NATIONAL OPTICAL ASTRONOMY OBSERVATORIES

FY 1987 PROGRAM PLAN

Addendum To Revision I

August 5, 1987

Table of Contents

PageI. INTRODUCTION 1

II. RESEARCH HIGHLIGHTS FOR FY 1986 3

A. Solar System Astronomy 3B. Galactic Astronomy 4C. Extragalactic Astronomy 7

III. FY 1987 SCIENTIFIC STAFF AND SUPPORT. 11

A. Staffing 11B. Scientific Program 11

1. Kitt Peak National Observatory. 122. National Solar Observatory 163. Cerro Tololo Inter-American Observatory 194. Advanced Development Program 23

C. Research Experience for Undergraduates (REU) Program 25a

IV. MAJOR PROJECTS AND INSTRUMENTATION 26

A. Major New Projects 281. NTT-Technology Development 282. GONG 30

B. User Instrumentation 31C. Research and Development 34D. Computer Developments. 36E. Major Facility Improvements 37F. Construction 39

V. OPERATIONS AND MAINTENANCE 40

A. Telescope Operations and User Support 40B. Program Support 42

1. Director's Office 422. Central Facilities Operations 423. Central Administrative Services 424. Public Information Office 435. Engineering and Technical Services 436. AURA Management 44

C. Major Facilities Maintenance 44a

VI. NON-NSF PROJECTS 45

APPENDIX 1 - NOAO Organizational Chart 48APPENDIX 2 - NOAO Management 49APPENDIX 3 - Scientific Staff and Primary Fields of Interest 50APPENDIX 4-User Statistics, FY-1986 54APPENDIX 5-Budget Tables 55

C. Research Experience for Undergraduates (REU) Program.

In December 1986 the National Science Foundation (NSF) announced a new programto attract talented students into research careers in the fields of mathematics, science and engineering. NOAO was invited to submit proposals both as an REU participation site and also as a supplement to a current program supporting researchexperience for minority students. Competitive proposals were submitted and basedupon the merits of the proposals awards were made. NOAO is very pleased to participate in the REU program. Our past experience in working with students-boththrough the minority program and through the summer research assistantprogram-coupled with this year's experience in working with students under theREU program testifies to the continued need for support of such programs.Currently there are twelve students participating in NOAO's REU site program.Eleven of the students are engaged in 12-week summer research programs either atNOAO's facility in Tucson or in Sacramento Peak. The twelfth student is working inTucson on a year-long project. Because of the delay in receiving the approval forthe supplemental program for minorities we were not able to advertise and activelyrecruit students for participation in that program for the summer. However, wewere able to attract one minority student from the University of Arizona for 12weeks this summer. In addition we have been in contact with the University ofArizona Minority Office regarding recruitment of minority students for participationin the REU program during the Fall 1987 semester. Through this method of reaching out to local minorities we expect to extend the REU program benefits to an additional five students.

The thirteen students currently involved in research with NOAO scientists are working on a variety of projects. As an illustration of how well this program is workingwe would like to briefly outline the projects and the benefits both the students andthe advisors are gaining from these interactions.

(1) Renate Kupke; W. Livingston, advisor; Tucson; Fourier Tach Spectrometer,Observations and Reductions (one year project).

This project is operating on a campaign basis-12 hours a day. Renate is takinga half-day observation. In addition she is learning to observe with the McMathtelescope and helping with the reduction of those observations.

(2) Tracy Hodge; D. Backman, advisor; Tucson; Analysis of Infrared Spectroscopyand Photometry of Epsilon Aurigae.

Tracy is receiving her first exposure to new astronomical data and the stepsleading from definition of an experimental problem to production of ascientific paper. She has participated in a 4-m observing run on Kitt Peak.Through her participation in the completion of a project which has beengranted long-term observing status at Kitt Peak for high-resolution (FTS)infrared spectroscopy of the binary star epsilon Aurigae she will also participate in the preparation of a review article on the subject of that same star.

(3) Marlisa MacLeod; S. Keil, advisor; Sacramento Peak; Energy Transport in SolarMagnetic Regions.

Marlisa is learning to handle large data bases, use an interactive graphiclanguage, write fortran subroutines for finding spectral parameters, how to useFourier techniques to filter and smooth data, and is being exposed to forefrontsolar research. The data she reduces will be incorporated into our program todetermine how magnetic fields alter the normal flow of energy through thesolar atmosphere and to understand how the solar atmosphere is heated.

25a

(4) Gregory Leonard; M. Giampapa, advisor; Tucson; Heating of the Chromosphereof a dMe Flare Star.

Gregory is benefiting from an introduction to advanced techniques for theanalysis of spectroscopic data as obtained with a modern spectrograph anddetector system. The advanced techniques involve the Fourier analysis of atime series of spectra of a dMe flare star. Through Gregory's assistance inreducing and analyzing the numerous spectra resulting from this particularexperiment this project will be completed at least four months earlier thanwithout his participation.

(5) Kenneth La ; J. Harvey, advisor; Tucson; Solar Rotation and Large Scale MotionsDeduced from Daily Motion of Small Magnetic Features.

Through his active participation in this project Kenneth is gaining an appreciation of the complexities of a full-scale research project. He is learning newtechniques of data reduction as well as being exposed to different computingtools and the operation of a modern astronomical telescope and its instrumentation. With Kenneth's assistance we will be able to make substantial progresson this research problem.

(6) Amy Barton; T. Kinman, advisor; Tucson; Identification of UCG and ZwickyGalaxies in Selected Fields.

Amy's participation in this project will gain her familiarity with the major starcatalogs and how these may be used to derive positions of the programobjects. She will be using the Grant two-coordinate comparator in conjunctionwith our Vax computer system to make these measurements. The actual measurements are being made on our glass copies of the Palomar survey. This combination of measuring machine and survey plates is only found in very fewobservatories in the world. Amy will also be writing a number of Fortran programs that will sort the data that she has measured and put the results into auseful format. She has already visited Kitt Peak for two nights and haswatched a number of astronomers observing.

(7) Walter Bennet; K. Hinkle, advisor; Tucson; Instrumentation for FourierTransform Spectroscopy.

Walter is getting a detailed introduction into the design and fabrication ofinstruments for large optical telescopes. This includes cryogenic and highvacuum equipment as well as optical components. He has made a number ofparts and assembled the optics for an experiment with GaAs detectors that weplan to undertake in August.

(8) David Williams; R. Altrock, advisor; Sacramento Peak; Analysis of Coronal Transients.

David is gaining familiarity with solar physics from a hands-on perspective andis getting a real education in solar physics data bases, image processing anddisplay, and computer operation, as well as the specific subject of coronal transients. David's efforts in data reduction and the early analysis portion of thisresearch project will lead to the production of a research paper authored byDavid and his advisor.

(9) Mary Hrovat; D. Neidig, advisor; Sacramento Peak; Measurements of the Spectrum and energetics of the 25 April 1984 White Light Flare.Mary is gaining an introduction to recent literature, analysis techniques andmajor scientific questions on the topic of solar flares. She also is gaining firsthand experience in working with computers and a microdensitometer, as wellas direct, working-level interaction with the personnel and activities of a majorastronomical observatory. Through Mary's participation in this project she and

25b

her advisor will co-author resulting scientific publications.

(10) David Borthwick; M. Belton, advisor; Tucson; Modelling the Rotation of theNucleus of p/Halley.

Through the new programming techniques that David learns a program topredict the brightness of p/Halley, as a function of time will be gained. In theprocess David will learn how to conduct a scientific research program, and beexposed to an area of astronomy currently emphasized in the national spaceprogram. David's program will be used by his advisor in conjunction withobservational results to establish a rotational ephemeris for p/Halley.

(11) Kevin Strobel; P. Massey and J. Barnes, advisors; Tucson; SpectrophotometricStandard Stars.

Kevin is learning the ins-and-outs of data reduction and analysis by reducingIRS and IIDS data on these standard stars. In addition this project allows Kevinto become familiar with the physical basis for the magnitude system. Throughthis project we will gain information on good fluxes to use for doing spectrophotometry.

(12) Gwendolyn Sweeney; C. Pilachowski, advisor; Tucson; Experiments in ImageQuality Control (minority program).

Gwendolyn is participating in several projects in adaptive optics. She isinvolved in a program to measure seeing on Kitt Peak, and in several projectsto develop new interferometric instruments at NOAO.

(13) John Boia; L. Davis, advisor; Tucson; Imaging Detectors Standards Consortium.

John is making great progress in reducing the Imaging Detectors StandardsConsortium observing data. In the course of this work he has also streamlinedthe reduction process considerably. Through this program John has gainedexperience in working in a scientific environment and in using modern computer facilities. He has also acquired a good background in photoelectric photometry, CCD photometry and photometric data reductions. It is expected thatthe reductions will be essentially complete by the end of the summer whenDavid leaves NOAO.

25c

IV. MAJOR PROJECTS AND INSTRUMENTATION

ADP

DEEPS $55KAdaptive Optics (IR) 197KInterferometric Distributed Array 230KCoatings & Gratings Research 65K

547K

NTT

NTT Mirror Development & General Studies 2016K4-m Design 50K

2066K

CTIO

Workstation/IRAF on Tololo 74KTektronix CCDs 51KMyclops II 45KTelescope Controllers 20K4-m Fiber Optic Feed 32KRutgers Fabry-Perot 7K1.5-m Seeing 25KIRAFonMV8000 14K1.5-m Echelle 24KRC Spectrograph Filters 12KSBRC Array Imaging System 41KSBRC Array Spectrometer 71KPrime Focus Corrector 6KSouthern Site Survey 18KLibrary Addition 36K

476K

KPNOWorkstation 95K

NSO - TucsonWorkstation 39KMcMath Improvements 15KInteractive Time-Series Display 16KSYNOP Spectrograph 30KFourier Tachometer 39K

139K

NSO - SunspotWorkstation Upgrade 8KCHIRP (Multi-Diode Array & Tower Mass Storage) 173KAdaptive Optics 103K

284K

Observatory InstrumentationIR Detector R&D 68KCTIO/KPNO Imager Instrument 106K

26

KPNO IR Spectrometer Instrument 148KCryogenic Echelle Instrument 158KIR Electronics #3 and #4 98KCryogenic Optical Bench 76KFTS A/D Converter 20KMcMath Stellar CCD 20KSpectromagnetograph 82KKPCA 79KCCD Development 92KTektronix CCDs 31KLab Dewar 26KCCD@KPN0 2.1-m 2KGold Spectrometer Camera Design 46KFiber Optics Cryogenic Camera Feed 15KSOHO/SOI Proposal 14K

1081K

GONG 1010K

Central Computer ServicesTelescope Control Software 65KCommunication Links 70KSupercomputer Installation 4KIRAF 110KWorkstation Program 88K

337K

This chapter discusses the major new projects (i.e. the development oftechnology for the next generation of telescopes--NTT-and GONG), the baseinstrumentation program and the new projects and instrumentation Initiativeswhich NOAO will be conducting in FY 1987. Within the base and Initiativesprograms we include new focal plane instrumentation, innovative ways to conductexperimental and observational astronomy, major improvements to existingfacilities, and development of computer-based capabilities. Not included aresmall telescope-improvement projects which are budgeted directly underOperations and Maintenance and carried out to the extent possible by a supportgroup whose primary responsbility is for maintenance of the existing telescopesand observing equipment.

We distinguish, then, six areas under this program category of major facilitiesand instrumentation, each one of which may be carried out within NOAO or incoordination with an external group:

• Major New Projects - principally new telescopes.Continuing work directed towards the provision of unique,powerful new capabilities for U.S. optical astronomy must berecognized as an essential central element of NOAO andmust be constantly present in its program.

• User Instrumentation - designed and constructed to providethe best possible capabilities for the user community incombination with the reliability and general user-friendlinessappropriate for national facilities.

27

C. Major Facilities Maintenance

The budget cuts of the past few years, combined with the reprogramming of fundstoward major initiatives such as the development of technology for the next generation of telescopes and the construction of the GONG network, have left us withsome serious maintenance problems that must be corrected. Two such items wereserious enough that we chose to reprogram monies originally earmarked for initiatives to operations and maintenance to address these problems.

(1) Frequency Converter (CTIO).One of the important early decisions of the AURA Board with respect to CTIO wasthe decision to have all electrical power on the mountain be 60 Hz. Originally, thisrequirement was not an inconvenience since all mountain power was provided by adiesel generator which could be run at either 50 or 60 Hz. However, the tremendous increase in the cost of fuel during the last decade caused CTIO to eventuallytie into the Chilean national network (ENDESA), saving roughly $100,000 per year.ENDESA now provides the mountain with a 50 Hz high voltage line which must bestepped-down via a frequency converter, i.e., a continually operating motor whichtakes the incoming voltage and gives out voltage at 60 Hz. The present converterwas purchased in 1976, and has a maximum output of 300 kilowatts.Because of the heavy increase in power demands in the past few years from morecomputers, refrigeration units, cryogenic pumps, etc., CTIO is operating daily nearthe capacity of the present converter. During the month of March 1987 the frequency converter overloaded twice and shutdown. These shutdowns are never"gentle", inasmuch as insulation burns and bushings score. Each time it has beennecessary to run off the emergency generator for a few days-which is adequate butexpensive-and we have been fortunate in being able to fix the converter. Thefailures in the present converter have already impacted the mountain operations tothe extent that it has been necessary to suspend much of the telescope seeingimprovements program, which involved cooling oil and using fans to circulate airthrough the domes, because of their power requirements. In addition there is considerable concern that any subsequent shutdown will cause severe damage to theconverter. Because of the urgency in this matter we have purchased a new frequency converter capable of 500 KW output. By the end of FY 1987 this problemshould be resolved.

(2) Roof (Tucson Offices).The roof on the older part of the headquarters building in Tucson is now 14 yearsold. Despite several attempts to patch the roof, many new leaks developed duringheavy winter rains this year. Acoustic ceiling tile and walls were damagedthroughout the building, and leaks into the computer room were so extensive thatwe were forced to shut down the computing system temporarily.We have concluded that the most cost effective solution is to remove the existingroofing and replace it down to, but not including, the metal deck. Damage is extensive, including fractures, bubbles, and overall deterioration of materials; anyattempt to make repairs would be a waste of funds and manpower. The roofingmaterials are saturated with water; the insulation has been compacted to such anextent that it no longer serves as an effective insulator. We are presently installinga roofing system that will consist of an insulation board, which will provide an R-19value, covered with a monolithic sheet of modified bitumen membrane which,because of its elastic properties, will be less likely to be damaged by traffic andbuilding movement caused by the extremes of Tucson temperatures. A protective

44a

layer of white coating will then be applied to reflect the Sun, thus lowering the rooftemperature during the summer and further preventing breakdown. The system hasa ten-year guarantee and a life expectancy of 15 to 20 years.

44b

VI. NON-NSF FUNDED PROJECTS

Listed below are NOAO programs whose funding derives from sources other thanNSF. Funding for some programs may extend beyond the current fiscal year.

Principal Projects:

USAF:

USAF:

USAF:

USAF:

USAF:

NASA:

NASA:

NASA:

NASA:

USAF:

OSD:

NASA

NASA

NASA

OSD:

Optical Testing for Large OpticsSacramento Peak SupportSolar Optical Observing Network (SOON)Adaptive OpticsMultilayer UV Mirror ResearchFTS Program for Upper Atmospheric ResearchInfrared Astronomy Satellite (IRAS)Project GalileoTuneable Wide Field Lyot FilterImage Enhancement Techniques

Multilayer UV Mirror ResearchVacuum Telescope SupportNASA/RMT - MIT/ETC ProjectsSpace Telescope Imaging Spectrograph (STIS)Interferometric Imaging

Other Projects:

NASA

NASA

NASA

DOE:

NASA:

NASA:

NASA:

NASA:

NASA:

NASA:

NASA:

NASA:

NASA:

NASA:

Solar Optical Telescope (J. Beckers)Solar Maximum Mission FilmSolar Optical Telescope (J. Harvey)Battelle Terrestrial MonitoringSupport of On-Site PersonnelSolar Maximum Mission TravelStellar Winds in Hot StarsTucson WorkshopComet HalleyWorkshop/Jovian SystemPhotometry & Astronomy of HalleyX-Ray Emitting StarsChromospheric Coronal EmissionsFlare StarsMiscellaneous projects less than $5K each

634K600K

150K

175K

100K

70K

117K

66K

57K

50K64K

72 K

96K

357K

71 K

24K

21K

20K

17K

18K

13K

9K9K9K

6K

7K

9K

8K5K

44K

2898K

USAF: Optical Testing for Large OpticsK. Shu and C. Roddier are principal investigators for this proposal to the USAF'sRome Air Development Center (RADC) for a program of optical test methodimprovements intended to shorten the time required to test large optics andimprove the spatial resolution obtainable. Funds provided are for payroll costsof scientific and engineering staff and for purchase of optical and computercomponents.

45

USAF: Sacramento Peak SupportUnder a Memorandum of Understanding between the United States Air Force(USAF) and the National Science Foundation (NSF), the USAF provides fundingto support a group of USAF employees who are physically located at SacramentoPeak and who support programs/projects which are of special interest to theUSAF.

USAF: Solar Optical Observing Network (SOON)The Solar Optical Observing Network (SOON) is a USAF-funded project for thefabrication and installation of five solar telescopes located worldwide. The finalSOON telescope was installed in Europe in FY 1986 under the direction of R.Dunn. Spare parts will be fabricated and delivered to the USAF this year tocomplete the project.

USAF: Adaptive OpticsThe USAF has provided NSO with funding to initiate development of a secondgeneration adaptive mirror. The work includes development of a phase detectorsystem, development of an interferometer to measure fringes from the activemirror surface, and development of an improved mirror control system with arange several times that of the first generation mirrors.

USAF: Multilayer UV Mirror ResearchThe USAF has asked M. Giampapa to expand his OSD funded subcontract withLockheed Space and Missile Company for multilayer mirror research. The USAFprogram studies soft x-ray spectral regions and selects those wavelengths whichwill provide the best diagnostics for solar active regions. Funding also providesfor the design, fabrication, and testing of normal incidence mirrors in theselected spectral regions.

NASA: FTS Program for Upper Atmospheric ResearchJ. Brault is participating in this project as principal investigator. Primaryactivities are upper atmospheric studies utilizing the FTS at the McMathtelescope.

NASA: Infrared Astronomy Satellite (IRAS)F. Gillett's participation on the Science Team of the IRAS will continue. In FY1987 he will participate in the processing of data obtained by the satellite,analyze the data in collaboration with a number of other scientists and preparethe results for publication.

NASA: Project GalileoM. Belton is participating in Project Galileo as the team leader for the SolidState Imaging System. Funding will be used to support Dr. Belton's travel toteam and project meetings, the cost of consultants to the team, and thedevelopment of a "Home Institution Image Processing System (HUPS) to beinstalled at the NOAO Tucson offices.

NASA: Tuneable Wide Field Lvot FilterR. Dunn and R. Smartt are principal investigators of this proposal submitted toNASA. During FY 1987 they will oversee the design and fabrication of atuneable wide field Lyot filter.

46

NASA: Image Enhancement TechniquesR. Smartt is heading a program to develop a correlation tracker algorithm andhardware for use with the Sacramento Peak Tower Telescope. The USAF hasalso provided funds for the installation of an active optics system at SacramentoPeak. The systems will be used to obtain diffraction-limited images of solaratmospheric dynamics and activity.

NASA: Vacuum Telescope SupportNSO has provided the solar physics community with full-disk, high resolutionmagnetograms and He 10830 spectroheliograms for a number of years using theVacuum Telescope for synoptic observations. Since 1979, NASA (a primary userof this data) has been providing funding to assist in the operational support andimprovement of the telescope.

NASA: NASA/RMT - MIT/ETC ProjectsB. Teegarden of NASA, in collaboration with G. Ricker of Massachusetts Instituteof Technology (MIT), will be operating the Rapidly Moving Telescope (RMT) andthe Explosive Transient Camera (ETC) on Kitt Peak for at least the next fiveyears. NASA funding is for support provided by KPNO operations personnel.

NASA: Space Telescope Imaging Spectrograph (STIS)NASA has provided funds to support S. Wolff and R. Green for theirparticipation in the STIS Instrumentation Definition Team. In addition, NOAOwill support the STIS instrument by testing CCD images and serving as technicalliaison between the manufacturer, the STIS team, and NASA. Finally, NOAO willprovide technical and scientific assistance in choosing the final flight packageddevice(s).

OSD: Interferometric Imaging

F. Roddier is performing research to demonstrate that image reconstructionthrough turbulence is feasible both in visible and infrared without a referencesource by combining pupil-plane interferometry with bi-spectral analysis.

47

National Optical Astronomy ObservatoriesFY-1987 Program PlanAddendum to Revision I

OnOn

NSF FUNDING

Advanced Development Program

New Telescope Technology

Cerro Tololo Inter-American

Observatory

Kitt Peak National Observatory

National Solar Observatory

Sunspot

USAF Support

Tucson

NASA Support

Observatory Instrumentation

Global Oscillations Network Group

Central Offices

Director's Office

Reserve

Resource & Program Management

Central Administrative Services

Central Facilities Operations

Central Computer Services

Central Engineering &

Technical Services

Management Fee

Total NSF Funding

NON-NSF FUNDING

NSF Funded

Non-NSF Funded

Total

Scientlf c

Staff 8 nstru-

Support3

mentatlo

$ 408 $ 547

2,066

900 440

1,529 95

370 284

664 139

1,081

1,010

130

95 337

$4,096 $5,999

73.35 67.80

APPENDIX 5

TABLE I

FUNDING BY SOURCE

(Amounts 1n Thousands)

Operations

8

mentation Construction Maintenance

36

$ 36

$ 295

3,528

4,029

1,702

<600>

493

<49>

258

335

1,270

1,441

658

$14,020

STAFFING SCHEDULE

(In Full Time Equivalents)

325.56

1 Includes NSF carryover of $1,627K and non-NSF carryover of $1,300K.2 Includes $1,100K new funds for UA mirror development subcontract.3 Includes $70K new funds for REU Programs, see Table 1-B.

Management Total Total Total

Fee FY-1987 ' FY-1986 FY-1985

$ $ 1,250 $ 635 $ 598

2,066 2 1,683 2,192

4,904 4,765 5,292

5,653 5,972 6,136

2,356 2,258 2,406

<600> <600> <435>

1,296 1,200 948

<49> <45> <45>

1,081 916 879

1.010 331 246

$ 426

388 193 348

335 <329>

145 37

1,270 1,129 1,083

1,441 1,332 1,401

1,090 1,242 1,698

660 583 766

426 399 378

$24,577 $21,809 $23,928

2,898 1,471 865

$27,475 $23,280 $24,793

466.71

6.15

472.86

462.90

10.13

490.15

1.00

491.15

TABLE I-A

ADDENDUM TO

FUNDING BY SOURCE TABLE

(Amounts In Thousands)

NSF Funding

Director's Office—Operations and Maintenance

Office of the Director

Visiting Committee TravelCXI

°^ Performance Awards

NOAO Director Search Committee

AURA/NSF Solar Science Study

Indirect Cost Credits

Minority Program

Office of University Relations

Visitors Program - Foreign Travel

Public Information Office

Total $258 $193 $348

FY-1987 FY-1986 FY-1985

$265 $283 $271

18 18 7

21

10

10

<193> <253> <1A0>.

12

38

20 19 23

117 126 127

5^] SunspotTucson

TABLE 1-B

ADDENDUM TO

SOURCE OF FUNDING TABLE

(Amounts in Thousands)

Research Experience for Undergraduates (REU) Programs

(Amounts shovm are included in Scientific Staff & Support on Table 1)

Kitt Peak National Observatory

National Solar Observatory

Central Offices

NOAO Pirector's Office

Central Computer Support

Numbier of Students

Funding Supported

23 6

12 3

17 3

14 A

4 1

Total 70

To be determined in the Fall of 1987.

U1

00

Personnel Costs

Supplies 8 Materials

Utilities 8 Communications

Purchased Services

Domestic Travel

Foreign Travel

Equipment

Real Estate

Subtotal

USAF 8 NASA Support

Total NSF Funding

Scientists

Engineers 8 Scientific

Programmers

Administrators & Supervisors

Clerical Workers'

Technicians

Maintenance 8 Service

Workers

Total

TABLE II

SUMMARY OF NSF FUNDING BY COST CATEGORY

(Anounts 1n Thousands)

ADP CTIO KPNO

NSO OBSERVATORYSUNSPOT TUCSON INST. GONG

CENTRAL MANAGEMENT TOTAL TOTAL TOTAL

OFFICES FEE FY-1987 FY-1986 FY-1985

798 $ 518 $2,573

176 11 1,063

276

77 1,410 326

37 20 44

16 5 183

146 102 439

$4,052 $1,398

831 298

$1,053 $ 743

74 311

306

<3>

115

70

282

265

119

35

36

57

13

63

$1,250 $2.066 $4,904

$1,250 $2,066 $4,904

$5.653 $2,356 $1,296 $1,081

<600> <49>

$5.653 $1.756 $1.247 $1,081

STAFFING SCHEDULE

(In Full Time Equivalents)

8.50 15.50

1.50 7.00 13.50 9.25 5.00 2.00

11.00 6.00 3.00 1.00

1.50 .80 22.80 9.50 4.10 2.25

5.00 5.00 38.50 31.00 13.00 5.50

30.50 9.00

16.50 12.80 139.30 21.75

.50

14.50

21.50

$ 613 $2 ,827

154 386

529

24 916

25 100

3 48

191 378

$1,010 $5,184

$1.010 $5.184

8.50

6.50

15.00

13.25

14.00

30.36

13.30

14.00

$14,575 $14,006 $14,495

3,304 3.244 3,416

1,376 1.378 1,434

3,338 1,939 2,509

438 315 382

353 356 412

1.842 1,216 1,754

6

$ 426 $25,226 $22,454 $24.408

<649> <645> <480>

$ 426 $24.577 $21.809 $23.928

70.10 71.00 75.00

66.50 64.00 60.50

35.00 43.00 53.00

71.31 70.10 71.40

132.30 125.55 128.00

91.50 89.25 102.25

466.71 462.90 490.15

TABLE III

SCIENTIFIC STAFF a SUPPORT

(Amounts In Thousands)

ADP CTIO 1KPNO

NSO CENTRAL

OFFICES

TOTAL

FY-1987

TOTAL

FY-1986

TOTAL

SUNSP0T TUCSON FY-1985

Personnel Costs $ 368 $ 796 $1 ,250 $ 309 $ 605 $ 189 $3,,517 $3 ,169 $3,037

Supplies 8 Materials 11 35 90 12 27 7 182 160 134

Purchased Services 4 48 12 3 67 35 15

Domestic Travel 11 4 35 20 19 27 116 52 45

Foreign Travel 7 48 65 6 10 2 138 101 106

Equipment

$

11

408 $

13

900 $1

41

.529 $

11

370 $4

76

,096 $3

44

.561

56

Total $ 664 $ 225 $3,393

Scientists

Engineers 8 Scientific

Programmers

Clerical Workers

Technicians

Total

7.50

1.00

4.50

20.00

STAFFING SCHEDULE

(In Full Time Equivalents)

22.85 4.00 10.00

1.50 1.00

5.50 11.00 4.50

63.35

1.00 1.00

5.50 6.50 5.50

4.50 1.50 1.00

71.50 73.25

ONo

TABLE IV

INSTRUMENTATION

(Anounts 1n Thousands)

CENTRAL

ADP NTT CTIO KPN0

NSO OBSERVATORY

INST. GONG

COMPUTER

SERVICES

TOTAL

FY-1987

TOTAL

FY-1986SUNSPOT TUCSON

FY-1985

Personnel Costs $ 233 $ 518 $ 243 $ $ 71 $ 54 $ 743 $ 613 $ 104 $2,579 $2,414 $2,356

Supplies 8 Materials 128 11 117 80 3 311 154 30 834 742 1,078

Purchased Services 64 1,410 11 19 7 24 27 1,562 1,005 1,228

Domestic Travel 5 209 5 25 1 65 36 75

Foreign Travel 5 3 7 3 2 20 <4> 31

Equipment

$

117

547

102

$2,066 $

66

440

95

$ 95

133

$ 284

54

$ 139

8

$1

191

,010 $

173

337

939

$5,999

612

$4,805

1,322

Total$1 ,081 $6,090

Scientists

Engineers 8 Scientific

Programmers 1.50

Administrators 8 Supervisors

Clerical Workers

Technicians 3.50

Maintenance 8 Service

Workers

Total 5.00

7.00 2.50

5.00 8.50

12.80 11.00

STAFFING SCHEDULE

(In Full Time Equivalents)

.50

1.00 6.50 8.50

14.50 6.50

.50

1.00

1.00 1.25

28.00

.80

38.00

1.00 21.50 15.00 1.50 67.80 62.90

2.00

29.85

4.50

1.50

29.63

.50

67.98

O

TABLE V

CONSTRUCTION

(Amounts 1n Thousands)

NSO CENTRAL TOTAL TOTAL TOTAL

ADP CTIO KPNO SUNSPOT TUCSON OFFICES FY-1987 FY-1986 FY-1985

Personnel Costs $ $ $ $ $ $ $ $ * 11

Supplies 8 Materials 24 24 42

Purchased Services 12 12 36

Total $ $ 36 $ $ $ $ $ 36 $ $ 89

ON

TABLE VI

OPERATIONS I MAINTENANCE BY COST CATEGORY

(Aaounts In Thousands)

ADP CTIO KPNO

NS0 CENTRAL

OFFICES

TOTAL

FY-1987

TOTAL

FY-1986

TOTAL

SUNSP0T TUCSON FY-1985

Personnel Costs $ 197 $ 1,534 $2,802 $1,018 $ 394 $2,534 $ 8,479 $8,423 $ 9,091

Supplies 8 Materials 37 887 741 206 44 349 2,264 2,342 2,162

Utilities 8 Communications 276 306 265 529 1,376 1,378 1,434

Purchased Services 13 299 <51> 107 14 889 1,271 500 852

Domestic Travel 21 40 80 15 29 72 257 227 262

Foreign Travel 9 132 5 2 3 44 195 259 275

Equipment 18 360 146 89 9 205 827 560 376

Real Estate6

Subtotal $ 295 $3,528 $4,029 $1,702 $ 493 $4,622 $14,669 $13,689 $14,458

USAF 8 NASA Support <600>

$1,102 $

<49>

444

<649>

$14,020

<645>

$13,044

<480>

Total $ 295 $3,528 $4,029 $4,622 $13,978

STAFFING SCHEDULE

(In Full Time Equivalents)

Scientists 1.00 1.00 1.75

Engineers 8 Scientific

Programmers

Administrators & Supervisors

Clerical Workers

Technicians

Maintenance 8 Service

Workers 38.00 30.50

7.25

11.00 9.25 5.00 1.00 12.25 38.50 30.25 29.65

11.00 6.00 3.00 1.00 14.00 35.00 43.00 48.50

1.50 21.80 7.50 2.60 1.25 30.36 65.01 63.60 64.40

1.50 25.50 31.00 13.00 5.50 13.30 89.80 95.15 97.37

91.50 89.25 101.75

4.00328.50 348.92

ON

TABLE VII

OPERATIONS S MAINTENANCE BY TYPE OF SERVICE

(Amounts 1n Thousands)

ADP CTIO KPNO

N!;o CENTRAL

OFFICES

TOTAL

FY-1987

TOTAL

FY-1986

TOTALSUNSPOT TUCSON FY-1985

Engineering 8 Technical

Services $ 115 $ 656 $1,054 $ 252 $ 81 $ 660 $ 2,818 $ 2,228 $ 1,850

Telescope Operations 522 886 605 255 2,268 2,104 2.086

Mountain Operations 880 1,527 672 3.079 3,068 3,156

Central Fadl itles/Tucson/

La Serena Operations 561 221 1,441 2.223 2.015 2,188

Central Computer Services658 658 408 735

Administration 180 909 341 173 157 1,528 3,288 3,866 4,444

Reserve335

$4,622

335

$14,669Subtotal OSM $ 295 $3,528 $4,029 $1,702 $ 493 $13,689 $14,459

USAF 8 NASA Support <600>

$1,102

<49>

$ 444

<649>

$14,020

<645>

$13,044

<480>

$13,979Total 08M-NSF Funds $ 295 $3,528 $4,029 $4,622

STAFFING SCHEDULE

(In Full Time Equivalents)

Engineering 8 Technical

Services 1.50

Telescope Operations 25.00 19.00 10.00 7.75

Mountain Operations

Facilities

Central Computer Services

Administration 2.50 24.30 6.00 4.10 2.00

10.00 16.00 8.00

25.00 19.00 10.00

33.00 36.00 10.50

16.00 5.00

4.00

24.30 6.00 4.10

Total 4.00 108.30 86.00 32.60 9.75

14.50 50.00

61.75

79.50

22.00 43.00

13.80 17.80

34.61 73.51

84.91 325.56

60..60

61..00

79,.35

41..00

7,,55

79.,00

328. 50

56 .92

62 .10

91..25

47..00

15..75

75.,90

348. 92

Purchased Services

ON

TABLE VIII

MANAGEMENT FEE

(Amounts In Thousands)

CTIO KPNO

NS 0 CENTRAL

OFFICES

TOTAL

FY-1987

TOTAL

FY-1986

TOTAL

ADP SUNSPOT TUCSON FY-1985

$ $ $ $ $ $ 426 $ 426 $ 399 $ 378

ONon

Personnel Costs

Supplies 8 Materials

Utilities t Communications

Purchased Services

Domestic Travel

Foreign Travel

Equipment

Total

Engineers 8 Scientific

Programmers

Clerical Workers

Technicians

Total

ADP

$312

73

314

12

17_

$728 $ 9

NON-NSF PROJECTS

(Amounts In Thousands)

KPNO SUNSPOT TUCSON

$342

24

$ 106

213

$ 72

21

202 817 186

34 16 17

4 30

64 3 10

$670 $1,185 $306

STAFFING SCHEDULE

(In Full Time Equivalents)

1.00

1.00

.25

1.00

1.25

1 In some Instances, funding extends beyond the current year.

CENTRAL

OFFICES

TOTAL

FY-1987 1TOTAL

FY-1986

TOTAL

FY-1985

$ 832 $ 315 $ 97

331 24 91

4 4

1.521 948 474

79 36 29

41 48 6

94 96 164

$2,898 $1 ,471 $865

.25

1,.50

6,.15

4.00

.75

5.38

10.13

1.00

1.00