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 | 2 | X123052.64+143304.9 | chandra | ccd7 | 398.586 | 300.459 | 175.99 | 13.4285 | 0.0339451 | 0.0025901 | 119.444 | 1 | 0.423986 | 0.423986 | 0 | 0.479299 | F | F | 2.68e+20 | 0 | 1 | ds | |||||
| Report | 1 | X123049.70+143531.1 | chandra | ccd7 | 485.229 | 597.53 | 37.2163 | 6.10113 | 0.00717829 | 0.00117679 | 25.2586 | 1 | 0.67565 | 0.398029 | 331.888 | 2.67211 | F | F | 2.68e+20 | 0 | 1 | ds | |||||
| Report | 1 | X123047.46+142448.6 | chandra | ccd6 | 270.8 | 307.2 | 9.29197 | 3.16229 | 0.00179223 | 0.00060994 | 14.5406 | 1 | 1.38137 | 0.548052 | 54.3863 | 8.09308 | A | F | 2.65e+20 | 0 | 1 | d | |||||
| Report | 9 | X123056.24+143220.5 | chandra | ccd7 | 291.722 | 209.722 | 8.82648 | 3 | 0.00170244 | 0.000578638 | 5.99051 | 0.999982 | 0.550175 | 0.492 | 79.972 | 1.39776 | F | F | 2.68e+20 | 0 | 1 | d | |||||
| Report | 1 | X123025.30+143932.6 | chandra | ccd3 | 122.3 | 368.1 | 8.82068 | 3.1623 | 0.00170133 | 0.000609942 | 14.5325 | 1 | 2.04205 | 1.62422 | 46.2227 | 9.10664 | F | F | 2.68e+20 | 0 | 1 | d | |||||
| Report | 5 | X123039.55+143009.8 | chandra | ccd6 | 504.214 | 960.072 | 6.90001 | 2.64575 | 0.00133087 | 0.000510311 | 10.7976 | 1 | 0.492 | 0.492 | 32.9272 | 3.84521 | F | F | 2.68e+20 | 0 | 1 | d | |||||
| Report | 4 | X123048.83+143545.4 | chandra | ccd7 | 510.5 | 626.167 | 5.86877 | 2.44949 | 0.00113196 | 0.000472456 | 3.98312 | 0.999573 | 0.518385 | 0.492 | 37.5343 | 2.93815 | F | F | 2.68e+20 | 0 | 1 | d | |||||
| Report | 3 | X123051.09+143423.5 | chandra | ccd7 | 443.7 | 459.7 | 4.86021 | 2.23607 | 0.000937434 | 0.000431292 | 3.29861 | 0.998177 | 0.492 | 0.492 | 45 | 1.53181 | F | F | 2.68e+20 | 0 | 1 | d | |||||
| Report | 5 | X123047.95+143116.3 | chandra | ccd7 | 536.5 | 79.3 | 4.85279 | 2.23608 | 0.000936002 | 0.000431292 | 3.29357 | 0.998177 | 0.689787 | 0.492 | 114.006 | 1.73952 | T | F | 2.68e+20 | 0 | 1 | d | |||||
| Report | 3 | X123054.01+142951.6 | chandra | ccd6 | 77.5 | 923 | 3.91374 | 2 | 0.000754879 | 0.000385759 | 6.12445 | 0.999933 | 0.658025 | 0.492 | 53.3496 | 3.09557 | F | F | 2.67e+20 | 0 | 1 | d | |||||
| Report | 6 | X123049.80+143604.7 | chandra | ccd7 | 481.75 | 665.5 | 3.85437 | 2 | 0.000743429 | 0.000385759 | 2.61595 | 0.993033 | 0.58344 | 0.492 | 90 | 3.22901 | F | F | 2.68e+20 | 0 | 1 | d | |||||
| Report | 4 | X123047.36+142527.1 | chandra | ccd6 | 273.75 | 385.5 | 3.81195 | 2.00001 | 0.000735246 | 0.00038576 | 5.96516 | 0.999933 | 1.08272 | 0.492 | 137.619 | 7.45739 | A | F | 2.65e+20 | 0 | 1 | d | |||||
| Report | 7 | X123057.10+143609.5 | chandra | ccd7 | 266.5 | 675.25 | 3.77373 | 2.00001 | 0.000727874 | 0.00038576 | 2.56122 | 0.976448 | 0.538384 | 0.492 | 14.4433 | 3.62545 | F | F | 2.68e+20 | 0 | 1 | d | |||||
| Report | 2 | X123041.22+142920.5 | chandra | ccd6 | 455 | 860 | 1.95775 | 1.41422 | 0.000377609 | 0.000272773 | 3.0636 | 0.991618 | 0.492 | 0.492 | 45 | 4.22333 | F | F | 2.67e+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