Outline o What is an array ? o Indexed array o Associative array o Multidimensional array.
August 5, 1987 · 1.5-mSeeing 25K IRAFonMV8000 14K 1.5-mEchelle 24K RC Spectrograph Filters 12K...
Transcript of August 5, 1987 · 1.5-mSeeing 25K IRAFonMV8000 14K 1.5-mEchelle 24K RC Spectrograph Filters 12K...
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.
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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.
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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