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 | X015841.42-432503.5 | chandra | ccd7 | 809.935 | 615.157 | 212.315 | 14.8339 | 0.042965 | 0.00300186 | 107.995 | 1 | 0.636342 | 0.38859 | 23.6088 | 0.300073 | F | F | 1.44e+20 | 3.2454e-13 | 1 | dsxf | ||||
| Report | srcpi bgdpi arf | 1 | X015821.94-432449.5 | chandra | ccd6 | 362.296 | 127.388 | 26.3803 | 5.13618 | 0.00533845 | 0.00103938 | 44.9831 | 1 | 0.838459 | 0.838459 | 0 | 3.24693 | F | F | 1.45e+20 | 5.82061e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 6 | X015843.46-432628.6 | chandra | ccd7 | 764.797 | 442.233 | 12.3154 | 3.50933 | 0.0024922 | 0.000710165 | 6.26426 | 0.999999 | 0.424908 | 0.424908 | 0 | 1.55575 | F | F | 1.43e+20 | 1.86934e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 4 | X015827.67-432521.1 | chandra | ccd6 | 234.722 | 62.7222 | 8.92534 | 3 | 0.00180616 | 0.000607091 | 15.2193 | 1 | 0.52763 | 0.492 | 27.1231 | 2.21324 | F | F | 1.44e+20 | 2.78175e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X015835.73-432416.9 | chandra | ccd7 | 935.389 | 709.278 | 8.88802 | 3 | 0.00179861 | 0.000607091 | 4.52092 | 0.999802 | 0.492 | 0.492 | 56.5993 | 1.07729 | F | F | 1.44e+20 | 1.35945e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X015844.95-431437.9 | chandra | ccd2 | 566.8 | 366.2 | 7.88182 | 3.16232 | 0.00159499 | 0.000639939 | 14.3861 | 1 | 2.68075 | 2.66195 | 151.414 | 10.4829 | F | F | 1.44e+20 | 2.26334e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X015839.11-431535.7 | chandra | ccd2 | 696.567 | 248.633 | 11.9839 | 3.87303 | 0.0024251 | 0.00078376 | 21.8733 | 1 | 3.66677 | 2.05117 | 106.433 | 9.47695 | A | F | 1.44e+20 | 3.69209e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X015843.16-432517.8 | chandra | ccd7 | 770.75 | 585.625 | 7.82716 | 2.82843 | 0.00158393 | 0.000572371 | 3.98131 | 0.999316 | 0.528574 | 0.492 | 164.272 | 0.656612 | F | F | 1.44e+20 | 1.23262e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X015903.78-432834.0 | chandra | ccd7 | 314.75 | 186.5 | 7.73015 | 2.82843 | 0.0015643 | 0.000572371 | 3.93196 | 0.999316 | 0.828118 | 0.492 | 147.87 | 5.58641 | A | F | 1.42e+20 | 1.23966e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X015849.39-432413.2 | chandra | ccd7 | 632.833 | 716.833 | 5.87538 | 2.44949 | 0.00118896 | 0.000495688 | 2.98853 | 0.993508 | 0.492 | 0.492 | 9.21747 | 1.94431 | F | F | 1.43e+20 | 8.89067e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X015757.01-432121.4 | chandra | ccd6 | 914.786 | 548.929 | 5.55736 | 2.64578 | 0.00112461 | 0.00053541 | 9.47629 | 0.999998 | 4.22622 | 1.7359 | 78.0895 | 8.61015 | A | F | 1.46e+20 | 1.4046e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X015817.43-432451.1 | chandra | ccd6 | 461.7 | 123.5 | 4.94597 | 2.23607 | 0.00100088 | 0.000452499 | 8.43375 | 0.999998 | 0.727012 | 0.492 | 43.7276 | 4.06236 | F | F | 1.45e+20 | 1.11038e-14 | 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