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 | X152504.77+771934.8 | chandra | ccd5 | 186.593 | 850.736 | 78.1441 | 13.8134 | 0.0104805 | 0.00185261 | 7.3621 | 1 | 7.69263 | 5.93603 | 112.531 | 12.2427 | 55.2191 | 44.7339 | -0.104902 | 0.128233 | F | F | 3.16e+20 | 1.17333e-13 | 1 | dsx |
Report | srcpi bgdpi arf | 1 | X152806.24+770551.2 | chandra | ccd7 | 592.084 | 455.825 | 58.2701 | 8.14095 | 0.00781492 | 0.00109183 | 29.126 | 1 | 1.21794 | 0.633952 | 9.91501 | 4.78149 | 46.9119 | 10.383 | -0.637559 | 0.179692 | F | F | 3.21e+20 | 6.4682e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 11 | X152659.81+770529.2 | chandra | ccd7 | 1044.3 | 410.353 | 42.4535 | 6.51564 | 0.00569367 | 0.000873847 | 21.2201 | 1 | 1.21137 | 0.716774 | 344.018 | 3.99858 | 36.3988 | 4.74949 | -0.769152 | 0.231707 | F | F | 3.21e+20 | 5.01723e-14 | 1 | dsx |
Report | srcpi bgdpi arf | 2 | X153041.00+771241.7 | chandra | ccd3 | 536.588 | 338.647 | 28.575 | 7.1441 | 0.00383241 | 0.00095815 | 9.84469 | 1 | 5.05251 | 4.05435 | 159.837 | 12.1626 | 18.2335 | 11.021 | -0.246543 | 0.252233 | F | F | 3.2e+20 | 5.80146e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X152918.03+771635.1 | chandra | ccd3 | 1100.77 | 806.273 | 18.3377 | 5.8734 | 0.0024594 | 0.000787726 | 8.49263 | 1 | 3.45154 | 2.92396 | 141.081 | 10.0689 | 10.5654 | 7.91568 | -0.143376 | 0.322454 | F | F | 3.17e+20 | 3.40232e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X152724.98+772015.8 | chandra | ccd2 | 1037.32 | 635.912 | 18.2086 | 5.66369 | 0.00244204 | 0.000759584 | 10.8985 | 1 | 3.28611 | 1.96965 | 131.019 | 10.8478 | 12.188 | 7.27442 | -0.252464 | 0.307141 | A | F | 3.15e+20 | 3.6026e-14 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X152715.15+771122.5 | chandra | ccd7 | 939.625 | 1128 | 7.74592 | 3.95804 | 0.00103885 | 0.000530834 | 15.367 | 1 | 0.492 | 0.492 | 124.722 | 1.95122 | 4.83061 | 2 | -0.414401 | 0.6067 | F | F | 3.2e+20 | 7.90343e-15 | 1 | dx |
Report | srcpi bgdpi arf | 7 | X152714.92+770924.3 | chandra | ccd7 | 941.125 | 887.625 | 7.59671 | 3.95804 | 0.00101884 | 0.000530834 | 11.9624 | 1 | 0.619863 | 0.492 | 63.2644 | 0.297458 | 3.86557 | 3.86557 | 0 | 0.388041 | T | F | 3.2e+20 | 7.60669e-15 | 1 | dx |
Report | srcpi bgdpi arf | 8 | X152735.69+771325.2 | chandra | ccd7 | 801.214 | 1377.5 | 10.5983 | 4.42783 | 0.0014214 | 0.00059384 | 16.7229 | 1 | 0.622639 | 0.492 | 9.49833 | 4.22631 | 7.93306 | 1.86611 | -0.619128 | 0.518103 | F | F | 3.19e+20 | 1.32431e-14 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X152737.59+771121.7 | chandra | ccd7 | 787.928 | 1126.5 | 6.63688 | 3.78388 | 0.000890108 | 0.000507477 | 11.0139 | 1 | 0.574002 | 0.492 | 130.935 | 2.46369 | 3 | 3.92738 | 0.133871 | 0.557582 | F | F | 3.2e+20 | 6.82978e-15 | 1 | dx |
Report | srcpi bgdpi arf | 9 | X152839.97+770547.8 | chandra | ccd7 | 361.928 | 449.643 | 6.55108 | 3.78388 | 0.000878601 | 0.000507477 | 9.7775 | 1 | 0.889734 | 0.589644 | 152.143 | 6.2173 | 3 | 2.66331 | -0.0594512 | 0.644886 | A | F | 3.21e+20 | 7.10644e-15 | 1 | dx |
Report | srcpi bgdpi arf | 2 | X152544.25+770806.4 | chandra | ccd6 | 723.5 | 80 | 5.73135 | 3.59808 | 0.000768671 | 0.000482563 | 11.0577 | 1 | 0.620488 | 0.492 | 52.0181 | 4.93409 | 3.86568 | 1.93284 | -0.333333 | 0.662749 | F | F | 3.2e+20 | 1.60084e-14 | 1 | dx |
Report | srcpi bgdpi arf | 1 | X152640.74+771504.7 | chandra | ccd6 | 338.333 | 928.833 | 5.3429 | 3.59808 | 0.000716573 | 0.000482563 | 6.59117 | 0.999994 | 0.508303 | 0.492 | 94.4575 | 5.85313 | 2.50718 | 2.83573 | 0.0614925 | 0.683643 | F | F | 3.18e+20 | 8.66398e-15 | 1 | dx |
Report | srcpi bgdpi arf | 6 | X152753.43+770622.6 | chandra | ccd7 | 679 | 518.833 | 5.73986 | 3.59808 | 0.000769804 | 0.000482557 | 11.2538 | 1 | 0.641061 | 0.492 | 11.477 | 3.92235 | 3.93496 | 0.804895 | -0.660372 | 0.872128 | F | F | 3.21e+20 | 5.95474e-15 | 1 | dx |
Report | srcpi bgdpi arf | 3 | X152613.73+771158.5 | chandra | ccd6 | 521.5 | 550.75 | 3.83061 | 3.17945 | 0.00051375 | 0.000426418 | 9.30741 | 0.999999 | 0.492 | 0.492 | 90 | 3.99898 | 3 | 0.830613 | -0.566329 | 0.970859 | F | F | 3.19e+20 | 5.98943e-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