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 | X123049.04+122329.8 | chandra | ccd7 | 135.696 | 779.394 | 376.729 | 32.6094 | 0.0800723 | 0.00693099 | 13.1266 | 1 | 1.47667 | 1.47667 | 0 | 0.295918 | T | F | 1.94e+20 | 5.1704e-13 | 1 | dscxf | ||||
Report | srcpi bgdpi arf rmf | 2 | X123048.95+122330.7 | chandra | ccd7 | 138.291 | 781.233 | 369.104 | 39.1201 | 0.0784518 | 0.00831485 | 12.8609 | 1 | 1.13017 | 1.13017 | 0 | 0.273741 | T | F | 1.94e+20 | 5.78754e-13 | 1 | dscx | ||||
Report | srcpi bgdpi arf rmf | 3 | X123048.63+122332.4 | chandra | ccd7 | 147.82 | 784.808 | 958.736 | 42.2637 | 0.203776 | 0.00898299 | 33.4058 | 1 | 0.482048 | 0.482048 | 0 | 0.244593 | F | F | 1.93e+20 | 1.50352e-12 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 4 | X123048.30+122334.6 | chandra | ccd7 | 157.765 | 789.108 | 125.298 | 24.3208 | 0.0266317 | 0.00516931 | 4.36583 | 0.999989 | 1.5 | 0.423784 | 335.619 | 0.2403 | A | F | 1.93e+20 | 1.96798e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 6 | X123050.20+122325.0 | chandra | ccd7 | 101.238 | 769.768 | 54.2415 | 24.9741 | 0.0115288 | 0.00530816 | 1.88997 | 0.96866 | 1.16797 | 1.16797 | 0 | 0.508188 | T | F | 1.94e+20 | 8.51112e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 7 | X123049.39+122328.4 | chandra | ccd7 | 125.203 | 776.483 | 3620.44 | 69.6519 | 0.769512 | 0.0148043 | 126.149 | 1 | 0.546896 | 0.546896 | 0 | 0.346852 | F | F | 1.94e+20 | 5.67279e-12 | 1 | dsx |
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