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 | X182211.92-143033.6 | chandra | ccd7 | 643.635 | 195.013 | 26.3185 | 5.37151 | 0.0101217 | 0.00206581 | 18.8187 | 1 | 1.38547 | 1.38547 | 0 | 5.44148 | F | F | 1.36e+22 | 1.42322e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X182224.24-142613.1 | chandra | ccd7 | 279.965 | 724.335 | 15.7186 | 4.13469 | 0.00604514 | 0.00159014 | 11.2394 | 1 | 0.487731 | 0.487731 | 0 | 2.37469 | F | F | 1.36e+22 | 8.02773e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X182217.17-142232.7 | chandra | ccd6 | 479.389 | 120.833 | 8.93161 | 3 | 0.0034349 | 0.00115373 | 16.6862 | 1 | 0.492 | 0.492 | 1.75177 | 2.67275 | F | F | 1.36e+22 | 5.34138e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X182204.26-142843.1 | chandra | ccd7 | 869.5 | 419 | 5.85389 | 2.44949 | 0.00225128 | 0.000942022 | 4.18576 | 0.999047 | 0.492 | 0.492 | 99.9916 | 4.44869 | F | F | 1.36e+22 | 3.12405e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X182222.54-141825.7 | chandra | ccd6 | 320.7 | 622.9 | 4.7273 | 2.23608 | 0.00181802 | 0.000859946 | 8.83165 | 0.999999 | 0.907778 | 0.492 | 118.296 | 6.97259 | A | F | 1.37e+22 | 3.13771e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X182252.85-142707.4 | chandra | ccd3 | 791.9 | 787.1 | 4.05834 | 2.23609 | 0.00156075 | 0.000859953 | 7.73645 | 0.99999 | 1.84033 | 0.841976 | 160.306 | 9.2677 | A | F | 1.35e+22 | 2.86353e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X182211.24-142152.6 | chandra | ccd6 | 654.5 | 202.5 | 3.937 | 2 | 0.00151409 | 0.000769157 | 7.3552 | 0.999987 | 0.492 | 0.492 | 67.5 | 3.46021 | F | F | 1.36e+22 | 2.39694e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X182227.97-142617.4 | chandra | ccd7 | 169.5 | 715.25 | 3.92636 | 2 | 0.00150999 | 0.000769157 | 2.8075 | 0.984977 | 0.492 | 0.492 | 2.35031e-08 | 3.2328 | F | F | 1.35e+22 | 2.03898e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X182201.91-142627.1 | chandra | ccd7 | 938.75 | 695.5 | 3.90516 | 2 | 0.00150184 | 0.000769157 | 2.79234 | 0.984977 | 0.879542 | 0.492 | 68.7235 | 3.50661 | A | F | 1.36e+22 | 2.07344e-14 | 1 | dx | ||||
| Report | 1 | X182228.24-141956.8 | chandra | ccd6 | 152.167 | 437.833 | 2.89115 | 1.73205 | 0.00111187 | 0.00066611 | 5.40131 | 0.999776 | 0.492 | 0.492 | 106.845 | 6.09025 | F | F | 1.36e+22 | 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