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 | X123049.25+122329.3 | chandra | ccd7 | 154.482 | 745.949 | 638.81 | 35.3977 | 0.140613 | 0.00779165 | 25.5572 | 1 | 1.84204 | 0.334709 | 340.906 | 0.185607 | 1096.2 | 171.065 | -0.730024 | 0.0376504 | A | F | 1.94e+20 | 8.68643e-13 | 1 | dscxf |
| Report | srcpi bgdpi arf rmf | 2 | X123049.01+122330.5 | chandra | ccd7 | 161.623 | 748.396 | 262.865 | 33.1343 | 0.0578612 | 0.00729344 | 10.5166 | 1 | 1.5 | 0.342035 | 341.15 | 0.159261 | 212.239 | 29.8631 | -0.753302 | 0.106376 | A | F | 1.94e+20 | 4.33045e-13 | 1 | dscx |
| Report | srcpi bgdpi arf rmf | 3 | X123048.63+122332.7 | chandra | ccd7 | 173.035 | 752.892 | 763.299 | 37.7838 | 0.168016 | 0.00831688 | 30.5376 | 1 | 0.576554 | 0.402218 | 338.676 | 0.120218 | 554.394 | 102.737 | -0.687318 | 0.0518401 | F | F | 1.93e+20 | 1.25787e-12 | 1 | dsx |
| Report | srcpi bgdpi arf | 4 | X123048.24+122335.3 | chandra | ccd7 | 184.61 | 758.149 | 69.5988 | 24.8432 | 0.0153199 | 0.00546843 | 2.78447 | 0.99699 | 1.02119 | 0.529895 | 346.724 | 0.119463 | 78.2544 | 14.8765 | -0.680525 | 0.216698 | T | F | 1.93e+20 | 1.14775e-13 | 1 | dsx |
| Report | srcpi bgdpi arf rmf | 7 | X123049.39+122328.5 | chandra | ccd7 | 150.299 | 744.449 | 2876.97 | 61.1722 | 0.633272 | 0.0134651 | 115.1 | 1 | 0.94331 | 0.328461 | 338.708 | 0.26119 | 1983.81 | 448.496 | -0.631217 | 0.0249748 | A | F | 1.94e+20 | 4.73903e-12 | 1 | dscx |
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