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https://ntrs.nasa.gov/search.jsp?R=19820022323 2018-07-13T20:08:14+00:00Z

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BRIGHT STAR CATALOGUE, 4th Edition

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(NASA-TM-84773) DOCUMENT.%1'ION FOR THE!MACHINE-VEADABL E VERSION Of THE BRIGHT STAR

MrA LIGUE ( NASA) 24 p HC A02 /MF A01 CSCL 03A

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May 1982

NSSDC/WDC-A-R&S 82-18

DOCUMENTATION FOR THE MACHINE-READABLE VERSION

OF THE

v

R.r?XGIIT STAR CATALOGUE, 9TH EDITION

Wayne H. Warren Jr.

May 1982

National Space Science Data Center (NSSDC)/World Data Center A for Rockets and Satellites (WDC-A-R&S)

National Aeronautics and Space AdministrationGoddard Space Flight CenterGreenbelt, Maryland 20771

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TABLE OF CONTENTS

Section 1 - INTRODUCTION AND SOURCE REFERENCE 1-1Section 2 - TAPE CONTENTS ., .......................................... 2-1Section 3 - TAPE CHARACTERISTICS .....,.........,... ► ....... . ..... .. 3-1Section 4 •• REMARKS, MODIFICATIONS, ACKNOWLEDGMENTS AND REFERENCES .. ► 4-1Section 5 - SAMPLE LISTING 5-1

LIST OF TABLES

Table

1 Tape Contents, Data File ...... ► ............. ► ......,........... 2-12 Tape Contents, Blank Records in Data File ................ .. ► .. 2-73 Tape Contents, Remarks DescrJ.ption File .................. ..... 2-84 Tape Contents, Remarks File 2-85 Tape Characteristics 3-1

iii

SECTION 1 - INTRODUCTION

The fourth edition of The BRIG11T STAR CATALOGUE (Hoffleit 1982) is an updatedand ,improved version or the provious edition published in 1964 by the sameauthor. In addition to the Large number of newly determined fundamental data,such as photoelectric magnitudes, MK spectral types, parallaxes, and radialvelocities, the new voxsion contains new data and information not included inthe third edition. Valuable information, such as the identification of xRsources, U-B and R-T colors, radial velocity comments (indication andidentification of spectroscopic and occultation binaries), and projectedrotational velocities, is included for the first time in the fourth addition,while the equatorial coordinates for equinoxes 1900 and 2000 are recorded togreater precision (0 0 1 in right ascension, 1" in declination). The remarkssection of the catalogue has been expanded and improved to contain manydetails concerning variability, spectral characteristics, duplicity, and groupmembership, and the remarks have been segregated by category to improveinformation retrieval and readability. The catalogue in general contains datacompiled through 19791 however, some information and variable-stardesignations found through 1981 are included in the remarks and manyvariable-star names have subsequently been transferred to the data file (seeSection 4).

This document describes the machine-readable version of The BRIGHT STARCATALOGURp 4th edition, as distributed by the Astronomical Data Center. It isintended to enable users to read and process the data without the commonproblems and guesswork often associated with such a task. For further detailson the compilation of the data and statistics of the catalogue, the sourcereference should be consulted. This document should be distributed with anymachine-readable version of the catalogue.

SOURCE REFERENCE

Hoffleit, D. (with the collaboration of Jaschek, C.) 1982, The BRXrjllT STARCATALOGUE, 4th revised edition (New Haven: Yale University observatory).

1-,1

t

SECTION 2 - TAPE CONTENT'S

A byte-by-byte description of the contento of the mAchine•readable ORMUT STAR('F^?ADOCUV, 4th Edition is given in Table 1, while Tables 3 and 4 describe thetiles aWsociated with the remarks. A suggested FORTRAN format specificationfor reading each datum is given in Table 1 and can be modified depending uponusagat however, caution is advised when substituting format specificationsrsince some data fields contain character data and others are blank whe)A, dataare absent. Particular care is required for color-index data, which can havevalid 0.00 values, but whose fields are blank when data are absent. It issafest to read such fields with A (character) Format specifications or tobuffer entire records in and check for blank fields before proceeding withinternal convarsi,on to binary numbers. Alternate format specifications aregiven in parentheses.

Table 1. Tape Contents. The BRXGHT STAR CATALOGUE, 4th Edition, Data File

SuggestedByte(s) tinits Format Descri tion

1- 4 14 BS w HR number.

5- 14 -_- A10 (10A1) Name, generally the Bayer and/orFlamsteed designation taken from the 3rdedition (Hoffleit 1964). This data fieldis divided uniformly, however, so thatcertain designations can be processedindividually by computer. An itemizeddescription of the name field follows:

5- 7 --- 33 Flamsteed number if one existst otherwiseblank.

8- 9 12 Coded Bayer designation (01 w a, 02 w $,..., 24 - w) ,, otherwise blank.

10- 11 --- 12 Sur.^Arscript number, for Bayer designationExample: HR 5545 22 T7 SER is coded:

2219 7SER

Note: There are exceptions to theuniformly coded Name iiel .d whic .,^ occur forblank records in the file. See Table 2for a list of the reoords and their Namefield contents.

12°- 14 r-- A3 Constellation abbreviation.

15 •»-- 1X Blank

2-1

x^

b

SuggestedByte( s) units Format Description

16- 23 ^-- AS Aurcheausterung (DM) number (BD north of-23 0 , CD from -23 0 to -520 , CpD :south of-520),

16 --- Al Sign of DM number.17- 18 --- A2 (12) DM zone.19- 23 - A5 (15) DM number.

24 --- 1x Blank

25- 30 --- IG Honry ,Draper Catalogue number.

31 - ix Blank

32 Al Infrared source flag (I if IR sourcalotherwise blank).

33 --- Al Reference for IR source when 1 is presentin byte 32 (blank if from NASA MergedInfrared Catalogue, Schmitz eat al. 1978)1' if from Engels et al. 1988). Colon (t)if uncertain identification..

34- 39 --- AG (6A1) Double or multiple stars (exceptspectroscopic and eclipsing)tNumber ADS (Aitken 1934)W Worley (1976) update of the IDS

(Jeffers eat al. 1963). Letters inbytes 40-41 following a W indicatewhich component(s) the HR numberrepresents

I xnnes (1927) southern double starsR Rossiter (1955)C CouteaL (1976)D Duplicity discovered by occultationS Duplicity discovered by speckle

interferometryA Ast,,ometric binary

The field is uniform on the tape (seeSection 4s ,remark 9) with the cataloguecode in byte 34, ADS numbers in bytes35-39 and components in bytes 40-41.,Additional remarks on duplicity may befound if an asterisk occurs in the notescolumn (byte 212).

2-2

i

R

R

i

l

i

i

i

r

i

`E

S:"r.

1 n

Suggested

Byte(g ) Units Format Description

40- 41 --- A2 Multiple-star components for systems forwhich HR number represents only certaincomponents of the system.

42 --- 1x Blank

43- 51 --- A9 (9A1) Variable star designations: (a) conetella-tin designations from the General Cata-loque of Variable St-ars (Kukarkin at al.1969-70), the Supplements 1-3 (Kukarkinet al. 1971, 1974, 1976), and the 62ndthrough 66th Namelists (Kukarkin at al.19761 Khol,opov at al. 1978, 1979, 1981) 1

(b) Numbers (alone) from the Catalogue ofstars suspected of Variabillty Kurkarkinat al. 1951, 1965)t (c) VAR and VAR? forunnamed variables as of dune 1981 and aus-pected unconfirmed variables not includedin the gonaral catalogues. Can apply tothe HR number and/or a close companion.

52 --- 1x Blank

53- 54 hours 12 Might ascensions (a) for 1900.

55 --- 1x Blank

56- 57 min 12 a58 --- 1X Blank

59- 62 sec x'4.1 aG3 --- 1X Blank

64 --- Al Sign of declination (6) for 1900.65- 66 a 22 6

67---

ix BlankG8- G9 ' 12 a

70 --- 1X Blank71- 72 01 12 6

73 -- 1x Blank

74- 75 hours 12 Right ascension (a) for 2000.76 --- 1X Blank

77- 78 min 12 a79 --- 1x Blank

80- 83 sec F4.1 a

84 --- 1x Blank

2-3

a^i

s

Fable 1. (22 Bugg)

SuggestedB te(s) Units Format Description

85 --- Al sign of declination (d) for 2000,86- 87 12 d

88 --- 1X Blank89- 90 ' 12 d

91 --- 1x Blank92- 93 '" 12 d

94 --- 1x Blank

95-100 0 F6.2 Galactic longitude 11.

101 --- 1x Blank

102-107 ° F602 galactic longitude xr.

106 --- 1X Blank

109-113 mag P'5.2 Visual magnitude (see byte 114), Somema gnitudea of variables and double starsare ralortod to 0.1 mag only, in whichcase byte 113 is blank.

114 --- Al Visual magnitude coda: blank w V on UBV(Johnson) systems R - HR magnitudesreduced to the UBV systeml H w original.HR magnitude.

115 --- 1x Blank

116-120 mag F5.2 B-V on Johnson system] otherwise blank.

121 --- ix Blank

122-126 mag x'5.2 U-B on Johnson systeml otherwise blank.

127 --- 1x Blank

128-132 mag F5.2 R--r on system indicated by the code inbyte 1331 otherwise blank.

133 --- Al Code for R-T systeml blank - on Johnsonsystems E - mainly from Eggen, on Karonsysteml C - from cousins; close to ;Cronsystem (the Johnson and iron filters havedifferent Xeff and may not be used inter-.changeably).

134 --- 1X Blank

e

f ;Ait

2-4,^ E

t

i

f

F

O

Suggested8 te(s) Units Format Descri Lion

135-154 20A1 (5A4) Spectral type, if the complete moderndetermination is too long for the datafield, it is giv n in the remarks file andthe last charactAr in the spectral-typefield is an astoisk (*). Mt. Wilsonluminosity classes are given in lower caseletters in bytes 135-136. The OW'r intoo: ':-Rayet types is in byte 137, but ingeneral the temperature class (o, Br A,«,. 5, C) is in byte 137 and can beselected using only that byte. Charactersnormally appearing as lower case instandard notation (e.g. p, a t Si, Mnr Tag,

lab) are coded in Lower case on the tape.Where Greek letters appear in a spectraltype, the coding used in the Name :Meld(see bytes 8-5*,) is employed, but thenumber is surrounded by Ope.g. b Del. - <04>nel..

155 ---- 1X Blank

156-161 " r6.3 Annual proper motion, 1 I a,r in rightascension. Sign always in byte 156.

162 --- 1x Blank

163-168 " F6.3 Annual proper motion, PS t in declination.Sign always in byte 163.

169 --- Al "D" if Following parallax is dynamicalrather than trigonometric: otherwiseblank.

170-174 F5.3 Trigonometric parallax unless a "D" iscoded in byte 169. sign always in byte170 for ntrig, and For n dyn . Blank For nodata.

175 --- ix Blank

176-179 km s-1 14 Radial velocity or blank (sere codes infollowing field).

2-5

suggested,Buse (s ) Unites rormat pescri Lion

180-183 --- A4 (4Al) Radial-velocity comments$ V,, , V? - variable or suspected variable radialvelocity) SDI SS1, SD2 - spectroscopicbinaries, single or double lined spectral0 - orbital data Available*

184 --- 1x Blank3

165 Al projected rotational velocity (v sin i)descriptive character. 'r<rr - less than; ?

less than or equal to (haxidecimalcharacter code 8C').

186-188 km s`" 1 13 v sin i

leg - Al colon (t) for uncertain v sin 1.

190 -- 1X Blank

191-194 mag F4.1 ©n, magnitude difference between two

t/components of a doublea, or between the twobrightest components of a multiple system.

195 - 1x Reserved for colon (z) to indicate Amuncertainty (none occurs, however).

196-201 rr p6.1 Separation of the same two componentsreferred to in bytes 191-194.

202 -- 1x Blank

203-206 -- 4A1 (A4) identification of the componentsrepresented in bytes 191-194 and 197-201.An " O rr in byte 204 indicates anoccultation binary.

207208 --- 12 (A2) Numbers of components assigned to amultiple system.

209-211 -- 3X Blank

212 --- Al An asterisk (*) indicates a note in theremarks file. otherwise blank.

2-6

C

i

There ace fourteen records in the data file wh 9h are blank except for HRnumber, Name, and sometimes VAttable -star doal,5ymntions. Theme rsoordsrepresent objects included in the first edition of the aAtAlogue and omittodin subsequent editions. (The records are retained in order to preserve the,numbering of the first catalogue * ) They are listed below so that theprogrammer can see what their fields contain, since they must be considered ifone is attempting to decode the Lrlamsteed and Bayer designations. The namesbelow begin in byte 6.

Table 2. Tape Contents. The r: 9XOIIT STAR CJ1TAZOCr f 4th Edition, Data File,Blank Records

,.

. HR Name Variable Des ignation

92 NOVA 15' 2 B CA$95 47 TUC

182 M 31 AND1057 NOVA 1901 GK PER1841 NOVA 1891 T AUR2472 NOVA 1903 DM ITEM2496 NGC 228107 19 rl v73671 NGC 28086309 NOVA 1848 V 941 OPH6515 NOVA 1603 V 843 OPti7189 NOVA 1899 V1016 SGR7539 NOVA 1670 CK VUL8296 NOVA 1876 Q CYG

2-7

1^

The second file of the catalogue contains a description of the remarks file,including the not4Won and abbreviations employed.

Table 3. Tape Contents, The BnXGF1T STAR CATALOGUE; 4th Rdition, RemarksDescription rile.

Bytes Descri tion

1 . 80 Free text in upper and lower case characters,

Fable 4, Tape Contents. The BRXGf1T STAR CATALOGUE, 4th Edition.Remarks rile.

Suggested

Bite (s ) Format Description

7- D is BS - HR number.

6- 7 2X Blank

8 . 11 A4 Remark category abbreviation [upper casescharacter(s) :starting in byte 83a N - Star names;C - Colors; S - Spectral VAR - Variability;SD - Spectroscopic binarieist RV - Radial, and/orrotational velocities; D - Double and multiplestarsi DYN - Dynamical. parallaxes; R - Stellar radiior diameters; P Solarization; G - Groupmembership; M - Miscellaneous. The categoryabbreviation is always followed by a colon (s).

12 1X Blank

13-132 3074 Remarks in free text form.

For printing only, the note can, of course, be read with a formatspecification of 12W or 33A4. Note that the remarks are in upper and lowercase characters, so the use of an extended chain printer is recommended. ifan extended chain printer is available, it may be desirable to decode theGreek letters, subscripts and supersoripts, in which case the RemarksDescription File (2) should be consulted for decoding information.

2-8

SECTION 3 .. TAPE CHARACTZRI8TXC8

The information in Table 5 is sufficient for A user to describe the indigenouscharacteristics of The ARIGHT STAR CATALOGUE, 4th edition, to a computer. Notincluded is information easily varied from installation to installation, suchas block dire (physical record length), blocking factor (number of logicalrecorAs per physical record), total number of blocks, gape density, number oftracks, and internal coding (ZuCDIC, ASCII, etc#). Thew& parameters shouldalways be transmitted if secondary copies of the catalogue are supplied toother users or installations, Parameters for the three files are separated bycommas*

Table 5. Tape Characteristics # Thai BRIGHT STAR CATALOGUC, 4th Edition

NUMBER OF FILES #{ r R f 4 1#! f f f.! 1 1##.# .. 1 #iii . f. Y. 1. f 1 f f f F i M I 3

LOGICAL RECORD LENGTH (BYTES) f r«. ..:. ..:.r..+rr r :.+ • . . + 2 121 80 1 132

RECORD FORMAT i f i#•. 11 !. 1 w f i r w 1. w. i i# i i. i i .. # i.# i w w. i i ... i .. ra^

TOTAL NUMBER OF LOGICAL AECOrJ)S .e.. 1.1.. i+ ...w .«w++.... 9110, 5e, 7959

* fixed block length (last block may be short)

3-1

SECTION 4 - REMARKS, MODIFICATIONS$ ACKNOWLEDGMENT$ AND RWORENCES

A magnetic tape of The DRXGHT STAR CATALOGUE, 4th edition data file wasreceived from Dr. E. Dorrit Hoffleit of Yale University Observatory on 10 1'March 1982. An additional magnetic tape containing four files (tape descrip-tion, remarks file description, remarks files anc supplementary remarks file)was requested and received on 22 April 1982. As received, the data werecontained on 18 tape files comprising left- and right-hand pages for groups of1000 stars. The following modifications were made to the data and remarksfiles.

1. The 18 files on the original tape were processed through a program tocombine them into a single data file of 9110 logical records. RedundantHR numbers of the right-hand-page files were removed.

2. The character "D"', signifying a dynamical parallax, occurred in byte 170(within the parallax data field). Since this would case problems for anumerical format specification, these characters were moved to byte 169(originally not used) and a "+" sign was place6 into byte 170 to matchthe trigonometric values normally in the data field.

3, The descriptive character 11411 for projected rotational velocity (byte185), available on printers but not on terminals, was present as a colon0) in the original records (the < sign occurred in its correct form,however). The colon was changed to hexidecimal character 8C, which willprint as a < sign on extended chain printers. Installations not havingthe S character will need to detect the 8C code and convert it to anothercharacter if it is to be printed.

4. A full spectral type of 21 characters was present for HR 8667. Since theallowed ll.ata field could not accommodate the type, it was shifted to theleft, thereby misaligning the temperature clP:ss. The spectral type wastherefore shortened, an asterisk (*) was appended in the normal fashion,and the full type was moved to the remarks file.

5. Also, the component separation for HR 1175 (1480 11 ) did not fit into theallotted field in the original format, so it was present in bytes 198-201as a shifted number having no decimal. point. Since byte 196 was neverused, the number was rewritten as 1480. in bytes 196-201, which is nowthe designated field for separation data.

6. Since the tape description file for the remarks applied only to theoriginal tape, it has been omitted from the catalogue.

7. As received, the remarks records had a problem whenever byte 132 (thelast byte of a logical record) contained a non-blank character, in thatan indeterminate character had been inzarted into byte 1 of the followingrecord and all successive bytes of that record were shifted to the right..

4-1

since this was apparently done by the DEC computer at Yale when the tapewas prepared, every occurrence of the indeterminate character was removedand the records shifted to align i4th the remaining remarks records.

B. The supplementary remarks file on the original tape had been preparedbecause additions and corrections were found after the remarks file hadgone to press. For brevity and ease of processing, the supplementaryremarks were merged into the main remarks file by performing the correc-tions noted and adding additional remarks to their appropriate locationsin the main remarks file,

9. The doublo-star fields (bytes 35-41) were not uniform in all cases: (a)numbers and letters occupied the same bytest (b,) the letter codes forcatalogue sources and components were not always in the same positionsiand (c) some numbers were shifted in the data field. The double-starfield was reviewed for all catalogue entries and edited to make the datauniform. The catalogue code (W I A, S, etc.) was moved to byte 34(originally blank) so that no number/letter overlap now occurs.

10, following a suggestion by Dr. Hoffleit, variable-star designations whichhad been added to the supplementary remarks after the data file had beencompleted were transferred to the variable-star fields of the maincatalogue and removed from the remarks.

ACKNOWLEDGMENTS

Appreciation is expressed to Dr. E. Dorrit Hoffleit and Mr. A. Partan forpreparing and sending the magnetic tapes of the data and remarks file, and toDr. Noffleit for communicating additional corrections to the data File and forreviewing this document.

REFERENCES

Couteau, P. 1976, Ciro. Xnf. No 75 (Meudon: TACT Commission des EtoilesDoubles)

Engels, D., Sherwood, W. A., Wamsteker, W. and Schultz, G. V. 1981, Astron.Astrophys. Suppl. 45, 5.

Hoffleit, D. 1964, Catalogue of Bright Stars, 3rd edition (New Haven: YaleUniversity observatory).

Hoffleit, D. (with the collaboration of Jaschek, C.) 1962, The BRIGHT STARCATALOGUE, 4th revised edition (New Haven: Yale University Observatory).

Tnnes, R. T. A. 1927, Southern Double Star Catalogue, -19" to -900,(Johannesburg: Union Observatory).

4-2

REFERENCES (continued)

aeffers, H. Mo e van don Bose W. H. and Greeby, F. M. 1963, ,index Catalogue ofVisual Double Stars, Pub;,. Lick Obs. 21.

Kholopove P. No t Kukarkina, N. P. and Perova, N. B e 1978, 63rd Name-Last ofVariable Stars, Xnf, Bull. Variable Stars, No. 1414.

Kholopovr P, N., Kukarkina, N. P. and Perova, N. Be 1979, 69th Name-List ofVariable Stars, snf. Bull. Variable Stars, No. 1581.

Kholopov, P• N•, Samus', No N., Kukarkina, N. Per Medvedeva, G. I. and Perova,

N. Be 1981 0 65th Name-List of Variable Stars., Tnf. Bull. Variable Stars,No, 1921,

Kholopov, P, N., SamuS', N. N., Kukarkina, N. Per Medvedevar G. I. and Perova,N. Be 19e1 r 66th Nama-List of Variable Stars, X"nf. Bull. Variable Stars,No. 2042.

Kukarkin, Be Vol Parenago, P. P., Efremov, Yu. No and Kholopov, P. N. 1951,Catalogue of Stars Suspected of Variability (Moscow: Publishing House ofthe Academy of Sciences of the U.S.S.R.).

'Kukarkin, Be v., 1holopov, P. N., Bfremov, Yu. N., Kukarkina, tie P.,Kurochkin, N. E,, Medvedeva, G, I., Perova, No Be, Pskovsky, Yu. P.,Fedorovich, V, P. and Frolov, M. S. 1971, First Supplement to the ThirdEdition of the General Catalogue of Variable Stars (Moscow: PublishingHouse of the Academy of Sciences of the U.S.S.R.).

Kukarkin, Be V., Kholopov; P. N • , Efremov, Yu. N., Kukarkina, No PerKurochkin, N. E•, Medvedeva, G. I., Perova, N. Be, Pskovsky, Yu. P.,Fedorovich, V. P. and Frolov, M. S. 1974, Second Supplement to the ThirdEdition of the General Catalogue of Variable Stars (Moscow: PublishingHouse of the Academy of Sciences of the U.S.S.R.).

Kukarkin, Be V., Kholopov, P. N,, Fedorovich, V, Per Kireyeva, N. Nor

Kukarkina, N. P.,.Medvedeva, G. I. and Perova, N. Be 1977, 62nd Name -List ofVariable Stars, Xnf. Bull. Variable Stars, No. 1248.

Kukarkin, Be V., Kholopov, P, N., Kukarkina, N. P., Kurochkin, No E.,Medvedeva, G. Ise Perova. N. B., Pskovsky, Yu. Per Fedorovich, V. P, andFrolov, M. S. 1976, Third Supplement to the Third Edition of the GeneralCatalogue of VariablE Stars (Moscow: Publishing House of the Academy ofSciences of the U.S.S.R.).

Kukarkin, Be V., Kholopov, P. N., Efremov, Yu. No and Kurochkin, N. Be 1965,Second Catalogue of Stars Suspected of Variability (Moscow: PublishingHouse of the Academy of Sciences of the U.S.S.R.).

4-3

REFERENCES - (concluded) ,

Kukarkin, 13, V. Kholopov, P. N., 4?skovskX, Yu« P., Sfremov, Yu. N.,Kukarkina, N. P., Kurochkin, N. Z., Medvedeva, G. x., Perova, N. D.,redorovich, V. P. and Frolov, M. S• 1969-70, General Catalogues of Variables jStars, 3rd edition (Moscow: Publishing Houses of the Academy of Sciences ofthe U.S.S.R.).

Rossiter, R. A. 1955, Cataloguo of Southern Double Stars,,,Publ. Cb^. Univ.W chi gnn 9 .

Schmitz, M. , Brown, L. W o , Mead, J. M. and Nagy) r To A. 1978, Mergred ,Xnfrare dCatalogkie, NASA TM-79683.

"

4-4

SECTION 5 -• SAMME LISTING

The s mple listings given on the following pages ,present logical data recordsfroLu each file just as they are recorded on the tape. Groups of records fromthe beginning and and of each file are illustrated. The beginning of eachrecord And bytes within the record are indicated by the column heading acrossthe top of each page (digits read vertically). Since files 1 and 3 containmore than 115 bytes per record, the remaining bytes (116-212 in file 1,116-132 in file 3) are printed in a second row.

5-1

ORIGINAL PAr." E3

OF POOR QUALITY

-•r,11

. n 0 .. a o 01 ': otW 4D At ll1 111 111 0 0 A W 10, A

nr0,49-• O s1-•Oh to .t M co N co 411 m At b 0% h h at vw010 `10 r JI ?i m m h r 09 N b N m^09

nd' •D ^+ V1 h M t0 r

t'9++O1 9f1 P1 0; co, 14 14

O r 10 ^0 at 10NM [• h '0 h h %a M— ON 1 1 1 1 1 I I I 1 I 1 I t Iq --

"'00 at M M'1 Q1 M r w t0 r b N 10 r # M010% » M h ^' p' NO C N N m IV UT 01 M r-mco e

00 (+ 4 O; * r a► M 0; A N 111 t» ^m r%tM tn

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M^

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m m U M O N N ^'" A. N tN't M M No 1O+ N b 111 M 00 0 't +t m M h N N m N ON st tG q ^^+ U1 at` at l<t' w N w. N r N 01 M b N U1.WO + I 1 t + 1 t + t I I 1 I I^•

A+mm co N h "! o1 01 O to h t11 O +" O t* 0, O N cowN • • a • • • • • •- • • • • • • •

0+ M 0' ' q ar0 M N mco

—

NN m

M 1A NhOt N in w t+ 1H r- t] thnt^+

to to In to w 10 w ^o a t+ h h . oo co coAi N

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nwntn o o d o ^ o o d O p O q o q dnnMhM to n M \0PN N O1 O *" M lA w N in r N 09

cm09 b N O to CO t11

N r M N 4 M1 N r r # M "" N in r •+ rrno v

1001 O M t0 O N h o7 co 01 a t0 m in p NW OD, A "' O to to M m N m u'1 Mwlho

bbAt %0 0 N h ON m m oo M M M at M a0 0

10 N At to tl1 0 N t0 d N N 0• N P M N N H10 u + co I 0 I to + N + N I m+ a t

co( M I 1 m 1 M I h 1 ^+ Nt0 m ^+ * r .+ w .+

WN r N b w w at at N O w t'► M. 10 W O-%00 r t0 m M r 00 at 4iw r^ — ^? co 0 M11104 %n " at M h O M ar to " ri

ON

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O O O r r b r •+ O •- N N N N m m 0• 1 • •

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++

Q- ^+1 O p OA

O O O O O O. O OOP m N 119 0 u1 W N U1 t% co O M O 1 11 0' wto r ill 09 O M m D` h M cr O' at O O VIln^ O O O O O q 4 •'^ O O O* O O O r

Di inat 09 O O O O O O p O O O O p O O O

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