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 | 6 | X082124.49-362908.0 | chandra | ccd7 | 916.866 | 449.403 | 176.104 | 13.5629 | 0.0831798 | 0.00640623 | 123.759 | 1 | 0.389054 | 0.389054 | 0 | 0.335688 | F | F | 7.27e+21 | 3.67195e-13 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 3 | X082152.23-362618.3 | chandra | ccd7 | 236.555 | 793.971 | 87.2431 | 9.35377 | 0.0412078 | 0.0044181 | 61.311 | 1 | 2.38292 | 2.38292 | 0 | 6.40123 | F | F | 7.18e+21 | 4.81001e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X082121.02-362903.0 | chandra | ccd7 | 1002.01 | 459.627 | 11.2623 | 3.35594 | 0.00531955 | 0.00158512 | 7.9147 | 1 | 0.652483 | 0.652483 | 0 | 0.821172 | F | F | 7.27e+21 | 5.74107e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X082143.62-363009.7 | chandra | ccd7 | 448.036 | 323.787 | 14.7457 | 3.84001 | 0.00696488 | 0.00181377 | 10.3627 | 1 | 1.21338 | 0.616713 | 76.7328 | 3.89723 | F | F | 7.23e+21 | 7.92466e-14 | 1 | dsx | ||||
Report | 4 | X082135.40-362556.4 | chandra | ccd7 | 648.75 | 838.25 | 3.96698 | 2 | 0.00187372 | 0.000944657 | 2.78784 | 0.982524 | 0.492 | 0.492 | 25.6701 | 4.14894 | F | F | 7.21e+21 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 5 | X082137.65-362507.9 | chandra | ccd7 | 593.5 | 936.75 | 3.92741 | 2 | 0.00185503 | 0.000944658 | 2.76003 | 0.982524 | 0.492 | 0.492 | 154.547 | 5.07433 | F | F | 7.19e+21 | 2.08637e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X082109.12-363620.6 | chandra | ccd6 | 563.5 | 376.5 | 1.80703 | 1.41422 | 0.00085351 | 0.000667977 | 4.82269 | 0.99102 | 1.04369 | 0.492 | 45 | 7.54038 | A | F | 7.38e+21 | 1.35905e-14 | 1 | dx | ||||
Report | 2 | X082046.70-363139.3 | chandra | ccd6 | 1113.17 | 947.5 | 2.98324 | 1.73205 | 0.00140907 | 0.000818097 | 7.96185 | 0.999986 | 0.769001 | 0.492 | 10.278 | 7.91287 | A | F | 7.37e+21 | 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