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 rmf | 4 | X122121.95+301037.3 | chandra | ccd6 | 1156.87 | 825.329 | 19531 | 149.37 | 4.15437 | 0.031772 | 22659.6 | 1 | 3.58515 | 3.03736 | 91.4308 | 9.46785 | F | F | 1.94e+20 | 5.20058e-11 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X122118.13+301544.4 | chandra | ccd5 | 638.097 | 650.14 | 51.0713 | 15.0178 | 0.0108633 | 0.00319441 | 4.43004 | 0.999984 | 7.44008 | 2.26623 | 96.0961 | 13.7976 | A | F | 1.92e+20 | 1.05809e-13 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 1 | X122254.80+300646.0 | chandra | ccd3 | 539.138 | 566.851 | 44.7164 | 8.85018 | 0.00951152 | 0.0018825 | 7.71326 | 1 | 5.7565 | 3.64277 | 18.7866 | 13.0201 | F | F | 2.07e+20 | 1.42571e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X122120.21+301610.9 | chandra | ccd5 | 583.312 | 704.076 | 37.1895 | 11.3372 | 0.0079105 | 0.00241152 | 3.2259 | 0.999147 | 16.8947 | 2.18056 | 60.7888 | 13.9168 | A | F | 1.92e+20 | 7.72754e-14 | 1 | dscx | ||||
Report | srcpi bgdpi arf | 2 | X122206.37+300645.2 | chandra | ccd7 | 636.312 | 1217.7 | 12.3356 | 3.77552 | 0.00262388 | 0.000803083 | 8.90496 | 1 | 0.706151 | 0.706151 | 0 | 3.1986 | F | F | 2.05e+20 | 2.06785e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X122219.35+300340.4 | chandra | ccd7 | 293.2 | 841.7 | 9.77343 | 3.16228 | 0.00207888 | 0.000672639 | 7.05535 | 0.999999 | 0.643177 | 0.492 | 157.097 | 5.21592 | F | F | 2.06e+20 | 1.77252e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 1 | X122213.84+301338.0 | chandra | ccd2 | 1004.5 | 540.227 | 8.81422 | 3.31667 | 0.00187484 | 0.000705478 | 14.2213 | 1 | 2.06003 | 1.52283 | 119.047 | 9.88982 | F | F | 1.95e+20 | 2.62379e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X122227.59+301018.8 | chandra | ccd2 | 641.773 | 135.682 | 9.38492 | 3.31666 | 0.00199624 | 0.000705476 | 15.1421 | 1 | 3.14498 | 1.5527 | 170.382 | 8.99533 | A | F | 2.04e+20 | 2.70048e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X122154.66+301108.4 | chandra | ccd6 | 294.611 | 888.056 | 8.34071 | 3.00001 | 0.00177413 | 0.000638123 | 9.67678 | 1 | 1.9236 | 0.92481 | 118.333 | 6.57995 | A | F | 1.95e+20 | 2.44012e-14 | 1 | dx | ||||
Report | 4 | X122156.19+300331.6 | chandra | ccd7 | 904.333 | 823.667 | 5.88741 | 2.44949 | 0.00125229 | 0.000521024 | 4.25007 | 0.999155 | 0.492 | 0.492 | 45 | 1.04387 | F | F | 1.98e+20 | 0 | 1 | d | |||||
Report | srcpi bgdpi arf | 3 | X122156.03+300225.0 | chandra | ccd7 | 908.5 | 688.167 | 5.80883 | 2.44949 | 0.00123558 | 0.000521024 | 4.19334 | 0.999155 | 0.492 | 0.492 | 12.3876 | 2.1491 | F | F | 1.98e+20 | 9.07316e-15 | 1 | dx | ||||
Report | 1 | X122158.98+300814.0 | chandra | ccd6 | 180.75 | 533.5 | 3.88432 | 2 | 0.000826221 | 0.000425414 | 4.50654 | 0.998979 | 0.600932 | 0.492 | 24.922 | 3.74177 | F | F | 1.96e+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