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 X211817.41+001317.0 chandra ccd6 1268.72 842.018 103.239 10.1607 0.0182549 0.00179662 159.112 1 1.64631 0.980497 52.3979 4.48876 F F 5.82e+20 2.21037e-13 1 dsxf
Report srcpi bgdpi arf 1 X211841.23+000657.1 chandra ccd5 1018.06 957.407 75.8205 10.3925 0.0134066 0.0018376 64.4694 1 5.30479 3.21705 140.829 11.1496 A F 5.6e+20 1.31378e-13 1 dx
Report srcpi bgdpi arf 2 X211816.97+001718.5 chandra ccd7 769.181 417.991 53.6225 7.54711 0.00948159 0.00133449 53.3341 1 0.563855 0.391373 0 2.03133 F F 5.85e+20 7.12566e-14 1 dsx
Report srcpi bgdpi arf 1 X211752.07+000647.8 chandra ccd2 710.485 519.011 21.4168 6.49031 0.00378694 0.00114762 4.70644 0.999988 9.01957 4.44655 38.4069 13.3927 F F 5.88e+20 5.46293e-14 1 dsx
Report srcpi bgdpi arf 1 X211828.56+002036.9 chandra ccd7 415.848 821.254 14.692 3.83301 0.00259786 0.000677758 14.613 1 0.646034 0.646034 0 3.38228 F F 5.79e+20 2.0357e-14 1 dsx
Report srcpi bgdpi arf 5 X211814.88+001543.4 chandra ccd7 833.024 224.61 14.0741 3.75155 0.00248859 0.000663352 13.9984 1 0.896502 0.437929 58.414 3.02763 F F 5.85e+20 1.98647e-14 1 dsx
Report 4 X211830.41+001802.1 chandra ccd7 358.9 506.1 9.76143 3.16228 0.00172602 0.000559155 9.70892 1 0.658655 0.492 75.3756 1.49747 T F 5.78e+20 0 1 d
Report srcpi bgdpi arf 2 X211746.53+001408.9 chandra ccd3 424.75 483.083 9.34109 3.46415 0.00165263 0.000612878 15.1333 1 3.83033 1.76375 142.781 10.1575 A F 6.04e+20 2.23181e-14 1 dx
Report srcpi bgdpi arf 1 X211752.86+001703.3 chandra ccd3 231.833 837.5 5.58734 2.4495 0.000988513 0.000433366 9.05194 0.999997 1.16309 0.492 176.028 8.06449 A F 6.01e+20 1.36129e-14 1 dx
Report srcpi bgdpi arf 3 X211824.07+001729.4 chandra ccd7 552.3 439.5 4.86956 2.23607 0.000861036 0.000395382 4.84337 0.999372 0.492 0.492 160.097 0.294051 F F 5.8e+20 6.43084e-15 1 dx
Report srcpi bgdpi arf 6 X211818.06+001519.7 chandra ccd7 735.5 175.9 4.86614 2.23607 0.000860431 0.000395382 4.83997 0.999372 0.492 0.492 115.67 2.67696 F F 5.83e+20 6.85075e-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