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 3 X092056.75+292332.4 chandra ccd3 793.48 148.96 104.12 11.1183 0.0108015 0.00115342 23.5811 1 3.05634 3.05634 0 9.33627 F F 1.67e+20 1.62222e-13 1 dsxf
Report srcpi bgdpi arf 1 X092143.40+293823.3 chandra ccd0 598.078 915.989 62.0917 8.30667 0.00643731 0.000861187 10.2844 1 1.45037 1.21641 139.708 8.69693 F F 1.67e+20 9.60169e-14 1 dx
Report srcpi bgdpi arf rmf 2 X092140.83+293809.5 chandra ccd0 666.631 888.436 528.213 24.9465 0.0547621 0.00258631 87.4893 1 2.68357 2.68357 0 8.22474 F F 1.67e+20 8.2328e-13 1 dsxf
Report srcpi bgdpi arf 1 X092051.15+292740.5 chandra ccd3 941.182 652.795 41.2264 6.63328 0.00427681 0.000688133 9.33697 1 2.12112 1.45149 93.4072 7.68966 F F 1.66e+20 6.23469e-14 1 dx
Report srcpi bgdpi arf 2 X092048.08+292717.5 chandra ccd3 1022.56 606.147 14.7176 4.12315 0.0015268 0.000427733 3.33325 0.999019 2.21387 1.24298 89.4048 8.45582 A F 1.66e+20 3.03349e-14 1 dx
Report srcpi bgdpi arf 1 X092202.02+292736.8 chandra ccd1 106.199 649.069 11.9949 5.27125 0.00124395 0.000546664 4.26878 0.999786 2.48932 1.12395 344.463 9.03515 F F 1.69e+20 1.77581e-14 1 dsx
Report srcpi bgdpi arf 3 X092144.14+292856.2 chandra ccd1 580.942 809.911 11.4973 3.39077 0.00119235 0.000351646 4.0917 0.999786 1.11692 0.445581 0.314925 4.93396 F F 1.67e+20 1.47005e-14 1 dsx
Report srcpi bgdpi arf 2 X092159.67+292728.5 chandra ccd1 168.167 631.583 9.52775 3.46415 0.000988095 0.000359256 3.39077 0.998615 2.31573 1.43298 152.079 8.61487 A F 1.69e+20 1.38229e-14 1 dx
Report srcpi bgdpi arf 7 X092102.97+292745.0 chandra ccd3 627.278 661.722 8.89929 3 0.000923208 0.000311219 2.01552 0.973931 0.526208 0.492 106.287 5.41096 F T 1.67e+20 1.21839e-14 1 dx
Report srcpi bgdpi arf 4 X092200.51+293202.2 chandra ccd0 143.976 142.457 12.8259 5.29735 0.00132972 0.000549199 2.12439 0.980995 1.5 0.4145 20.9446 8.19379 A F 1.68e+20 1.86466e-14 1 dsx
Report srcpi bgdpi arf 4 X092118.27+292327.4 chandra ccd3 221.278 137.944 8.40458 3.00001 0.000871887 0.00031122 1.90347 0.959232 1.27451 0.89045 39.0497 7.49338 F F 1.68e+20 1.19655e-14 1 dx
Report srcpi bgdpi arf 6 X092131.69+292810.2 chandra ccd1 910.928 715.643 6.87924 2.64575 0.000713426 0.000274383 2.44821 0.984442 0.581482 0.492 20.0505 3.26188 F F 1.67e+20 8.44226e-15 1 dx
Report srcpi bgdpi arf 3 X092101.40+293349.7 chandra ccd2 670.333 359 5.85991 2.44949 0.000607516 0.000253947 6.88377 0.999989 0.652664 0.492 74.2326 5.60431 F F 1.66e+20 8.49213e-15 1 dx
Report srcpi bgdpi arf 2 X092120.95+293809.1 chandra ccd2 152 886 5.48483 2.4495 0.00056863 0.000253948 6.44315 0.999989 0.492 0.492 45 7.29933 F F 1.66e+20 8.62711e-15 1 dx
Report srcpi bgdpi arf 7 X092144.73+293812.4 chandra ccd0 562.652 893.864 27.194 5.74462 0.00281931 0.000595569 4.50421 0.999977 3.25556 2.23366 168.673 8.69278 F T 1.67e+20 4.18219e-14 1 dx
Report srcpi bgdpi arf 9 X092134.64+293153.5 chandra ccd0 830.182 124.076 41.4425 6.43758 0.00429652 0.000667412 6.86423 1 0.545975 0.545975 0 2.67357 F F 1.67e+20 5.10643e-14 1 dsx
Report srcpi bgdpi arf 1 X092058.45+293132.4 chandra ccd2 748.833 79.8335 2.84988 1.73206 0.000295456 0.000179568 3.34782 0.993518 0.543766 0.492 55.278 5.44395 F F 1.66e+20 3.94803e-15 1 dx
Report 4 X092116.09+293148.3 chandra ccd2 281 112 1.94398 1.41422 0.000201539 0.000146616 2.28363 0.962791 0.492 0.492 45 1.82396 F F 1.66e+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