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 | X020436.10-100919.3 | chandra | ccd7 | 201.703 | 852.734 | 32.5747 | 5.70742 | 0.00239695 | 0.00041997 | 19.1304 | 1 | 0.579938 | 0.579938 | 0 | 2.73845 | F | F | 2.23e+20 | 1.86692e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X020411.22-101324.1 | chandra | ccd7 | 948.186 | 355.061 | 26.2554 | 5.124 | 0.00193196 | 0.000377041 | 15.4192 | 1 | 1.01798 | 1.01798 | 0 | 5.29783 | F | F | 2.18e+20 | 1.66891e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X020433.24-101148.6 | chandra | ccd7 | 287.441 | 549.109 | 16.2272 | 4.0283 | 0.00119405 | 0.000296416 | 9.52988 | 1 | 0.522502 | 0.522502 | 0 | 3.20654 | F | T | 2.22e+20 | 9.79476e-15 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X020418.73-100959.2 | chandra | ccd7 | 722.3 | 771 | 9.16338 | 3.16229 | 0.000674269 | 0.000232691 | 5.38145 | 0.999989 | 0.595682 | 0.492 | 171.28 | 1.67009 | F | F | 2.25e+20 | 5.05886e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X020413.30-100804.5 | chandra | ccd7 | 885.167 | 1004.17 | 8.46418 | 3.00001 | 0.00062282 | 0.00022075 | 4.97083 | 0.999948 | 0.492 | 0.492 | 112.5 | 3.13404 | F | F | 2.27e+20 | 5.03509e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X020420.31-100827.3 | chandra | ccd7 | 674.929 | 957.786 | 6.38867 | 2.64576 | 0.000470098 | 0.000194683 | 3.75193 | 0.999143 | 0.492 | 0.492 | 139.731 | 1.44337 | F | F | 2.26e+20 | 3.54492e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X020409.63-100745.6 | chandra | ccd7 | 995.931 | 1043.06 | 25.7955 | 5.07893 | 0.00189811 | 0.000373723 | 15.1491 | 1 | 1.14048 | 1.14048 | 0 | 4.08707 | F | F | 2.23e+20 | 2.82138e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 8 | X020411.47-101400.9 | chandra | ccd7 | 940.167 | 279.833 | 7.58423 | 3.00003 | 0.000558071 | 0.000220751 | 4.45406 | 0.99978 | 0.492 | 0.492 | 45 | 5.74229 | F | F | 2.17e+20 | 5.02602e-15 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 9 | X020411.45-101358.7 | chandra | ccd7 | 940.75 | 284.25 | 3.14053 | 2.00002 | 0.00023109 | 0.000147168 | 1.84437 | 0.971309 | 1.15422 | 0.492 | 174.116 | 5.71557 | A | F | 2.17e+20 | 2.08163e-15 | 1 | dcx | ||||
Report | srcpi bgdpi arf | 10 | X020437.17-101436.0 | chandra | ccd7 | 169.192 | 208.385 | 21.9309 | 5.09907 | 0.00161374 | 0.000375205 | 12.8796 | 1 | 1.54969 | 1.2101 | 21.9645 | 6.0634 | F | F | 2.19e+20 | 1.35235e-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