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 | 1 | X183723.59-060550.9 | chandra | ccd7 | 1069.12 | 901.292 | 115.372 | 11.1315 | 0.0128083 | 0.00123579 | 57.4221 | 1 | 0.80223 | 0.80223 | 0 | 3.4454 | F | F | 1.64e+22 | 0 | 1 | ds | |||||
Report | 5 | X183731.17-061006.9 | chandra | ccd7 | 839.447 | 381.082 | 116.308 | 10.9406 | 0.0129122 | 0.00121459 | 57.888 | 1 | 0.488215 | 0.488215 | 0 | 1.30566 | F | T | 1.66e+22 | 0 | 1 | ds | |||||
Report | 3 | X183743.98-060751.7 | chandra | ccd7 | 451.036 | 655.916 | 36.9971 | 6.09758 | 0.00410731 | 0.000676934 | 18.4139 | 1 | 0.654941 | 0.654941 | 0 | 3.44995 | F | F | 1.68e+22 | 0 | 1 | ds | |||||
Report | 2 | X183735.46-060921.5 | chandra | ccd7 | 708.75 | 472.75 | 7.7526 | 2.82843 | 0.000860666 | 0.000314002 | 3.85857 | 0.999012 | 0.492 | 0.492 | 103.283 | 1.31656 | F | F | 1.67e+22 | 0 | 1 | d | |||||
Report | 4 | X183742.78-061142.4 | chandra | ccd7 | 487 | 186.333 | 5.64199 | 2.4495 | 0.000626353 | 0.000271935 | 2.80809 | 0.991369 | 0.822328 | 0.492 | 6.80027 | 4.17957 | A | T | 1.68e+22 | 0 | 1 | d | |||||
Report | 7 | X183731.36-061014.6 | chandra | ccd7 | 833.3 | 364.9 | 4.72171 | 2.23608 | 0.000524187 | 0.000248241 | 2.35006 | 0.977519 | 0.492 | 0.492 | 108.014 | 1.43867 | F | F | 1.66e+22 | 0 | 1 | d | |||||
Report | 1 | X183709.99-060805.9 | chandra | ccd6 | 446.833 | 737.5 | 2.94571 | 1.73205 | 0.000327022 | 0.000192286 | 3.88292 | 0.997102 | 0.492 | 0.492 | 3.85109e-08 | 5.18175 | F | F | 1.62e+22 | 0 | 1 | d | |||||
Report | 2 | X183721.88-060721.9 | chandra | ccd6 | 86.5 | 826.929 | 6.82385 | 2.64575 | 0.00075756 | 0.000293722 | 8.99494 | 1 | 0.605674 | 0.492 | 135.818 | 2.61622 | F | F | 1.64e+22 | 0 | 1 | d | |||||
Report | 3 | X183715.64-061004.4 | chandra | ccd6 | 276.193 | 497.084 | 21.5643 | 4.64374 | 0.002394 | 0.000515532 | 28.4252 | 1 | 0.972498 | 0.972498 | 0 | 3.93453 | F | F | 1.63e+22 | 0 | 1 | ds |
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