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 | 3 | X182524.77-114524.7 | chandra | ccd7 | 705.152 | 784.902 | 235.775 | 15.5662 | 0.0401209 | 0.00264885 | 130.454 | 1 | 0.522391 | 0.405997 | 109.974 | 1.49992 | F | F | 1.47e+22 | 8.30232e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X182517.41-114351.2 | chandra | ccd7 | 924.698 | 974.843 | 17.7346 | 4.21125 | 0.00301783 | 0.000716611 | 9.81255 | 1 | 1.06026 | 0.54475 | 58.1716 | 3.16042 | F | F | 1.45e+22 | 4.26772e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X182559.68-114707.1 | chandra | ccd3 | 998.577 | 887.115 | 11.9479 | 3.60557 | 0.00203312 | 0.000613544 | 2.78774 | 0.99558 | 1.5633 | 1.18765 | 12.2035 | 7.69702 | F | F | 1.53e+22 | 3.80206e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X182604.00-114719.0 | chandra | ccd3 | 870.222 | 863.41 | 14.0445 | 5.69325 | 0.00238989 | 0.000968796 | 3.27694 | 0.998677 | 0.908564 | 0.908564 | 0 | 8.77002 | F | F | 1.54e+22 | 4.61093e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X182604.73-113806.2 | chandra | ccd2 | 940.5 | 951.4 | 8.55587 | 3.16231 | 0.00145591 | 0.000538115 | 11.4831 | 1 | 1.89919 | 1.58282 | 121.432 | 10.7165 | F | F | 1.52e+22 | 2.91396e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X182524.29-114043.1 | chandra | ccd6 | 810.9 | 309.7 | 4.93175 | 2.23607 | 0.00083967 | 0.000380709 | 6.45511 | 0.999967 | 0.492 | 0.492 | 148.283 | 4.13159 | F | T | 1.46e+22 | 1.34796e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X182519.34-113850.9 | chandra | ccd6 | 958.9 | 537.7 | 4.73935 | 2.23607 | 0.000806914 | 0.00038071 | 6.20329 | 0.999967 | 0.857479 | 0.492 | 15.2551 | 6.32099 | A | F | 1.44e+22 | 1.35558e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X182517.28-114331.0 | chandra | ccd7 | 928.1 | 1015.5 | 4.69854 | 2.23608 | 0.00079953 | 0.000380503 | 2.5997 | 0.981249 | 0.634366 | 0.492 | 75.4727 | 3.28801 | F | F | 1.45e+22 | 1.13344e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X182526.50-113726.6 | chandra | ccd6 | 745.1 | 709.1 | 4.5869 | 2.23608 | 0.000780958 | 0.00038071 | 6.00375 | 0.999967 | 1.49548 | 0.528959 | 157.049 | 7.21731 | A | F | 1.45e+22 | 1.46829e-14 | 1 | dx | ||||
| Report | 1 | X182516.13-113714.0 | chandra | ccd6 | 1054.75 | 734.75 | 3.90988 | 2 | 0.000665689 | 0.000340517 | 5.1176 | 0.999652 | 0.492 | 0.492 | 90 | 8.11722 | F | F | 1.43e+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