File:37 coma berenices.jpg

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Description37 coma berenices.jpg	English: Image of star 37 Com created by Aladin previewer. 中文：后发座37（周鼎二）的图像。
Date	29 May 2011
Source	Space Telescope Science Institute，NASA
Author	Aladin previewer

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	This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
	Warnings: Use of NASA logos, insignia and emblems is restricted per U.S. law 14 CFR 1221. The NASA website hosts a large number of images from the Soviet/Russian space agency, and other non-American space agencies. These are not necessarily in the public domain. Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI.[1] See also {{PD-Hubble}} and {{Cc-Hubble}}. The SOHO (ESA & NASA) joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use. [2] Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. [3] The National Space Science Data Center (NSSDC) site has been known to host copyrighted content. Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	05:36, 29 May 2011		768 × 768 (44 KB)	Iamchenzetian (talk \| contribs)	{{Information \|Description ={{en\|1=Image of star 37 Com created by Aladin previewer.}} {{zh\|1=后发座37（周鼎二）的图像。}} \|Source =NASA \|Author =Aladin previewer \|Date =2011-05-29 \|Permission = \|other_versions

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File:The meeting of day and night in a mountain valley with invisible pink unicorn.jpg

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Usage on ky.wikipedia.org
- Жылдыз
Usage on pl.wiktionary.org
- ἀστήρ
Usage on ru.wiktionary.org
- 𐍃𐍄𐌰𐌹𐍂𐌽𐍉
Usage on zh.wikipedia.org
- 周鼎二

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SIMPLE = T / file does conform to FITS standard BITPIX = 16 / number of bits per data pixel NAXIS = 2 / number of data axes NAXIS1 = 768 / length of data axis 1 NAXIS2 = 768 / length of data axis 2 BZERO = 0. / PhysValue = BZERO + BSCALE * ArrayValue BSCALE = 1. / PhysValue = BZERO + BSCALE * ArrayValue COMMENT Standard WCS reduction: CRVAL1 = 195.068689499984 / WCS Ref value (RA in decimal degrees) CRVAL2 = 30.7850367222373 / WCS Ref value (DEC in decimal degrees) CRPIX1 = 384. / WCS Coordinate reference pixel CRPIX2 = 384. / WCS Coordinate reference pixel CD1_1 = -0.00027994385451684 / WCS Coordinate scale matrix CD1_2 = -3.17650320773367E-06 / WCS Coordinate scale matrix CD2_1 = -3.17650320773367E-06 / WCS Coordinate scale matrix CD2_2 = 0.00027994385451684 / WCS Coordinate scale matrix CTYPE1 = 'RA---TAN' / WCS Coordinate type CTYPE2 = 'DEC--TAN' / WCS Coordinate type EQUINOX = 2000. / Equinox RADESYS = 'FK5 ' / Coordinate system MJD-OBS = 49093.2820833333 / Modified Julian Date at start of observation EPOCH = 1993.28893109742 / Epoch in Julian Year at start of observation CUNIT1 = 'DEG ' / RA Coordinate Unit CUNIT2 = 'DEG ' / DEC Coordinate Unit CDELT1 = 0.000279961875715917 / WCS Coordinate scale matrix CDELT2 = 0.000279961875715917 / WCS Coordinate scale matrix COMMENT Standard WCS reduction: ORIGIN = 'CASB -- STScI ' /Origin of FITS image PLTLABEL= 'SF05110 ' /Observatory plate label PLATEID = 'A0ZK ' /GSSS Plate ID REGION = 'XP443 ' /GSSS Region Name DATE-OBS= '1993/04/16 ' /UT date of Observation UT = '##################' /UT time of observation XPLTRAH = 13 / Plate center RA XPLTRAM = 4 XPLTRAS = 1.5124752666678E+01 PLTDECSN= '+ ' /Plate center Dec PLTDECD = 29 / PLTDECM = 48 / PLTDECS = 4.2217839999998E+01 / EXPOSURE= 1.2000000000000E+02 /Exposure time minutes BANDPASS= 35 /GSSS Bandpass code PLTGRADE= 0 /Plate grade PLTSCALE= 6.7199996948240E+01 /Plate Scale arcsec per mm SITELAT = '+33:24:24.00 ' /Latitude of Observatory SITELONG= '-116:51:48.00 ' /Longitude of Observatory TELESCOP= 'Palomar 48-in Schm' /Telescope where plate taken CNPIX1 = 14175 / New CNPIX1 CNPIX2 = 14637 / New CNPIX2 DATATYPE= 'INTEGER*2 ' /Type of Data SCANIMG = 'XP443_A0ZK_01_00.PIM' /Name of original scan SCANNUM = 1 /Identifies scan of the plate DCHOPPED= F /Image repaired for chopping effects DSHEARED= F /Image repaired for shearing effects DSCNDNUM= 0 /Identifies descendant of plate scan image XPIXELSZ= 1.5029459953310E+01 /X pixel size microns YPIXELSZ= 1.5000000000000E+01 /Y pixel size microns PPO1 = -3.0694170000000E+06 /Orientation Coefficients PPO2 = 0.0000000000000E+00 / PPO3 = 1.7750000000000E+05 / PPO4 = 0.0000000000000E+00 / PPO5 = 3.0694170000000E+06 / PPO6 = 1.7750000000000E+05 / AMDX1 = 6.7125858914605E+01 /Plate solution x coefficients AMDX2 = -1.7099853133797E-01 / AMDX3 = -2.9351315397844E+02 / AMDX4 = -3.4086184506888E-05 / AMDX5 = 1.7970780776335E-05 / AMDX6 = -1.8410776887200E-05 / AMDX7 = 0.0000000000000E+00 / AMDX8 = 2.4764366122428E-06 / AMDX9 = -3.3781428350811E-08 / AMDX10 = 2.3097963064171E-06 / AMDX11 = 6.9086083390832E-10 / AMDX12 = 0.0000000000000E+00 / AMDX13 = 0.0000000000000E+00 / AMDX14 = 0.0000000000000E+00 / AMDX15 = 0.0000000000000E+00 / AMDX16 = 0.0000000000000E+00 / AMDX17 = 0.0000000000000E+00 / AMDX18 = 0.0000000000000E+00 / AMDX19 = 0.0000000000000E+00 / AMDX20 = 0.0000000000000E+00 / AMDY1 = 6.7128246618532E+01 /Plate solution y coefficients AMDY2 = 1.7674252257576E-01 / AMDY3 = 3.1473075358839E+02 / AMDY4 = 4.5223165365682E-05 / AMDY5 = -1.8863782189854E-05 / AMDY6 = 1.8857190597407E-05 / AMDY7 = 0.0000000000000E+00 / AMDY8 = 2.2794883926525E-06 / AMDY9 = -6.9561167347992E-08 / AMDY10 = 2.3095189208090E-06 / AMDY11 = 5.0763924552193E-08 / AMDY12 = 0.0000000000000E+00 / AMDY13 = 0.0000000000000E+00 / AMDY14 = 0.0000000000000E+00 / AMDY15 = 0.0000000000000E+00 / AMDY16 = 0.0000000000000E+00 / AMDY17 = 0.0000000000000E+00 / AMDY18 = 0.0000000000000E+00 / AMDY19 = 0.0000000000000E+00 / AMDY20 = 0.0000000000000E+00 / NBFCPYRT= 2 /Number of brief copyright statement lines BFCPYRT1= 'Copyright (c) 1992-2000, Caltech and AURA; subject to all records in'BFCPYRT2= 'the header file. ' / NFLCPYRT= 12 /Number of full copyright statement lines FLCPYRT1= 'The compressed files of the "Palomar Observatory - Space Telescope' FLCPYRT2= 'Science Institute Digital Sky Survey" of the northern sky, based on' FLCPYRT3= 'scans of the Second Palomar Sky Survey are copyright (c) 1993-2000' FLCPYRT4= 'by the California Institute of Technology and are distributed herein'FLCPYRT5= 'by agreement. All Rights Reserved.' / FLCPYRT6= ' ' / FLCPYRT7= 'All material not subject to the above copyright provision is' / FLCPYRT8= 'copyright (c) 2000 by the Association of Universities for Research' FLCPYRT9= 'in Astronomy, Inc. All Rights Reserved.' / FLCPYRTA= ' ' / FLCPYRTB= 'Produced under Contract No. NAS5-2555 with the National Aeronautics' FLCPYRTC= 'and Space Administration.' / END

File:37 coma berenices.jpg

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