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 | 1 | X185643.61+021921.5 | chandra | ccd7 | 527.079 | 791.196 | 66.9377 | 8.62266 | 0.0118492 | 0.00152637 | 34.7696 | 1 | 0.403076 | 0.403076 | 0 | 1.21447 | F | F | 1.44e+22 | 1.59629e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X185658.08+022742.1 | chandra | ccd6 | 339.717 | 787.109 | 29.3775 | 5.65688 | 0.00520035 | 0.00100137 | 39.595 | 1 | 1.21495 | 0.897451 | 165.163 | 8.09431 | F | F | 1.46e+22 | 9.44777e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 3 | X185648.01+021836.6 | chandra | ccd7 | 392.802 | 699.919 | 9.85337 | 3.13901 | 0.00174422 | 0.000555661 | 5.11816 | 0.999966 | 0.668509 | 0.429754 | 0 | 2.33785 | F | F | 1.44e+22 | 2.36e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X185737.66+022044.4 | chandra | ccd2 | 405.875 | 476.25 | 6.28806 | 2.82847 | 0.0011131 | 0.000500689 | 8.94081 | 0.999999 | 2.91008 | 1.45167 | 89.2717 | 13.6962 | A | F | 1.39e+22 | 2.49492e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X185652.87+021856.7 | chandra | ccd7 | 244.5 | 740.333 | 5.63358 | 2.4495 | 0.000997245 | 0.000433605 | 2.92627 | 0.995096 | 0.801366 | 0.492 | 61.3435 | 2.9793 | A | F | 1.44e+22 | 1.36344e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X185723.82+021844.1 | chandra | ccd2 | 827.5 | 231.667 | 5.03807 | 2.44952 | 0.000891828 | 0.000433608 | 7.16348 | 0.999987 | 1.36414 | 0.492 | 2.36264e-08 | 10.3988 | A | F | 1.4e+22 | 1.76257e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 5 | X185646.66+021832.1 | chandra | ccd7 | 433.5 | 690.3 | 4.84103 | 2.23607 | 0.000856949 | 0.000395825 | 2.51459 | 0.986161 | 0.492 | 0.492 | 3.73992e-08 | 2.23716 | F | F | 1.44e+22 | 1.16397e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X185643.98+022035.8 | chandra | ccd7 | 515.1 | 941.7 | 4.8255 | 2.23607 | 0.000854199 | 0.000395825 | 2.50652 | 0.986161 | 0.492 | 0.492 | 138.563 | 0.288763 | F | F | 1.45e+22 | 1.15961e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 6 | X185644.42+021652.7 | chandra | ccd7 | 501.75 | 488.25 | 3.77011 | 2.00001 | 0.000667376 | 0.000354037 | 1.95832 | 0.964465 | 0.492 | 0.492 | 161.565 | 3.70096 | F | F | 1.44e+22 | 9.34206e-15 | 1 | dx | ||||
Report | 2 | X185637.55+022641.4 | chandra | ccd6 | 965.167 | 663.833 | 2.80371 | 1.73206 | 0.000496307 | 0.000306605 | 3.77884 | 0.997526 | 0.492 | 0.492 | 90 | 6.27302 | F | F | 1.47e+22 | 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