -0.117363 | 0.589981 | F | F | 5.71e+21 | 5.14181e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X175500.04-291811.7 | chandra | ccd3 | 446.5 | 449.3 | 5.8563 | 3.59808 | 0.00300965 | 0.00184911 | 15.4488 | 1 | 0.579845 | 0.492 | 111.137 | 5.57895 | 1 | 4.8563 | 0.658487 | 0.745381 | F | F | 4.93e+21 | 4.13677e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X175505.70-292529.7 | chandra | ccd2 | 199.75 | 603 | 3.7536 | 3.17945 | 0.00192904 | 0.00163397 | 7.56176 | 0.999994 | 0.845795 | 0.492 | 88.2393 | 7.3676 | 1.85216 | 1.90144 | 0.013129 | 0.862199 | A | F | 4.79e+21 | 2.82407e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X175453.43-292657.8 | chandra | ccd2 | 525.75 | 424.25 | 3.94085 | 3.17945 | 0.00202527 | 0.00163397 | 16.2031 | 1 | 0.704643 | 0.492 | 23.3679 | 6.66731 | 1.94085 | 2 | 0.0150104 | 0.821253 | F | F | 4.84e+21 | 3.32662e-14 | 1 | dx |
| Report | 1 | X175438.87-291717.1 | chandra | ccd3 | 1009.17 | 560.5 | 2.97333 | 1.73205 | 0.00152805 | 0.000890131 | 6.60037 | 0.99994 | 0.492 | 0.492 | 5.35186e-08 | 3.87616 | F | F | 5.24e+21 | 0 | 1 | d | |||||
| Report | 2 | X175438.82-291610.9 | chandra | ccd3 | 1010.5 | 695.167 | 2.9607 | 1.73205 | 0.00152155 | 0.000890131 | 6.57233 | 0.99994 | 0.492 | 0.492 | 71.565 | 4.97982 | F | F | 5.28e+21 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 5 | X175447.28-292045.4 | chandra | ccd3 | 785.833 | 137.167 | 2.91531 | 2.93649 | 0.00149823 | 0.00150911 | 10.0175 | 0.999998 | 0.492 | 0.492 | 0 | 1.98612 | 2.91531 | 0 | -1 | 1.4553 | F | F | 5e+21 | 1.91018e-14 | 1 | dx |
| Report | 1 | X175504.56-292838.4 | chandra | ccd2 | 230.5 | 219.5 | 0.917637 | 1 | 0.000471589 | 0.000513919 | 1.98242 | 0.980075 | 0.492 | 0.492 | 90 | 9.40814 | F | F | 4.76e+21 | 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