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 | 1 | X121945.23+124753.8 | chandra | ccd7 | 534.593 | 844.176 | 38.5265 | 6.94461 | 0.00756449 | 0.00136354 | 17.0999 | 1 | 0.520193 | 0.520193 | 0 | 0.284596 | F | F | 3.37e+20 | 5.54915e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X122020.73+125133.2 | chandra | ccd2 | 895.894 | 543.924 | 29.538 | 5.7446 | 0.00579963 | 0.00112792 | 46.1537 | 1 | 2.14959 | 1.83047 | 162.446 | 9.3855 | F | F | 3.49e+20 | 7.94924e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 9 | X121944.89+124748.3 | chandra | ccd7 | 544.417 | 832.417 | 23.5519 | 4.89898 | 0.00462429 | 0.00096189 | 10.4534 | 1 | 0.49517 | 0.492 | 123.523 | 0.357618 | F | F | 3.37e+20 | 3.39473e-14 | 1 | dpx | ||||
Report | 3 | X121953.02+124914.1 | chandra | ccd7 | 303.199 | 1007.26 | 14.2852 | 3.83879 | 0.00280482 | 0.000753726 | 6.34046 | 1 | 0.550801 | 0.550801 | 0 | 2.26448 | F | F | 3.4e+20 | 0 | 1 | ds | |||||
Report | srcpi bgdpi arf | 2 | X121946.72+125045.5 | chandra | ccd6 | 566.405 | 144.017 | 13.321 | 3.64979 | 0.00261551 | 0.000716617 | 20.5004 | 1 | 0.82936 | 0.443177 | 40.4279 | 2.63567 | F | F | 3.38e+20 | 2.78167e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X121945.13+124749.7 | chandra | ccd7 | 537.1 | 835.2 | 9.67792 | 3.16228 | 0.00190021 | 0.000620898 | 4.29552 | 0.999735 | 0.492 | 0.492 | 36.5813 | 0.342428 | F | F | 3.37e+20 | 1.39387e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X121934.56+124646.7 | chandra | ccd7 | 851.375 | 707.25 | 7.7988 | 2.82843 | 0.00153125 | 0.000555348 | 3.46148 | 0.997705 | 0.624023 | 0.492 | 179.069 | 2.86097 | F | F | 3.18e+20 | 1.17134e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 7 | X121958.91+124821.3 | chandra | ccd7 | 127.5 | 899.643 | 6.68998 | 2.64576 | 0.00131354 | 0.000519481 | 2.96934 | 0.99389 | 0.751504 | 0.492 | 168.315 | 3.43717 | A | F | 3.41e+20 | 1.07751e-14 | 1 | dx | ||||
Report | 1 | X121949.78+125026.1 | chandra | ccd6 | 474.9 | 104.1 | 4.90217 | 2.23607 | 0.000962517 | 0.000439041 | 7.54423 | 0.999995 | 0.554847 | 0.492 | 7.46571 | 2.57254 | F | F | 3.39e+20 | 0 | 1 | d | |||||
Report | 5 | X121937.40+125003.8 | chandra | ccd6 | 842.9 | 58.8999 | 4.89038 | 2.23607 | 0.000960201 | 0.000439041 | 7.52608 | 0.999995 | 0.536926 | 0.492 | 23.4238 | 2.62623 | F | F | 3.19e+20 | 0 | 1 | d | |||||
Report | 1 | X122018.50+124057.1 | chandra | ccd3 | 877.5 | 304 | 3.52808 | 2.00002 | 0.000692719 | 0.000392693 | 5.45179 | 0.999081 | 0.546444 | 0.492 | 145.278 | 10.9268 | F | F | 3.39e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X121950.57+125146.1 | chandra | ccd6 | 451.5 | 266.833 | 2.9101 | 1.73205 | 0.000571383 | 0.00034008 | 4.47851 | 0.999053 | 0.492 | 0.492 | 49.7312 | 3.86814 | F | F | 3.4e+20 | 6.6959e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X122003.49+125315.7 | chandra | ccd6 | 67.5 | 449 | 1.81732 | 1.41422 | 0.000356822 | 0.000277675 | 2.79678 | 0.990828 | 0.492 | 0.492 | 90 | 6.83289 | F | F | 3.44e+20 | 5.45138e-15 | 1 | dx |
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