Source List

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 1 X093155.61+370548.5 chandra ccd6 696.085 867.227 227.115 15.2115 0.0415873 0.0027854 109.832 1 4.63712 3.25877 63.0934 8.09591 F F 1.17e+20 5.379e-13 1 dsxf
Report srcpi bgdpi arf 1 X093207.47+365745.8 chandra ccd7 705.571 917.091 73.9152 8.96162 0.0135347 0.00164097 41.3349 1 0.392672 0.392672 0 0.293085 F F 1.17e+20 9.99007e-14 1 dsx
Report srcpi bgdpi arf 1 X093248.00+370049.4 chandra ccd2 773.403 67.7583 26.934 5.56782 0.00493188 0.00101952 40.4544 1 3.31064 2.0225 177.645 8.79509 A F 1.18e+20 6.90187e-14 1 dx
Report srcpi bgdpi arf 8 X093202.71+365558.6 chandra ccd7 821.45 699.357 27.6276 5.2562 0.00505891 0.000962466 15.4499 1 0.569894 0.272592 116.043 2.10594 F F 1.17e+20 3.78476e-14 1 dsx
Report srcpi bgdpi arf 3 X093155.90+365116.2 chandra ccd7 987.237 124.868 17.7754 4.35892 0.00325485 0.000798161 9.94034 1 1.10603 0.715342 67.7147 7.00409 A F 1.16e+20 3.23837e-14 1 dx
Report srcpi bgdpi arf 3 X093249.25+365509.0 chandra ccd3 1034.68 366.864 12.8347 3.87302 0.00235016 0.000709189 19.0173 1 2.24838 0.492 45.5016 9.01651 A F 1.21e+20 3.39823e-14 1 dx
Report srcpi bgdpi arf 2 X093310.83+365817.0 chandra ccd3 509.605 750.237 12.1363 4.35899 0.00222227 0.000798175 17.9825 1 4.15542 3.03336 54.5928 12.8819 F F 1.21e+20 3.41259e-14 1 dx
Report srcpi bgdpi arf 2 X093214.04+365856.3 chandra ccd7 545.125 1060 7.70913 2.82843 0.00141162 0.000517914 4.3111 0.999506 0.492 0.492 16.2062 1.82111 F F 1.17e+20 1.05827e-14 1 dx
Report srcpi bgdpi arf 1 X093309.72+365803.9 chandra ccd3 536.731 723.577 7.67411 3.60564 0.00140521 0.000660228 11.3708 1 4.87199 2.41971 111.002 12.6555 A F 1.21e+20 2.03375e-14 1 dx
Report srcpi bgdpi arf 4 X093201.01+365422.8 chandra ccd7 862.5 504.072 6.75107 2.64576 0.00123619 0.000484464 3.77533 0.998247 0.591488 0.492 38.5625 3.73135 F F 1.16e+20 9.5425e-15 1 dx
Report srcpi bgdpi arf 7 X093157.25+365626.4 chandra ccd7 954 755.333 5.82341 2.44949 0.00106632 0.000448527 3.25657 0.998247 0.492 0.492 57.7317 2.36788 F F 1.17e+20 8.12575e-15 1 dx
Report srcpi bgdpi arf 5 X093221.02+365609.3 chandra ccd7 374.7 720.7 4.80794 2.23607 0.000880382 0.000409447 2.6887 0.994312 0.492 0.492 164.518 3.43771 F F 1.17e+20 7.5998e-15 1 dx
Report srcpi bgdpi arf 6 X093229.62+365418.4 chandra ccd7 164.9 495.3 4.61479 2.23608 0.000845014 0.000409448 2.58068 0.983235 0.69027 0.492 40.3945 5.90947 F F 1.17e+20 7.28395e-15 1 dx
Report 5 X093152.81+370027.3 chandra ccd6 764 214 3.91558 2 0.000716982 0.00036622 1.89357 0.969238 0.492 0.492 45 3.68476 F F 1.17e+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