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 | 3 | X110216.46+022611.2 | chandra | ccd6 | 376.375 | 1006.5 | 7.95078 | 2.82843 | 0.00522092 | 0.0018573 | 23.5145 | 1 | 0.595344 | 0.492 | 158.7 | 2.48524 | F | F | 3.92e+20 | 0 | 1 | d | |||||
Report | 1 | X110141.35+023710.6 | chandra | ccd3 | 724.625 | 705.875 | 7.78396 | 2.82843 | 0.00511138 | 0.0018573 | 22.6502 | 1 | 2.33657 | 2.01257 | 150.645 | 12.7493 | F | T | 3.91e+20 | 0 | 1 | d | |||||
Report | 2 | X110157.40+023435.1 | chandra | ccd3 | 236 | 389.75 | 3.968 | 2 | 0.00260561 | 0.00131331 | 11.5463 | 1 | 0.758283 | 0.492 | 95.3922 | 8.08047 | A | F | 3.92e+20 | 0 | 1 | d | |||||
Report | 2 | X110206.51+022117.0 | chandra | ccd6 | 679.5 | 408.5 | 3.68902 | 2.00001 | 0.00242241 | 0.00131332 | 10.9103 | 0.999994 | 0.959428 | 0.492 | 132.618 | 7.94722 | A | F | 3.86e+20 | 0 | 1 | d | |||||
Report | 1 | X110201.69+022740.9 | chandra | ccd6 | 826.167 | 1188.83 | 2.98351 | 1.73205 | 0.00195914 | 0.00113736 | 8.82378 | 0.999994 | 0.492 | 0.492 | 109.903 | 4.4322 | F | T | 3.9e+20 | 0 | 1 | d | |||||
Report | 1 | X110210.57+023152.5 | chandra | ccd7 | 1024.83 | 764.167 | 2.93862 | 1.73205 | 0.00192966 | 0.00113736 | 5.69804 | 0.999831 | 0.492 | 0.492 | 106.845 | 3.91484 | F | T | 3.93e+20 | 0 | 1 | d | |||||
Report | 1 | X110150.65+023037.4 | chandra | ccd2 | 21.5 | 859.5 | 0.974875 | 1 | 0.000640157 | 0.000656657 | 3.06537 | 0.995217 | 0.492 | 0.492 | 90 | 7.38384 | F | T | 3.9e+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