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 | X124711.01+120626.8 | chandra | ccd6 | 459.351 | 794.37 | 30.9019 | 5.55895 | 0.00607125 | 0.00109216 | 16.2017 | 1 | 1.71987 | 1.06986 | 10.7934 | 4.04436 | T | F | 2.22e+20 | 6.51721e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 4 | X124721.35+120731.0 | chandra | ccd7 | 876.024 | 187.763 | 15.2356 | 3.90328 | 0.00299332 | 0.000766872 | 15.0331 | 1 | 0.634788 | 0.344537 | 78.4888 | 2.40051 | F | F | 2.23e+20 | 2.22856e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X124707.16+120411.6 | chandra | ccd6 | 574.125 | 519.443 | 14.7885 | 3.84558 | 0.00290547 | 0.000755535 | 7.75355 | 1 | 1.66889 | 1.66889 | 0 | 6.45256 | F | F | 2.21e+20 | 3.26841e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 6 | X124702.60+120730.0 | chandra | ccd6 | 710.102 | 922.837 | 8.18335 | 4.37001 | 0.00160777 | 0.000858568 | 4.2905 | 0.999594 | 0.335964 | 0.335964 | 0 | 4.81561 | F | F | 2.2e+20 | 1.75567e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X124635.58+121217.2 | chandra | ccd2 | 675.611 | 434.389 | 6.84651 | 3.00005 | 0.00134511 | 0.00058941 | 10.5901 | 1 | 2.47894 | 1.86375 | 80.03 | 11.053 | F | F | 2.15e+20 | 1.91065e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X124723.19+121018.1 | chandra | ccd7 | 820.643 | 526.929 | 6.78582 | 2.64576 | 0.00133319 | 0.000519803 | 6.69564 | 0.999988 | 0.492 | 0.492 | 158.863 | 0.944832 | F | F | 2.28e+20 | 9.7587e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X124703.00+120430.8 | chandra | ccd6 | 697.786 | 558.072 | 6.73651 | 2.64576 | 0.0013235 | 0.000519803 | 3.53193 | 0.998621 | 0.958158 | 0.492 | 167.743 | 6.75054 | A | F | 2.2e+20 | 1.49787e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X124723.90+121005.9 | chandra | ccd7 | 799.7 | 502.1 | 4.72059 | 2.23608 | 0.000927439 | 0.000439314 | 4.65786 | 0.999318 | 0.528476 | 0.492 | 66.2552 | 1.04149 | F | F | 2.28e+20 | 6.76946e-15 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X124640.69+121123.5 | chandra | ccd2 | 523.3 | 325.1 | 4.63208 | 2.23608 | 0.00091005 | 0.000439315 | 7.16484 | 0.999995 | 1.40611 | 0.492 | 60.3715 | 9.65777 | A | F | 2.16e+20 | 1.28281e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X124715.48+121407.2 | chandra | ccd7 | 1050.5 | 992.5 | 2.89667 | 1.73205 | 0.000569099 | 0.000340291 | 2.85818 | 0.979304 | 0.492 | 0.492 | 90 | 4.36048 | F | F | 2.26e+20 | 5.12156e-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