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 | X042720.30+710417.9 | chandra | ccd7 | 202.408 | 626.864 | 89.2898 | 9.58285 | 0.00607921 | 0.000652439 | 64.2052 | 1 | 0.489382 | 0.39155 | 353.112 | 1.38333 | 65.6612 | 22.9322 | -0.482304 | 0.131419 | F | F | 1.07e+21 | 4.78058e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X042901.99+710110.5 | chandra | ccd6 | 159.612 | 606.569 | 97.3833 | 10.3817 | 0.00663029 | 0.00070683 | 46.6465 | 1 | 5.33172 | 5.33172 | 0 | 9.85881 | 52.5605 | 45.3472 | -0.073675 | 0.117654 | F | F | 1.07e+21 | 9.69659e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X042916.86+705832.4 | chandra | ccd5 | 997.722 | 640.981 | 74.915 | 11.8051 | 0.00510052 | 0.000803739 | 11.6876 | 1 | 4.51684 | 4.38326 | 91.513 | 11.9513 | 66.8372 | 5.96765 | -0.836065 | 0.20822 | F | F | 1.07e+21 | 5.21908e-14 | 1 | dx |
Report | srcpi bgdpi arf rmf | 1 | X042628.87+705209.6 | chandra | ccd2 | 1035.61 | 704.019 | 112.543 | 12.2145 | 0.00766575 | 0.000831975 | 18.5901 | 1 | 7.50709 | 5.35818 | 79.8162 | 12.0241 | 77.8027 | 44.4355 | -0.272969 | 0.109887 | F | F | 1.06e+21 | 1.18986e-13 | 1 | dsxf |
Report | srcpi bgdpi arf | 1 | X042524.50+705159.7 | chandra | ccd3 | 705.934 | 335.797 | 73.4663 | 12.6682 | 0.00500192 | 0.000862508 | 7.87566 | 1 | 9.57182 | 9.57182 | 0 | 14.2959 | 65.3194 | 21.6355 | -0.502374 | 0.172581 | F | F | 1.06e+21 | 7.18608e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 3 | X042739.48+710247.3 | chandra | ccd6 | 978.233 | 799.117 | 42.44 | 6.71711 | 0.0028895 | 0.000457331 | 20.3287 | 1 | 0.856842 | 0.544641 | 127.566 | 2.98946 | 23.9461 | 19.5153 | -0.101948 | 0.178276 | F | F | 1.07e+21 | 3.07944e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X042702.85+710337.2 | chandra | ccd7 | 374.994 | 544.079 | 38.6559 | 6.39842 | 0.00263185 | 0.000435631 | 27.7961 | 1 | 0.325758 | 0.325758 | 0 | 0.196652 | 26.9152 | 12.9152 | -0.35149 | 0.197013 | F | F | 1.07e+21 | 2.03262e-14 | 1 | dsbx |
Report | srcpi bgdpi arf | 2 | X042820.05+705822.2 | chandra | ccd6 | 573.182 | 261.25 | 57.0066 | 8.79423 | 0.00388125 | 0.000598748 | 32.9491 | 1 | 2.60217 | 1.43742 | 12.9683 | 8.16271 | 22.1113 | 33.8953 | 0.210403 | 0.159579 | A | F | 1.07e+21 | 4.77178e-14 | 1 | dx |
Report | srcpi bgdpi arf | 6 | X042732.19+710237.0 | chandra | ccd6 | 1050.41 | 777.929 | 29.7006 | 5.44983 | 0.00202215 | 0.000371048 | 14.2266 | 1 | 0.659871 | 0.659871 | 0 | 2.51109 | 10.9152 | 17.661 | 0.236061 | 0.232895 | F | T | 1.07e+21 | 2.13391e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 3 | X042633.22+710239.3 | chandra | ccd7 | 668.429 | 426.768 | 17.3944 | 4.17066 | 0.00118428 | 0.000283956 | 12.5077 | 1 | 0.533659 | 0.332596 | 54.4226 | 2.77532 | 14.789 | -0.158284 | -1 | 0.478132 | F | F | 1.07e+21 | 9.34997e-15 | 1 | dsx |
Report | srcpi bgdpi arf | 10 | X042712.70+710135.7 | chandra | ccd7 | 277.314 | 297.282 | 15.547 | 4.43789 | 0.00105851 | 0.00030215 | 11.1793 | 1 | 0.454193 | 0.454193 | 0 | 2.25493 | 13.6609 | -0.169527 | -1 | 0.504463 | F | F | 1.07e+21 | 8.40902e-15 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X042639.30+705457.5 | chandra | ccd2 | 930.35 | 1044.55 | 15.7068 | 5.66369 | 0.00106984 | 0.000385773 | 6.82697 | 1 | 3.29229 | 2.26175 | 115.089 | 9.03426 | 9.06933 | 5.63747 | -0.233352 | 0.38979 | F | F | 1.07e+21 | 1.52343e-14 | 1 | dx |
Report | srcpi bgdpi arf | 5 | X042627.06+710536.6 | chandra | ccd7 | 727.961 | 786.885 | 12.6505 | 4.7081 | 0.000861294 | 0.000320546 | 21.3981 | 1 | 0.715284 | 0.492 | 140.416 | 3.56572 | 8.82524 | 3.82524 | -0.395242 | 0.403035 | F | F | 1.07e+21 | 6.85559e-15 | 1 | dbx |
Report | srcpi bgdpi arf | 4 | X042754.71+710557.4 | chandra | ccd6 | 828.278 | 1185.39 | 8.47276 | 4.1225 | 0.000576862 | 0.000280677 | 11.6687 | 1 | 0.948104 | 0.492 | 60.0918 | 4.61916 | 0.824254 | 7.69244 | 0.806438 | 0.627837 | A | F | 1.08e+21 | 6.76155e-15 | 1 | dx |
Report | srcpi bgdpi arf | 7 | X042657.25+710734.0 | chandra | ccd7 | 429.625 | 1024.88 | 8.60999 | 4.1225 | 0.000586202 | 0.000280676 | 13.7869 | 1 | 0.748106 | 0.492 | 120.875 | 3.85821 | 4.88857 | 3.77714 | -0.128256 | 0.48425 | A | F | 1.08e+21 | 5.15257e-15 | 1 | dx |
Report | srcpi bgdpi arf | 4 | X042649.80+710211.8 | chandra | ccd7 | 503.786 | 370.214 | 6.40715 | 3.78388 | 0.000436223 | 0.000257621 | 8.3213 | 1 | 0.492 | 0.492 | 152.496 | 1.9674 | 3.91531 | 2.49184 | -0.222169 | 0.612093 | F | F | 1.07e+21 | 3.58125e-15 | 1 | dx |
Report | srcpi bgdpi arf | 9 | X042616.01+710902.0 | chandra | ccd7 | 835.75 | 1204.5 | 7.3464 | 4.1225 | 0.000500171 | 0.000280676 | 5.71293 | 0.999991 | 1.51972 | 0.802156 | 123.42 | 6.58344 | 4.68716 | 2.74863 | -0.260703 | 0.578473 | A | F | 1.08e+21 | 4.72075e-15 | 1 | dx |
Report | srcpi bgdpi arf | 6 | X042707.03+710731.1 | chandra | ccd7 | 333.167 | 1019 | 5.74592 | 3.59808 | 0.000391204 | 0.000244971 | 11.3992 | 1 | 0.492 | 0.492 | 111.355 | 3.76887 | 5 | 0.74592 | -0.740365 | 0.789465 | F | T | 1.08e+21 | 3.54515e-15 | 1 | dx |
Report | srcpi bgdpi arf | 8 | X042615.36+710808.4 | chandra | ccd7 | 842.5 | 1095.7 | 4.74827 | 3.39792 | 0.000323281 | 0.000231343 | 9.4639 | 1 | 0.661639 | 0.492 | 4.30782 | 5.92835 | 0 | 3.8112 | 1 | 1.2008 | F | F | 1.07e+21 | 2.77057e-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