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 | arf | 1 | X043939.48+071656.5 | chandra | ccd1 | 193.021 | 992.932 | 11.1853 | 3.43438 | 0.00701053 | 0.00215254 | 14.3254 | 1 | 1.52051 | 1.52051 | 0 | 7.1809 | F | F | 9.02e+20 | 7.46681e-14 | 1 | dsx | ||||
Report | arf | 4 | X043908.73+071645.3 | chandra | ccd3 | 101.389 | 849.389 | 8.93877 | 3 | 0.00560236 | 0.00188025 | 14.0978 | 1 | 0.492 | 0.492 | 58.9486 | 1.05827 | F | F | 9.15e+20 | 5.42346e-14 | 1 | dx | ||||
Report | arf | 1 | X043906.89+071701.2 | chandra | ccd3 | 157.125 | 881.75 | 7.91564 | 2.82843 | 0.00496111 | 0.00177271 | 12.4842 | 1 | 0.492 | 0.492 | 174.056 | 1.1573 | F | F | 9.16e+20 | 4.82178e-14 | 1 | dx | ||||
Report | 2 | X043907.30+072122.3 | chandra | ccd2 | 240.5 | 403.5 | 5.95603 | 2.44949 | 0.00373293 | 0.00153521 | 15.4877 | 1 | 0.499628 | 0.492 | 18.4349 | 3.76887 | F | F | 9.22e+20 | 0 | 1 | d | |||||
Report | 1 | X043916.56+071845.7 | chandra | ccd0 | 992.5 | 190.25 | 3.97184 | 2 | 0.00248934 | 0.0012535 | 10.7684 | 1 | 0.492 | 0.492 | 90 | 1.80818 | F | F | 9.15e+20 | 0 | 1 | d | |||||
Report | 2 | X043916.00+071518.9 | chandra | ccd1 | 902.5 | 793.833 | 2.98585 | 1.73205 | 0.00187138 | 0.00108556 | 3.82409 | 0.996448 | 0.492 | 0.492 | 90 | 2.72391 | F | F | 9.1e+20 | 0 | 1 | d | |||||
Report | arf | 3 | X043900.49+071601.5 | chandra | ccd3 | 350.5 | 760.5 | 2.7709 | 2.00004 | 0.00173666 | 0.00125352 | 4.37014 | 0.999209 | 0.492 | 0.492 | 45 | 3.0274 | F | F | 9.18e+20 | 1.7241e-14 | 1 | dx | ||||
Report | 1 | X043906.41+071858.4 | chandra | ccd2 | 267.5 | 111 | 1.98405 | 1.41421 | 0.0012435 | 0.000886356 | 5.1592 | 0.999517 | 0.492 | 0.492 | 90 | 1.65715 | F | F | 9.2e+20 | 0 | 1 | d | |||||
Report | 2 | X043849.27+071532.5 | chandra | ccd3 | 690 | 701.5 | 1.97135 | 1.41421 | 0.00123554 | 0.000886357 | 3.10912 | 0.991965 | 0.492 | 0.492 | 116.565 | 5.72899 | F | F | 9.22e+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