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 | 1 | X122142.80+112412.2 | chandra | ccd7 | 477.044 | 205.779 | 21.8023 | 4.66929 | 0.00430753 | 0.000922523 | 9.30465 | 1 | 1.94685 | 1.94685 | 0 | 6.30326 | F | F | 2.45e+20 | 3.79492e-14 | 1 | dsbx | ||||
| Report | srcpi bgdpi arf | 2 | X122121.25+112903.3 | chandra | ccd7 | 1120.83 | 797.493 | 14.3043 | 5.36286 | 0.00282613 | 0.00105955 | 6.1047 | 0.999999 | 0.795566 | 0.795566 | 0 | 5.02879 | F | F | 2.48e+20 | 2.37606e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X122220.85+112653.5 | chandra | ccd2 | 920.906 | 540.861 | 17.2523 | 5.46867 | 0.00340857 | 0.00108046 | 4.84988 | 0.999977 | 6.08848 | 2.17093 | 96.0233 | 10.4546 | A | F | 2.46e+20 | 4.73932e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 3 | X122137.56+113042.7 | chandra | ccd7 | 633.539 | 999.37 | 10.6206 | 3.55469 | 0.00209833 | 0.000702306 | 4.53259 | 0.999938 | 0.340954 | 0.340954 | 0 | 0.847343 | F | F | 2.48e+20 | 1.54286e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 7 | X122140.39+113028.9 | chandra | ccd7 | 548.6 | 970.9 | 9.7734 | 3.16228 | 0.00193093 | 0.000624773 | 4.17103 | 0.999804 | 0.492 | 0.492 | 12.8205 | 0.129075 | F | F | 2.48e+20 | 1.41507e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 6 | X122115.51+112743.3 | chandra | ccd7 | 1292.05 | 634.409 | 9.38167 | 3.31666 | 0.00185354 | 0.000655273 | 4.00385 | 0.999412 | 1.49363 | 0.643043 | 163.745 | 6.81535 | A | F | 2.48e+20 | 1.73027e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 1 | X122154.01+113243.4 | chandra | ccd6 | 704.643 | 365.357 | 6.87263 | 2.64575 | 0.00135783 | 0.000522723 | 10.5843 | 1 | 0.492 | 0.492 | 120.85 | 3.90509 | F | F | 2.48e+20 | 1.48547e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X122153.55+113215.3 | chandra | ccd6 | 718.333 | 308.167 | 5.84893 | 2.44949 | 0.00115558 | 0.000483947 | 9.00771 | 1 | 0.600428 | 0.492 | 162.47 | 3.56016 | F | F | 2.48e+20 | 1.25654e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X122126.31+113012.4 | chandra | ccd7 | 969 | 937.5 | 5.77866 | 2.4495 | 0.00114169 | 0.000483948 | 2.46618 | 0.989148 | 0.603866 | 0.492 | 86.0733 | 3.58703 | F | F | 2.49e+20 | 9.04732e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X122135.98+113121.7 | chandra | ccd7 | 680.3 | 1078.3 | 4.82667 | 2.23607 | 0.000953608 | 0.000441782 | 2.0599 | 0.975021 | 0.492 | 0.492 | 95.655 | 1.48475 | F | F | 2.49e+20 | 7.08675e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 3 | X122155.62+113447.8 | chandra | ccd6 | 656.75 | 618.25 | 3.94194 | 2 | 0.000778811 | 0.000395141 | 6.07083 | 0.999922 | 0.492 | 0.492 | 82.9819 | 5.60834 | F | F | 2.49e+20 | 8.84185e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 5 | X122155.49+113205.6 | chandra | ccd6 | 660.5 | 288.5 | 3.91986 | 2 | 0.000774449 | 0.000395141 | 6.03684 | 0.999922 | 0.492 | 0.492 | 2.35031e-08 | 3.91107 | F | F | 2.48e+20 | 8.50458e-15 | 1 | dx | ||||
| Report | 4 | X122154.30+113550.8 | chandra | ccd6 | 696.167 | 746.167 | 2.84585 | 1.73206 | 0.000562256 | 0.000342203 | 4.38279 | 0.999058 | 0.492 | 0.492 | 45 | 6.2728 | F | F | 2.5e+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