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 X112319.79+041010.9 chandra ccd1 426.365 525.489 114.574 10.96 0.0172736 0.00165237 48.6432 1 1.47666 0.880694 346.267 5.55491 F F 3.85e+20 2.03963e-13 1 dsxf
Report srcpi bgdpi arf 7 X112258.32+041423.7 chandra ccd2 361.206 147.313 9.51054 3.352 0.00143384 0.000505357 8.85471 1 0.270393 0.270393 0 1.43547 F F 3.88e+20 1.69233e-14 1 dsx
Report srcpi bgdpi arf 1 X112258.42+041754.8 chandra ccd2 358.002 576.468 12.0388 3.55256 0.001815 0.000535592 11.2086 1 1.47901 0.307986 236.805 4.84497 A F 3.9e+20 2.19719e-14 1 dsx
Report srcpi bgdpi arf 3 X112247.50+041708.9 chandra ccd2 689.7 482.7 9.81557 3.16228 0.00147982 0.000476752 9.13871 1 0.874705 0.492 131.347 5.23987 A F 3.91e+20 1.88217e-14 1 dx
Report srcpi bgdpi arf 2 X112313.08+041117.0 chandra ccd1 629.833 659.278 8.87436 3 0.00133792 0.000452287 3.76767 0.999347 0.694126 0.492 21.7 3.5523 F F 3.86e+20 1.57281e-14 1 dx
Report srcpi bgdpi arf 5 X112300.88+041746.0 chandra ccd2 282.722 558.056 8.74703 3.00001 0.00131872 0.000452287 8.14386 1 0.994707 0.492 98.2641 4.66627 A F 3.9e+20 1.99e-14 1 dx
Report srcpi bgdpi arf 2 X112252.49+041656.6 chandra ccd2 537.75 457.5 7.78378 2.82843 0.0011735 0.00042642 7.24703 0.999996 1.00926 0.492 132.527 4.369 A F 3.9e+20 1.54242e-14 1 dx
Report srcpi bgdpi arf 1 X112331.33+041029.1 chandra ccd0 297 65.125 7.37578 2.82844 0.00111199 0.000426422 12.2581 1 1.17914 0.867206 40.3002 8.03855 F F 3.85e+20 1.4553e-14 1 dx
Report srcpi bgdpi arf 2 X112313.55+041208.9 chandra ccd0 837.5 267.928 6.9354 2.64575 0.0010456 0.000398879 11.5262 1 0.639792 0.492 14.6244 3.30913 F F 3.86e+20 1.43339e-14 1 dx
Report 1 X112244.28+041414.7 chandra ccd3 571.5 605.643 6.91717 2.64575 0.00104285 0.000398879 10.9164 1 0.825414 0.492 110.755 4.28455 A F 3.89e+20 0 1 d
Report srcpi bgdpi arf 2 X112238.87+041320.6 chandra ccd3 736 495.667 5.85726 2.44949 0.000883052 0.000369291 9.24369 1 0.534027 0.492 63.652 5.483 F F 3.89e+20 1.10835e-14 1 dx
Report srcpi bgdpi arf 3 X112319.58+041355.2 chandra ccd0 654.3 483.9 4.8803 2.23607 0.000735764 0.000337115 8.11073 0.999998 0.690961 0.492 51.2644 4.74282 F F 3.87e+20 8.89751e-15 1 dx
Report 4 X112311.70+041255.5 chandra ccd0 893.7 362.5 4.93251 2.23607 0.000743636 0.000337114 8.19751 0.999998 0.492 0.492 34.0993 2.71419 F F 3.86e+20 0 1 d
Report srcpi bgdpi arf 4 X112235.20+041725.9 chandra ccd2 1063.5 517.1 4.72586 2.23608 0.000712481 0.000337116 4.39998 0.998769 0.845015 0.492 34.6523 7.72068 A F 3.92e+20 9.81168e-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