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 | X123048.88+122331.1 | chandra | ccd7 | 356.446 | 311.095 | 143.503 | 15.0336 | 0.0305127 | 0.00319656 | 5.2815 | 1 | 0.492 | 0.492 | 31.21 | 0.748456 | F | F | 1.94e+20 | 2.15026e-13 | 1 | dbx | ||||
Report | srcpi bgdpi arf rmf | 2 | X123048.62+122332.5 | chandra | ccd7 | 364.591 | 314.444 | 1203.27 | 45.8837 | 0.255849 | 0.00975617 | 44.2852 | 1 | 0.677142 | 0.462653 | 339.892 | 0.740949 | T | T | 1.93e+20 | 1.52369e-12 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 3 | X123048.24+122335.4 | chandra | ccd7 | 376.017 | 320.357 | 97.9481 | 28.5895 | 0.0208265 | 0.00607893 | 3.60488 | 0.999804 | 0.665185 | 0.665185 | 0 | 0.752913 | F | F | 1.93e+20 | 1.46653e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 5 | X123047.54+122340.2 | chandra | ccd7 | 396.897 | 330.036 | 113.167 | 21.0935 | 0.0240624 | 0.00448505 | 4.165 | 0.999977 | 1.5 | 1.5 | 0 | 0.818607 | T | F | 1.93e+20 | 1.69273e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf rmf | 6 | X123049.37+122328.5 | chandra | ccd7 | 342.259 | 306.211 | 7020.2 | 95.9948 | 1.49269 | 0.0204112 | 258.372 | 1 | 0.66358 | 0.66358 | 0 | 0.780419 | T | F | 1.94e+20 | 1.05217e-11 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 10 | X123050.18+122323.4 | chandra | ccd7 | 318.096 | 295.915 | 96.7441 | 18.4387 | 0.0205705 | 0.00392059 | 3.56057 | 0.999776 | 1.49 | 1.49 | 0 | 0.87356 | T | F | 1.94e+20 | 1.45127e-13 | 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