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 | 3 | X213032.87+050217.4 | chandra | ccd7 | 153.288 | 296.553 | 95.1716 | 9.75559 | 0.0166632 | 0.00170806 | 53.7747 | 1 | 0.495803 | 0.343145 | 95.5459 | 0.584359 | F | F | 4.97e+20 | 1.10734e-13 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X213030.94+050621.2 | chandra | ccd7 | 212.005 | 792.021 | 16.9787 | 4.88702 | 0.00297272 | 0.000855644 | 9.59345 | 1 | 1.3565 | 0.443677 | 337.821 | 4.66247 | F | F | 4.98e+20 | 2.0981e-14 | 1 | dsx | ||||
| Report | srcpi bgdpi arf | 1 | X212955.47+050509.6 | chandra | ccd3 | 244.591 | 223.136 | 8.26956 | 3.31668 | 0.00144788 | 0.000580701 | 11.4813 | 1 | 3.27533 | 1.26262 | 74.2869 | 9.89313 | A | F | 5.07e+20 | 1.85741e-14 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 2 | X213031.64+050639.3 | chandra | ccd7 | 190.214 | 828.214 | 6.1159 | 2.64577 | 0.0010708 | 0.000463235 | 3.45566 | 0.99849 | 0.594358 | 0.492 | 53.6408 | 4.95341 | F | F | 4.98e+20 | 7.60406e-15 | 1 | dx | ||||
| Report | srcpi bgdpi arf | 4 | X213030.78+050109.8 | chandra | ccd7 | 216.3 | 158.5 | 4.47386 | 2.23608 | 0.000783307 | 0.000391505 | 2.52786 | 0.984978 | 0.492 | 0.492 | 180 | 0.725184 | F | F | 4.98e+20 | 5.23607e-15 | 1 | dx | ||||
| Report | 1 | X213034.97+045813.1 | chandra | ccd6 | 173 | 846.5 | 3.86847 | 2 | 0.000677311 | 0.000350171 | 4.79147 | 0.999428 | 0.492 | 0.492 | 121.717 | 3.53468 | F | F | 4.97e+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