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 rmf | 1 | X094133.72+594811.1 | chandra | ccd7 | 208.473 | 995.084 | 109.9 | 10.5822 | 0.110082 | 0.0105997 | 65.9753 | 1 | 1.00847 | 0.615445 | 357.571 | 2.84259 | T | F | 2.06e+20 | 6.0907e-13 | 1 | dsxf | ||||
Report | srcpi bgdpi arf | 5 | X094055.56+594436.4 | chandra | ccd7 | 794.184 | 558.634 | 9.67121 | 4.04993 | 0.0096872 | 0.00405662 | 5.80583 | 0.999993 | 0.725851 | 0.725851 | 0 | 3.8303 | F | F | 2.04e+20 | 6.21386e-14 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 2 | X094202.95+593711.5 | chandra | ccd3 | 864.91 | 434.462 | 62.5232 | 10.053 | 0.0150375 | 0.00241785 | 10.0713 | 1 | 5.83945 | 5.83945 | 0 | 12.5296 | F | F | 1.95e+20 | 2.04413e-13 | 1 | dsx | ||||
Report | srcpi bgdpi arf | 1 | X094214.41+594449.2 | chandra | ccd2 | 1168.39 | 437.889 | 31.5135 | 6.00005 | 0.0075817 | 0.00144352 | 37.9725 | 1 | 2.47076 | 2.01555 | 74.3129 | 8.52681 | F | F | 2e+20 | 9.21483e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 2 | X094254.03+595034.4 | chandra | ccd2 | 564.357 | 1142.71 | 11.0114 | 3.74172 | 0.00264918 | 0.000900203 | 13.2683 | 1 | 3.27786 | 2.26468 | 157.157 | 13.1955 | F | F | 1.98e+20 | 3.74902e-14 | 1 | dx | ||||
Report | srcpi bgdpi arf | 4 | X094051.96+594510.0 | chandra | ccd7 | 848.808 | 626.5 | 10.0858 | 3.6056 | 0.00242572 | 0.000867173 | 6.05475 | 0.999993 | 0.692783 | 0.492 | 60.8038 | 3.64931 | F | F | 2.05e+20 | 1.55544e-14 | 1 | dbx |
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