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 X210211.51-064644.6 chandra ccd7 372.101 832.214 126.828 11.4415 0.0336145 0.00303247 88.7924 1 0.419397 0.419397 0 0.294928 F F 5.19e+20 2.55754e-13 1 dsxf
Report srcpi bgdpi arf 4 X210205.35-064755.9 chandra ccd7 558.74 687.284 94.7855 9.73578 0.025122 0.00258038 66.3594 1 0.737474 0.417462 324.918 1.94611 T F 5.16e+20 1.87763e-13 1 dsx
Report srcpi bgdpi arf 2 X210208.55-064502.1 chandra ccd7 461.5 1040.1 9.82601 3.16228 0.00260429 0.000838131 6.8792 0.999998 0.492 0.492 60.4819 1.58197 F F 5.15e+20 3.79474e-14 1 dx
Report srcpi bgdpi arf 2 X210208.04-063904.7 chandra ccd6 312.268 722.991 8.69549 4.85176 0.00230466 0.00128591 2.25692 0.982521 1.35317 1.35317 0 7.46564 F F 5.07e+20 2.64824e-14 1 dsx
Report srcpi bgdpi arf 3 X210207.04-064245.7 chandra ccd6 342.136 273.227 16.8271 4.12311 0.00445985 0.00109279 4.36749 0.999925 0.492 0.492 42.2798 3.86834 F F 5.11e+20 4.9041e-14 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