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 | 2 | X121037.04+102504.2 | chandra | ccd7 | 345.389 | 287.389 | 8.98139 | 3 | 0.00762113 | 0.00254564 | 27.1303 | 1 | 0.492 | 0.492 | 58.9486 | 2.49056 | F | F | 1.75e+20 | 0 | 1 | d | |||||
Report | 1 | X121040.54+102725.3 | chandra | ccd7 | 240.667 | 574.333 | 5.92516 | 2.44949 | 0.00502777 | 0.00207851 | 17.8982 | 1 | 0.809639 | 0.492 | 2.5641 | 4.13233 | A | F | 1.76e+20 | 0 | 1 | d | |||||
Report | 3 | X121016.30+102216.9 | chandra | ccd6 | 624.5 | 993.5 | 2.99374 | 1.73205 | 0.00254033 | 0.00146973 | 17.4721 | 1 | 0.673699 | 0.492 | 153.435 | 3.76963 | F | F | 1.72e+20 | 0 | 1 | d | |||||
Report | 1 | X120937.18+102857.7 | chandra | ccd3 | 879 | 281.5 | 2 | 1.41421 | 0.00169709 | 0.00120003 | 13.5185 | 0.999998 | 1.12227 | 0.492 | 80.5377 | 12.853 | A | F | 1.72e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 1 | X120951.19+101942.8 | chandra | ccd2 | 224.5 | 100.5 | 1.94843 | 1.41422 | 0.00165333 | 0.00120003 | 11.0604 | 0.999528 | 0.492 | 0.492 | 90 | 10.2533 | F | F | 1.6e+20 | 2.06772e-14 | 1 | dx | ||||
Report | 1 | X121004.77+101704.5 | chandra | ccd6 | 970.5 | 358.5 | 0.999955 | 1 | 0.000848508 | 0.000848546 | 5.83594 | 0.999577 | 0.492 | 0.492 | 90 | 9.61774 | F | F | 1.68e+20 | 0 | 1 | d | |||||
Report | 2 | X121019.50+101920.3 | chandra | ccd6 | 528.5 | 634.5 | 0.998592 | 1 | 0.000847352 | 0.000848546 | 5.82799 | 0.999577 | 0.492 | 0.492 | 90 | 5.9488 | F | F | 1.7e+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