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 | X005104.89-010152.0 | chandra | ccd7 | 740.747 | 1051.26 | 137.596 | 12.0983 | 0.0384722 | 0.00338272 | 63.2292 | 1 | 0.411828 | 0.411828 | 0 | 1.13821 | F | F | 3.46e+20 | 2.02677e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 3 | X005102.44-010244.2 | chandra | ccd7 | 815.455 | 945.225 | 33.3092 | 5.77141 | 0.00931333 | 0.0016137 | 15.3065 | 1 | 0.472633 | 0.472633 | 0 | 0.298923 | F | F | 3.46e+20 | 6.84089e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 2 | X005102.96-010907.1 | chandra | ccd7 | 799.739 | 166.842 | 15.5078 | 5.06728 | 0.00433602 | 0.00141682 | 7.12627 | 1 | 1.5 | 1.245 | 325.531 | 6.53384 | F | F | 3.51e+20 | 3.5709e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 8 | X005101.31-010557.5 | chandra | ccd7 | 850.062 | 552.217 | 10.2316 | 3.19869 | 0.00286077 | 0.000894359 | 4.70171 | 0.999872 | 0.629952 | 0.629952 | 0 | 3.36393 | F | F | 3.48e+20 | 2.17172e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X005113.00-010119.4 | chandra | ccd7 | 493.278 | 1117.06 | 8.71324 | 3.00001 | 0.00243621 | 0.000838799 | 4.00398 | 0.999585 | 0.669501 | 0.492 | 155.389 | 3.16696 | F | F | 3.48e+20 | 1.92562e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X005055.97-010207.3 | chandra | ccd7 | 1012.38 | 1019.75 | 7.86973 | 2.82843 | 0.00220037 | 0.000790826 | 3.61636 | 0.998736 | 0.492 | 0.492 | 17.3674 | 1.43638 | F | F | 3.43e+20 | 1.64884e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 7 | X005104.16-010857.2 | chandra | ccd7 | 762.5 | 186.5 | 4.56521 | 2.23608 | 0.00127643 | 0.000625205 | 2.09784 | 0.976779 | 1.4182 | 0.702908 | 100.519 | 6.39674 | A | F | 3.51e+20 | 1.03294e-14 | 1 | dx | ||||
| Report | 1 | X005058.66-005845.0 | chandra | ccd6 | 433.167 | 493.833 | 2.94543 | 1.73205 | 0.00082354 | 0.00048428 | 5.46002 | 0.999763 | 0.543766 | 0.492 | 145.278 | 3.90445 | F | F | 3.42e+20 | 0 | 1 | d | |||||
| Report | srcpi bgdpi arf | 2 | X005042.12-005513.6 | chandra | ccd6 | 937.5 | 923.5 | 4.92747 | 2.44952 | 0.00137772 | 0.000684883 | 9.13417 | 0.999999 | 2.33155 | 1.28227 | 84.4795 | 8.80292 | A | F | 3.33e+20 | 1.71243e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X005049.10-010004.1 | chandra | ccd6 | 725.221 | 333.597 | 15.7738 | 3.97162 | 0.00441038 | 0.00111047 | 29.2403 | 1 | 1.20643 | 0.679921 | 90.1479 | 3.97935 | F | F | 3.39e+20 | 5.65266e-14 | 1 | dsx |
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