SIMPLE = T / file does conform to FITS standard BITPIX = 8 / number of bits per data pixel NAXIS = 0 / number of data axes EXTEND = T / FITS dataset may contain extensions COMMENT FITS (Flexible Image Transport System) format is defined in 'AstronomyCOMMENT and Astrophysics', volume 376, page 359; bibcode: 2001A&A...376..359H SRCFN = '/tmp/tmp.fits.ADvpp2' / Source image SRCEXT = 1 / Source image extension (1=primary) COMMENT Parameters used for source extraction HISTORY Created by Astrometry.net's image2xy program. HISTORY SVN URL: svn+ssh://astrometry.net/svn/tags/tarball-0.38/astrometry/util/HISTORY SVN Rev: 16745 HISTORY SVN Date: 2010-11-19 20:47:53 +0000 (Fri, 19 Nov 2010) HISTORY Visit us on the web at http://astrometry.net/ NEXTEND = 1 / Number of extensions LONGSTRN= 'OGIP 1.0' / The OGIP long string convention may be used COMMENT This FITS file may contain long string keyword values that are COMMENT continued over multiple keywords. This convention uses the '&' COMMENT character at the end of the string which is then continued COMMENT on subsequent keywords whose name = 'CONTINUE'. IMAGEW = 4256 / image width IMAGEH = 2832 / image height ANRUN = T / Solve this field! ANVERUNI= T / Uniformize field during verification ANVERDUP= F / Deduplicate field during verification ANAPPL1 = 0.5 / scale: arcsec/pixel min ANAPPU1 = 0.6 / scale: arcsec/pixel max ANTWEAK = T / Tweak: yes please! ANTWEAKO= 2 / Tweak order ANSOLVED= './m67_4s_12800iso_1302145416.solved' / solved output file ANMATCH = './m67_4s_12800iso_1302145416.match' / match output file ANRDLS = './m67_4s_12800iso_1302145416.rdls' / ra-dec output file ANWCS = './m67_4s_12800iso_1302145416.wcs' / WCS header output filename ANCORR = './m67_4s_12800iso_1302145416.corr' / Correspondences output filename END XTENSION= 'BINTABLE' / binary table extension BITPIX = 8 / 8-bit bytes NAXIS = 2 / 2-dimensional binary table NAXIS1 = 16 / width of table in bytes NAXIS2 = 155 / number of rows in table PCOUNT = 0 / size of special data area GCOUNT = 1 / one data group (required keyword) TFIELDS = 4 / number of fields in each row TTYPE1 = 'X ' / X coordinate TFORM1 = 'E ' / data format of field: 4-byte REAL TUNIT1 = 'pix ' / physical unit of field TTYPE2 = 'Y ' / Y coordinate TFORM2 = 'E ' / data format of field: 4-byte REAL TUNIT2 = 'pix ' / physical unit of field TTYPE3 = 'FLUX ' / Flux of source TFORM3 = 'E ' / data format of field: 4-byte REAL TUNIT3 = 'unknown ' / physical unit of field TTYPE4 = 'BACKGROUND' / Sky background of source TFORM4 = 'E ' / data format of field: 4-byte REAL TUNIT4 = 'unknown ' / physical unit of field EXTNAME = 'SOURCES ' / name of this binary table extension SRCEXT = 1 / Extension number in src image IMAGEW = 4256 / Input image width IMAGEH = 2832 / Input image height ESTSIGMA= 2.020305 / Estimated source image variance DPSF = 1. / image2xy Assumed gaussian psf width PLIM = 4. / image2xy Significance to keep DLIM = 1. / image2xy Closest two peaks can be SADDLE = 2. / image2xy Saddle difference (in sig) MAXPER = 1000 / image2xy Max num of peaks per object MAXPEAKS= 10000 / image2xy Max num of peaks total MAXSIZE = 2000 / image2xy Max size for extended objects HALFBOX = 100 / image2xy Half-size for sliding sky window REMLINEN= 0 / Number of sources removed by "removelines.py" COMMENT The X and Y points are specified assuming 1,1 is the center of the leftmCOMMENT ost bottom pixel of the image in accordance with the FITS standard. HISTORY This xylist was filtered by the "removelines.py" program HISTORY to remove horizontal and vertical lines of sources HISTORY This xylist was filtered by the "uniformize.py" program END EQUE0~A A EE/~A` A0 EE\E@ A D8E0}A@ A E9 E