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 | 2 | X094202.05+042244.5 | chandra | ccd7 | 362.003 | 738.861 | 55.5473 | 7.56964 | 0.0136394 | 0.0018587 | 32.7276 | 1 | 0.398757 | 0.398757 | 0 | 0.110508 | F | F | 3.27e+20 | 9.72621e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X094146.23+041739.2 | chandra | ccd7 | 843.043 | 118.376 | 15.3257 | 5.12468 | 0.00376317 | 0.00125835 | 9.02965 | 1 | 0.890347 | 0.890347 | 0 | 6.43453 | F | F | 3.24e+20 | 3.28325e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 9 | X094201.83+041938.0 | chandra | ccd7 | 368.634 | 359.737 | 16.5961 | 4.11333 | 0.00407513 | 0.00101002 | 9.77815 | 1 | 0.831792 | 0.290094 | 103.025 | 3.04177 | A | F | 3.26e+20 | 3.095e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 3 | X094149.80+042154.2 | chandra | ccd7 | 734.365 | 636.735 | 14.1795 | 3.946 | 0.00348171 | 0.000968924 | 8.35433 | 1 | 0.355338 | 0.355338 | 0 | 3.23319 | F | F | 3.27e+20 | 2.59101e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 6 | X094202.04+042609.2 | chandra | ccd7 | 362.44 | 1154.9 | 15.1645 | 3.89416 | 0.0037236 | 0.000956201 | 8.93467 | 1 | 1.13931 | 0.655798 | 13.2513 | 3.48104 | F | F | 3.28e+20 | 2.8888e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X094212.77+042542.7 | chandra | ccd6 | 1014.6 | 797.5 | 9.86178 | 3.16228 | 0.00242342 | 0.000777093 | 18.7016 | 1 | 0.629568 | 0.492 | 5.97488 | 3.98985 | F | F | 3.28e+20 | 2.55784e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X094145.02+042001.1 | chandra | ccd7 | 879.1 | 406.4 | 9.61325 | 3.16229 | 0.00236049 | 0.000776484 | 5.66397 | 0.999989 | 0.706091 | 0.555761 | 146.626 | 5.07875 | F | F | 3.26e+20 | 1.80438e-14 | 1 | dx | ||||
Report | 7 | X094156.59+042622.6 | chandra | ccd7 | 527.357 | 1181.79 | 6.81934 | 2.64576 | 0.00167446 | 0.000649653 | 4.01784 | 0.999183 | 0.681305 | 0.492 | 133.782 | 3.97689 | F | F | 3.28e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 8 | X094159.39+042639.1 | chandra | ccd7 | 442.3 | 1215.3 | 4.89071 | 2.23607 | 0.00120089 | 0.000549057 | 2.88153 | 0.990474 | 0.492 | 0.492 | 156.137 | 4.04927 | F | F | 3.29e+20 | 1.01752e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X094152.74+042235.2 | chandra | ccd7 | 644.5 | 719.5 | 4.8872 | 2.23607 | 0.00120003 | 0.000549056 | 2.87946 | 0.990474 | 0.492 | 0.492 | 45 | 2.40824 | F | F | 3.27e+20 | 8.81035e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X094209.64+042342.4 | chandra | ccd6 | 1109.75 | 553 | 3.92311 | 2 | 0.000964059 | 0.000491477 | 7.43967 | 0.999989 | 0.492 | 0.492 | 52.0181 | 2.0807 | F | F | 3.28e+20 | 9.85492e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X094221.90+042812.1 | chandra | ccd6 | 737 | 1101.25 | 3.73827 | 2.00001 | 0.000918636 | 0.000491479 | 7.08914 | 0.999989 | 1.15896 | 0.909327 | 139.265 | 7.36295 | F | F | 3.29e+20 | 1.08473e-14 | 1 | dx | ||||
Report | 4 | X094223.20+042754.2 | chandra | ccd6 | 697.5 | 1065 | 1.81528 | 1.41422 | 0.000446085 | 0.000347529 | 3.44245 | 0.997087 | 0.760713 | 0.492 | 14.0362 | 7.36678 | A | F | 3.29e+20 | 0 | 1 | d | |||||
Report | 5 | X094216.32+042439.1 | chandra | ccd6 | 906.75 | 668.25 | 3.9696 | 2 | 0.000975484 | 0.000491477 | 7.52783 | 0.999989 | 0.492 | 0.492 | 45 | 3.99486 | F | F | 3.28e+20 | 0 | 1 | d |
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