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 | 1 | X191201.15+170201.3 | chandra | ccd7 | 286.5 | 893.167 | 2.95467 | 1.73205 | 0.00203299 | 0.00119176 | 6.05816 | 0.99989 | 0.54799 | 0.492 | 123.019 | 3.61812 | F | F | 5.96e+21 | 0 | 1 | d | |||||
| Report | 3 | X191144.65+165842.2 | chandra | ccd7 | 767.5 | 488.5 | 2.94721 | 1.73205 | 0.00202786 | 0.00119176 | 6.04287 | 0.99989 | 0.587531 | 0.492 | 151.845 | 2.65341 | F | F | 5.92e+21 | 0 | 1 | d | |||||
| Report | 1 | X191104.57+165636.5 | chandra | ccd3 | 833.5 | 1008.83 | 2.84628 | 1.73206 | 0.00195841 | 0.00119176 | 10.8743 | 0.999949 | 3.34797 | 1.08011 | 143.317 | 12.4052 | A | F | 5.62e+21 | 0 | 1 | d | |||||
| Report | 1 | X191211.61+165237.9 | chandra | ccd6 | 730.167 | 511.167 | 2.81526 | 1.73206 | 0.00193707 | 0.00119176 | 10.1959 | 0.99993 | 0.721646 | 0.492 | 16.845 | 7.10737 | F | F | 6.17e+21 | 0 | 1 | d | |||||
| Report | 2 | X191125.64+165502.1 | chandra | ccd3 | 219 | 816.5 | 1.98497 | 1.41421 | 0.00136578 | 0.000973065 | 7.58363 | 0.999949 | 0.492 | 0.492 | 180 | 8.05123 | F | F | 5.79e+21 | 0 | 1 | d | |||||
| Report | 2 | X191203.20+170002.4 | chandra | ccd7 | 226.5 | 651.5 | 0.974147 | 1 | 0.000670272 | 0.000688062 | 1.99736 | 0.97582 | 0.492 | 0.492 | 90 | 2.26618 | F | F | 5.97e+21 | 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