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 | 2 | X182615.07-145054.2 | chandra | ccd7 | 468.09 | 788.06 | 1422.98 | 38.8127 | 0.282321 | 0.00770049 | 155.773 | 1 | 0.491704 | 0.416706 | 305.255 | 1.19416 | F | F | 8.87e+21 | 0 | 1 | ds | |||||
| Report | 1 | X182623.35-144606.5 | chandra | ccd6 | 119.5 | 325.5 | 2.94849 | 1.73205 | 0.000584981 | 0.00034364 | 4.44918 | 0.998906 | 0.492 | 0.492 | 90 | 4.47067 | F | F | 8.99e+21 | 0 | 1 | d | |||||
| Report | 2 | X182621.21-144352.5 | chandra | ccd6 | 182.5 | 597.833 | 2.74143 | 1.73206 | 0.000543901 | 0.000343641 | 4.13673 | 0.998906 | 0.856757 | 0.492 | 23.4875 | 6.62609 | A | F | 9.19e+21 | 0 | 1 | d | |||||
| Report | 3 | X182620.03-144146.4 | chandra | ccd6 | 217.389 | 854.167 | 7.94242 | 3.00002 | 0.00157578 | 0.000595205 | 11.9849 | 1 | 2.9663 | 1.44123 | 2.28068 | 8.71832 | A | F | 9.36e+21 | 0 | 1 | d | |||||
| Report | 4 | X182622.81-144644.4 | chandra | ccd6 | 135.746 | 248.914 | 44.6568 | 6.68257 | 0.00885998 | 0.00132583 | 67.3857 | 1 | 1.08824 | 0.724393 | 31.1104 | 3.82587 | F | F | 8.95e+21 | 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