SIMPLE = T / BITPIX = 16 / NAXIS = 2 / NAXIS1 = 796 / NAXIS2 = 520 / BSCALE = 1.0 / BZERO = 0 / JD = 2453139.74559 / Julian Date at beginning of exposure DATE-OBS= 5.13 / MM.DD Local date at previous sunset LMST = 15.30 / HH.MM mean LST at beginning of exposure EXPOSURE= 120.00 / Time in seconds, excluding readout CCD_TEMP= -10.00 / Temperature of CCD OBJECT = meridian / approximately OBSERVER= P.R.McCullough_et_al / SIZE = 5.0x8.0 / Size of image in degrees LATITUDE= 40.11023 / Latitude of the Observing Site LONGITUD= 88.22070 / Longitude (both in degrees) INSTRUME= KAF0400 / Nikon 50mm f 1.4 at 2.0 TELESCOP= Stardial / This is copyrighted material. EMAIL = pmcc@astro.uiuc.edu / If you use it, please email us... URL = www.astro.uiuc.edu / ...so we may justify continuing it. CTYPE1 = 'RA---TAN' / CTYPE2 = 'DEC--TAN' / CRVAL1 = 234.0000 / CRVAL2 = -4.5000 / CRPIX1 = 389.3500 / CRPIX2 = 306.9782 / CD1_1 = -0.000054468132 / CD1_2 = 0.009966718033 / CD2_1 = 0.009972654283 / CD2_2 = 0.000052702420 / CDELT1 = 0.0099698 / CDELT2 = -0.0099698 / CROTA1 = 90.3129272 / CROTA2 = 90.3129272 / N_ASTROM= 31 / No. of astrometry stars EQUINOX = 2000 / BKG0 = 10327.88 / Average value before background subtraction COMMENT / Background = BKG1 + BKG2*P1(X) + BKG3*P1(Y) + COMMENT / BKG4*P2(X) +BKG5*P3(X) +BKG6*P4(X) +BKG7*P5(X) COMMENT / X(i) = (i-0.5*NAXIS1)/(0.5*NAXIS1) COMMENT / Y(j) = (j-0.5*NAXIS2)/(0.5*NAXIS2) COMMENT / Pn(v) = Legendre Polynomial of degree n of v BKG1 = 10325.69 / BKG2 = -244.23 / BKG3 = -327.95 / BKG4 = -199.40 / BKG5 = 68.85 / BKG6 = -220.73 / BKG7 = -1.01 / END ݙ mܯmȈ9+vq]OSwuTVZfTDD@e+UwKT]ݛk(I@JO9nUN7UUNT*ffgr**jmUUUUUUUU%U3U3U3U>̪;5;V;UBfffffffffffffffefg3ڙ3("&35Bfb"""fHS0`3l~UT5JU:LW*Nd5,H"])3UWw4)˧BL̀S23>+UkRԓR* W/)TEKD5RCU-TA 4MMMKI̙d9rdL*eS ̷3320"""""&R3323"dӲd ii&i 3S@i `ʑ*fDșR%Ha3332J"RS.h 4&f07JiM 56ۚ BhK JT cUtUT+PuctzAPdQcU'XOӠ:-MKRnhM1? Ȣ$˦%ˢyI*ߧs=U;ĤH,̴*fffffJFg^ T^'G RTGtR*[6)www*"*wUN:jhREI%I RZj*HiNnd9-ɔ&Hjf\ɒBfTLə2fDs2U*e932̷3(33.f\*f@uNfBHL̳3"QudU.d6ݺ'4]2lA2LS4 .h4)4i2)52X,9IeT%RC(eLNRHe,ʕ2)P)eSR2:rʩʩ2FUHM,YT,ʬyTʠ2*<ݻ`6Q؈*LeS* TRk*M]ݫ D@T@RTĂ=e* Ԡ