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 4 X120130.37+011138.7 chandra ccd7 923.786 388.844 176.643 13.3394 0.113432 0.00856596 219.278 1 2.16015 1.22242 111.461 5.80535 118.76 43.7125 -0.46191 0.093603 F F 1.8e+20 9.79793e-13 1 dsxf
Report srcpi bgdpi arf 1 X120155.81+011334.7 chandra ccd7 148.336 624.706 12.4196 3.52415 0.00797525 0.00226303 15.4172 1 1.13857 0.356938 140.325 4.04011 4.9469 3.97345 -0.109127 0.469375 F F 1.78e+20 7.22166e-14 1 dsx
Report 2 X120134.52+011339.9 chandra ccd7 796.75 634.75 3.9931 2 0.00256415 0.00128429 4.95688 0.999439 0.492 0.492 45 3.578 F F 1.78e+20 0 1 d
Report srcpi bgdpi arf 1 X120150.09+011855.7 chandra ccd6 827.25 328.5 3.91531 3.17945 0.00251419 0.00204166 13.4537 1 0.492 0.492 129.116 2.99803 2 1.91531 -0.0216313 0.82671 F F 1.74e+20 2.75965e-14 1 dx
Report 3 X120123.50+011304.7 chandra ccd7 1132.83 563.167 2.90229 1.73205 0.00186369 0.00111223 3.60278 0.995577 0.492 0.492 109.903 6.08094 F F 1.79e+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