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 | 3 | X103638.12+124745.9 | chandra | ccd6 | 280.733 | 511.455 | 46.6687 | 6.83145 | 0.00922037 | 0.00134969 | 73.4583 | 1 | 2.82814 | 1.92264 | 1.63967 | 6.24766 | F | F | 2.34e+20 | 1.0701e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X103617.07+124252.9 | chandra | ccd7 | 765.854 | 944.79 | 33.9575 | 5.82731 | 0.006709 | 0.0011513 | 35.6352 | 1 | 0.650947 | 0.479428 | 118.1 | 1.78848 | F | F | 2.33e+20 | 4.96861e-14 | 1 | dsx | ||||
Report | 5 | X103627.42+124126.2 | chandra | ccd7 | 457.883 | 768.724 | 25.4802 | 5.04779 | 0.00503414 | 0.000997296 | 26.7391 | 1 | 0.41019 | 0.41019 | 0 | 1.32328 | F | F | 2.33e+20 | 0 | 1 | ds | |||||
Report | 3 | X103622.10+124221.4 | chandra | ccd7 | 615.8 | 880.3 | 9.80339 | 3.16228 | 0.00193686 | 0.000624773 | 10.2877 | 1 | 0.492 | 0.492 | 42.2538 | 0.545168 | F | F | 2.33e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X103642.99+124847.2 | chandra | ccd6 | 135.625 | 635.5 | 7.35229 | 2.82844 | 0.00145259 | 0.000558817 | 11.5728 | 1 | 1.17486 | 0.662374 | 144.975 | 7.76474 | A | F | 2.34e+20 | 1.83165e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X103711.55+123737.6 | chandra | ccd3 | 462.5 | 664.125 | 6.58268 | 2.82846 | 0.00130054 | 0.00055882 | 10.6761 | 1 | 2.61554 | 1.23723 | 135.011 | 12.53 | A | F | 2.36e+20 | 1.82295e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X103626.28+124959.9 | chandra | ccd6 | 632.3 | 783.3 | 4.80556 | 2.23607 | 0.000949436 | 0.000441782 | 7.56414 | 0.999996 | 0.598016 | 0.492 | 105.482 | 7.50558 | F | F | 2.35e+20 | 1.117e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X103611.03+124253.4 | chandra | ccd7 | 944.9 | 945.5 | 4.75355 | 2.23608 | 0.000939161 | 0.000441782 | 4.9884 | 0.99964 | 0.649616 | 0.492 | 8.4292 | 3.24426 | F | F | 2.33e+20 | 7.63471e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X103655.84+124430.5 | chandra | ccd2 | 1070.3 | 471.9 | 4.7325 | 2.23608 | 0.000935003 | 0.000441782 | 7.70081 | 0.999997 | 0.945265 | 0.492 | 178.913 | 7.96086 | A | F | 2.37e+20 | 1.26009e-14 | 1 | dx | ||||
Report | 2 | X103719.57+124733.5 | chandra | ccd2 | 365.1 | 844.5 | 4.41961 | 2.23608 | 0.000873184 | 0.000441784 | 7.19166 | 0.999953 | 1.37789 | 0.492 | 52.5806 | 14.4044 | A | F | 2.4e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X103720.66+124624.9 | chandra | ccd2 | 332.389 | 704.944 | 6.85485 | 3.00006 | 0.00135431 | 0.000592722 | 11.1543 | 1 | 1.3714 | 0.492 | 19.2494 | 14.3015 | A | F | 2.4e+20 | 1.99303e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X103632.62+124135.7 | chandra | ccd7 | 302.75 | 787.5 | 3.86098 | 2 | 0.000762816 | 0.000395142 | 4.05173 | 0.997565 | 0.492 | 0.492 | 2.35031e-08 | 2.23903 | F | F | 2.33e+20 | 5.94041e-15 | 1 | dx | ||||
Report | 6 | X103630.32+124708.3 | chandra | ccd6 | 512.167 | 434.5 | 2.92573 | 1.73205 | 0.000578038 | 0.000342203 | 4.60521 | 0.999198 | 0.492 | 0.492 | 18.4349 | 4.86061 | F | F | 2.33e+20 | 0 | 1 | d | |||||
Report | 4 | X103624.83+124907.1 | chandra | ccd6 | 675.5 | 676 | 1.91981 | 1.41422 | 0.000379297 | 0.000279407 | 3.02185 | 0.991878 | 0.492 | 0.492 | 26.5651 | 6.61076 | F | F | 2.34e+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