Transcript
National
Optical Astronomy Observatories
NATIONAL OPTICAL ASTRONOMY OBSERVATORIES
FY 1990 PROGRAM PLAN REVISION 1
June 1, 1990
National
Optical Astronomy
950N.Cherry Ave. P.O. Box 26732 Tucson, Arizona 85726-6732
(602)327-5511
Observatories Kitt Peak National Observatory
FAX: (602) 325-9360
Telex 1561401 Aura Ut Internet: noao (5 noao. edu
CerroTololo Inter-American Observatory
National Solar Observatory
June 1, 1990
Mr. Seth L. Turtle
Program Manager, NOAO Room 618 Division of Astronomical Sciences National Science Foundation
1800 G Street, N.W.
Washington, D.C. 20550 Dear Seth:
Enclosed are 10 copies of Revision 1 to the National Optical Astronomy Observatories' FY 1990 Program Plan incorporating the changes requested in Ms. Karen Sandberg's letter of April 19, 1990. The revision consists of the following pages: New -
Section II.C, Research Experiences for Undergraduates, pp. 20a - 20b.
Revised -
Section IV.A., Instrumentation for Cerro Tololo Inter-American Observatory, pp. 30 - 31.
New -
Section VII, Non-NSF Funded Projects, pp. 46 - 50.
Revised -
Appendix 4, FY 1989 User Statistics.
Revised -
Appendix 5, Budget Tables.
The revised Plan reflects the following actions which were necessary to achieve the required reduction in FY 1990 funding: GONG hardware acquisitions deferred
$400,000
Across-the-board program cuts
$510,000
Savings in personnel costs including reduced salary
$260,000
increases and deferred hiring for open positions
C<& Sidney
olff
Director
Operated by the Association ofUniversities for Research in Astronomy, Inc. (AURA) under cooperative agreement with the National Science Foundation
sjp enclosures xc:
G.
Oertel
OAC Members NOAO Associate Directors
NOAO Deputy Directors NOAO Unit Heads
II.
C. Research Experiences for Undergraduates.
The Research Experiences for Undergraduates Program (REU) is an integral part of NSF's overall plan 10 strengthen undergraduate science, engineering and mathematics education throughout the United Slates. This requires continuing efforts to attract talented students into research careers in these fields, and to help ensure that they receive the best education possible. There is widespread agreement (National Science Board Task Committee on Undergraduate Science and Engineering Education) that active research experience is one of the most effective techniques for training undergraduates for such careers, and that too few experiences are now available. NSF has established the REU Program to help meet this need.
For the past couple of years, NOAO has been invited to submit proposals as a REU participation site. Awards were made based upon the merits of the proposals received, and NOAO is pleased to have been awarded funds each time. Our past experience in working with students testifies to the continued need for support of such programs.
The NSF award of $50,000 for the 1990 Summer Research Experiences Program will be used to fund 11 research assistants; seven in Tucson, Arizona and four in Sunspot, New Mexico. This award will cover salary, travel and fringe benefits for a 12-week period. Of the 11 students, four will be assigned to work with KPNO staff; four with NSO Sunspot staff; two with NSO Tucson staff; and one with CCS staff members.
Some of the proposed research work for the summer of 1990 follows: One student will be involved in two projects; both related to phenomena in the Jovian system. In the first, he/she will investigate the evolutionary development of 'plume' activity in Jupiter's equatorial region. This project is in the data collecting phase. In the second project, emphasis will be on the theoretical prediction of the sum-mm line spectrum of a possible S02 atmosphere of Io and CO atmosphere on Pluto.
A second student will work with two staff members in generating artificial images using existing software; reducing crowded artificial stellar field images with IRAF/DAOPHOT; and participating in the evaluation of the results. The student will also write small sppIRAF tasks to analyze and display the results.
Another summer task to be undertaken will be theoretical modeling. This project will involve hydrodynamic or magneto hydrodynamics (MHD) flows in active galaxies or clusters of galaxies. Using the newly-implemented CCD on the Schmidt telescope, one member of staff was able to obtain UBV CCD images of most of Cyg OB2, and spectra for many of the brighter stars without previously known spectral types using the multi-object fiber-fed device Nessie on the 4-m Mayall Telescope. The REU student will help reduce and analyze these data.
20a
A fifth student will work on the analysis of high-resolution spectral line profiles in late-type, high luminosity stars. Another will work on the reduction and analysis of spectroscopic data obtained with the NSO McMath CCD system on Kitt Peak and the Jack Evans Facility at Sacramento Peak. There will be one of three projects awaiting another student. This student will either obtain and reduce observations of the full solar disk with the solar Vacuum Telescope on Kitt Peak; transfer archived data to a modern storage media in a standardized format; and handle data reduction for information obtained at the geographic South Pole in November 1988. The students at Sacramento Peak will work on projects related to the Max '91 collaboration that will emphasize activity studies over the next few years. The research assistants will obtain observations, handle data analysis, and work with modeling of the solar processes.
20b
IV. INSTRUMENTATION
A. Cerro Tololo Inter-American Observatory. Non-
Payroll $33K
Major Projects
CCD TV acquisition cameras Prototype CCD controller Second generation IR imager
Payroll $38K
$ 71K
57K
30K
87K
60K
28K
88K
Total
4-m PF corrector
32K
3K
35K
Large format prime focus CCD
55K
UK
66K
Smaller Projects 1.5-m bench mounted echelle
IK
IK
4-m cassegrain focus filter bolt Spectrograph control Miscellaneous projects
4K
4K
5K
20K
15K
36K
36K
Evaluation/Comparison of New Telescope Sites
15K
47K
62K
$303K
$ 167K
$470K
The FY 1990 CTIO projects budget has been allotted to the following efforts, Five major projects will consume the major fraction of available manpower and capital resources. CCD TV acquisition cameras. This project represents the production of multiple copies of the very successful, thermo-electrically cooled CCD TV acquisition camera developed during the past year. When completed, these will be installed on all of the four major telescopes. Prototype CCD controller, production of CCD controller. A prototype design for a new array controller is nearing completioa This major effort aims to replace the "Vidicon electronics boxes" which together with the Forth 11 LSI/11 computer systems have been the workhorse optical detector controllers for the observatory for most of the past decade. The new controller, based on transputers and integrated into the Sun-based IRAF data reduction environment, will control all the CCD instruments at CTIO and, with slight modification, the IR array instruments as well. The project will move into the initial production phase during the latter half of FY 1990, in which five copies of the controller will be produced. The capital cost includes some effort on the IR controller. Second generation IR imager. The new IR imager is to be designed to use the larger format IR array detectors which are now becoming available. In addition, the instrument will permit use of the narrow-band (2%) linear variable filters which have been purchased and a polarimeter. More flexible input optics will permit the use of the detector at different plate scales on the CTIO 4-m, 1.5-m and 0.9-m telescopes. The optics will be designed to handle the PtSi arrays already purchased as well as the somewhat larger format arrays we expect may become available over the next five years.
4-m PF corrector. The funds for the optical components of this wide field corrector and atmospheric dispersion corrector (ADC) were committed in FY 1989. The optics will be received and the corrector will be built in FY 1990. The wide field and ADC will have important benefits for the Argus multiple 30
fiber spectrograph and with the new larger-format CCDs being purchased. Capital costs in the table reflect those remaining.
Large format prime focus CCD. To take advantage of the new wide field corrector and the larger format CCDs being procured, this project will, in addition to permitting use of a large-field, permit one use of grisms and short-scanning techniques. In addition to these the following smaller projects were also allocated funds: 1.5-m bench mounted echelle; 4-m cassegrain focus filter bolt; and the spectrograph control.
Finally, a major investment will be made, primarily for contract manpower, to continue the evaluation and comparison of the sites for new telescopes on the AURA property in Chile, at Cerro Pachoh, Cerro Morado, and Cerro Tololo.
31
VTJ.
NON-NSF FUNDED PROJECTS
Listed below are NOAO programs whose funding derives from sources other than NSF. Funding for some programs may extend beyond the current fiscal year. Principal Projects:
InK's
USAF
Sacramento Peak Support Adaptive Optics Micro-Advanced Coronagraph 3.5-m and Advanced Optical Testing
NASA
STIS
141
USAF USAF
USAF
$625 203 188 174
USAF
Liquid Crystal Filter
140
NASA
IRAF Extension
139
NASA
SOI/MDI Project Vacuum Telescope Support
104
NASA
96
NASA
Galileo Mission
78
NASA
RMT - MIT/ETC Projects
76
NASA
IRAS
73
NASA
Tuneable Lyot Filter Upgrade Coronagraph Solar Mass Ejection Imager Fabry Perot Filter
56
44
USAF/U/AZ
Upper Atmospheric Research 3.5-m Honeycomb Mirror
NASA
Stellar Winds in Hot Stars
35
USAF
Video Imaging System Upgrade Polarimeter NOAA Support for J. Brault SOT Support for J. Harvey Chromospheric Emissions Photometry of Halley Interferometric Imaging CO Synoptic Study X-Ray Luminosity Functions Miscellaneous projects less than $10K each
29
USAF USAF USAF
50 50 50
Other Projects: NASA
USAF
NOAA NASA NASA NASA
OSDS/SDI NASA
NASA
38
25 17 17
16 16 13 12 11
57
$2,573
Total
USAF: Sacramento Peak Support
Under a Memorandum of Understanding between the United Sutes Air Force (USAF) and the National Science Foundation (NSF), the USAF provides funds ($600K) for general support of a group of USAF personnel who are physically located at Sacramento Peak and who support programs/projects which are of special interest to the USAF. Additional funding ($25K) is provided to help support a Research Assistant to perform data reduction. 46
USAF Adaptive Optics
The USAF has provided NSO with funding to continue development of a second generation adaptive mirror. The work includes development of a phase detector system, development of an interferometer to measure fringes from the active mirror surface, and development of an improved mirror control system with a range several times that of the first generation mirrors. USAF Prototype Micro-Advanced Reflecting Coronagraph
R. Smartt serves as principal investigator at NSO/SP on this project with the USAF to fabricate 15-cm super-polished mirrors through a subcontract to an optical company; to evaluate the scattering properties of these mirrors in laboratory conditions using the optical evaluation facilities of the Evans Solar Facility at SPO; to develop a fast CCD camera and data processing systems for detecting faint objects rapidly; and to integrate the optics and detector package on the Evans Solar Facility spar. Testing of the system will be conducted during this second year of the project USAF 3.5-m and Advanced Optical Testing
C. Roddier is the principal investigator for this proposal to the USAF's Rome Air Development Center (RADC) for a program of optical test method improvements intended to shorten the time required to test large optics and improve the spatial resolution obtainable. Funds provided are for payroll costs of scientific and engineering staff and for purchase of optical and computer components. NASA Space Telescope Imaging Spectrograph (STIS)
NASA has continued to provide funds to support S. Wolff and R. Green for their participation in the STIS Instrumentation Definition Team. In addition, NOAO will support the STIS instrument by testing CCD images and serving as technical liaison between the manufacturer, the STIS team, and NASA. In addition, NOAO will provide technical and scientific assistance in choosing the final flight package device. USAF Liquid Crystal Filter
This project for the USAF will develop a Liquid Crystal Filter. Work will include obtaining a controller system for rapid wavelength tuning of both the liquid crystal device and the universal birefringent filter that will permit acquisition of vector magnetograms, interfacing the controller to filters, and documentation of the controller system. NASA Extension of IRAF Support
Continuing the work begun in 1982, the NOAO Central Computer Service personnel have again been supported by NASA in the project to develop the Image Reduction and Analysis Facility (IRAF) Software. This software, which has now been distributed to some 200 users
throughout the country, operates on UNIX computers and high-end graphics workstations, provides new network access to remote data bases, and has developed new hardware interfaces for image display hardware. In addition to NASA-compatible terminals, NOAO provides 47
technical onsite consultation to NASA scientists, sponsor seminars and conferences on IRAF, and assists NASA in evaluating relevant new technology. This work directly supports the
NASA space science astrophysics community, including the Space Telescope Science Institute. NASA SOI/MDI Project
NSO staff working on the Solar Oscillations Imager - Michelson Doppler Imager will focus on the instrument design, data acquisition systems, data reduction processes and systems, and related ground support equipment. Collaboration between this project and the GONG project will significantly enhance the scientific return of both programs. At the project level, the areas of such a collaboration include sharing experience and facilities in the doppler imager development, sharing the development of common computer software and hardware, the joint use of these computing systems where deemed appropriate, and the coordination of the observations programs during the time that the two experiments are operational simultaneously. NASA Vacuum Telescope Support
NSO has provided the solar physics community with full-disk, high resolution magnetograms and He 10830 spectroheliograms for a number of years using the Vacuum Telescope for synoptic observations. Since 1979, NASA (a primary user of this data) has been providing funding to assist in the operational support and improvement of the telescope. NASA Project Galileo
M. Belton is continuing his work in Project Galileo as the team leader for the Solid State Imaging System. Funding will be used to support travel to team and project meetings, the cost of consultants to the team, and the development of a "Home Institution Image Processing System" (HIJPS) to be installed at the NOAO Tucson offices. NASA RMT - MIT/ETC Projects
B. Teegarden of NASA, in collaboration with G. Ricker of Massachusetts Institute of Technology (MIT), is operating the Rapidly Moving Telescope (RMT) and the Explosive Transient Camera (ETC) on Kitt Peak. NASA funding is provided to refurbish facilities and for support provided by KPNO operations personnel. NASA Infrared Astronomy Satellite (IRAS)
F. Gillett is working with scientists at the Lowell Observatory to obtain a FITS tape of the NGC 6822 infrared maps, obtain H-alpha images of the galaxy, make far-infrared color maps from the IRAS data, and then compare the spatial distribution of the H-alpha emission with that of the far-infrared in order to separate the component of the dust heated by star formation from that heated by the general interstellar radiation field. NASA Tuneable Wide Field Lyot Filter
R. Dunn and R. Smartt are principal investigators of this continuing project for the design and fabrication of a tuneable wide field Lyot filter. 48
USAF Upgrade Coronagraph
The USAF is funding the provision of a dedicated light feed for the coronal photometer at the Evans Solar Facility as well as to up-grade the multiband polarimeter for flare patrol observations. Both projects are in support of the Max '91 campaign of coordinated activity measurements being conducted by the USAF Solar Research Branch.
USAF Solar Mass Ejection Imager Funds have been received from the USAF under a subcontract from the University of California, San Diego, for NSO staff to conduct studies of the design of a space-bome instrument to image disturbances in the interplanetary medium. USAF Fabry Perot Filter
USAF has funded NSO support of AFGL data analysis for the Solar Research Branch, including a video imaging capability and hardcopy of computer processed images. This work is conducted at the NSO's Sacramento Peak Observatory in Sunspot. Other Projects include: NASA FTS Program for Upper Atmospheric Research
J. Brault is participating in this project as principal investigator. The primary activities are upper atmospheric studies utilizing the FTS at the McMath Telescope.
USAF/ Casting & Preparing to Polish a 3.5-m Borosilicate Honeycomb Mirror UofA
NOAO administers a subcontract between the USAF and the University of Arizona Mirror Lab which requires the UofA to cast a 3.5-m borosilicate honeycomb mirror blank and to design, develop, and construct polishing facilities that are being used to finish the blank. USAF
monitors the technical work on the project, with all work being completed by the UofA. NASA Stellar Winds in Hot Stars
P. Massey of KPNO is continuing this study begun several years ago to extend the knowledge of stellar winds to the hot stars in M31 and M33 identified by optical photometry and spectroscopy. His observations are made at NASA's IUE Observatory. USAF Video Imaging System
The Air Force continues to provide funds for a Narrowband Filter System and work on a Video Imaging/Display System. USAF Upgrade Polarimeter
The Air Force continues to provide funds to upgrade the Multiband Polarimeter for flare patrol observations.
49
NOAA Support for J. Brault
NOAA is supporting the work of J. Brault of NSO in applying Fourier techniques to optimize current A.L. nonlinear least squares data analyses software, to develop tropospheric trace gas
spectroscopy experiment for support of OH gas experiment, and to participate in the analysis of OH data.
NASA SOT Support for J. Harvey
NASA continues to support the work of J. Harvey on the Orbiting Solar Laboratory Project as a facility scientist investigating the dynamics of solar magnetic fields. NASA Chromospheric Emissions
M. Giampapa of NSO is making observations at NASA's IUE Observatory in order to yield further insights on the nature of chromospheric and coronal heating in the ordinary, inactive dM stars. The results to be obtained in this program will yield critical observational constraints on the possible mechanisms for atmospheric heating in the dM stars. NASA Photometry of Halley
M. Belton of KPNO is continuing his study of Comet Halley to (1) obtain an accurate, well
sampled, photometric time-series of the comet which tracks the pre/post-perihelion asymmetry in the light curve, covers the final decay of the coma, and which covers a substantial portion of the light curve at a time when the cometary light is dominated by the reflection of sunlight from the nucleus itself; (2) derive a precise ephemeris for the nuclear spin; (3) separate the effects of rotation in the light curve from the effects of changes in the average rate of sublimation; (4) determine astrometric positions for the comet.
OSD/SDI Interferometric Imaging
C. Roddier of NOAO and F. Roddier of the University of Hawaii are performing research to
demonstrate that image reconstruction through turbulence is feasible both in visible and infrared without a reference source by combining pupil-plane interferometry with bi-spectral analysis. NASA CO Synoptic Study
NASA continues to support the observations of integrated sunlight, relevant to a NASAsponsored investigation of the spectroscopic detectability of extra-solar planetary systems. NASA X-Ray Luminosity Functions
A. Porter of NOAO is measuring the X-ray luminosities and upper limits of 80 clusters of galaxies which lie within long exposure IPC fields, and will use the results to study the X-ra> luminosity function at high redshift, looking for evolution in its slope since lookback times of about five billion years. 50
APPENDIX 4
NATIONAL OPTICAL ASTRONOMY OBSERVATORIES
USER STATISTICS1 FY 1989
VISITOR TELESCOPE USAGE
Visiting Observers
cno2 U.S. Foreign
KPNO3 U.S. Foreign
NSO4
U.S.
NOAO TOTALS
Foreign
U.S.
Foreign
Toial
109
40
332
43
222
61
663
144
807
Graduate Students
22
3
110
8
15
6
147
17
164
Other (technicians, research assistants, etc.)
3
3
23
6
11
3
37
12
49
134
46
455
57
248
70
847
173
1020
54
24
99
36
47
28
200
66
266
Astronomers
Total Visitors Institutions
1 The figures in these tables reflect the number of observeiVusers physically present at the Observatory and also include multiple visits by a single observer/user. These tables do not include NOAO staff.
2 During fiscal year 1989, a total of 222 observing programs were carried out by visitors and the NOAO staff at Cerro Tololo. Visiting astronomers were assigned 74% of the scheduled telescope time and the remaining 26% was assigned to the staff.
3 During fiscal year 1989, a total of 318 observing programs were carried out by visitors and the NOAO staff at Kitt Peak. Visiting astronomers were assigned 80% of the scheduled telescope time and the remaining 20% was assigned to the staff.
4 During fiscal year 1989, a total of 151 observing programs were carried out by visitors and the NOAO staff at the National Solar Observatory. Visiting astronomers were assigned 68% of the scheduled telescope time and the remaining 32% was assigned to the staff.
VISITOR REDUCTION FACILITIES USAGE NOAO - Tucson
Visiting Scientists
Number of Institutions
VAX Computer Systems Grant Comparator - 2 axis PDS Microdensitometer
100 8
3
Ph.D.
Student
Other
Totaf
263
213
36
14
12
5
11
28
33
77
24
20
*The numbers reflected above show duplicated usage of NOAO-Tucson reduction facilities by visiting scientists. NOAO staff are not included in these figures.
NATIONAL OPTICAL ASTRONOMY OBSERVATORIES
APPENDIX
5
FY-1990 Program Plan - Revision I June 1, 1990 TABLE
I
FUNDING BY SOURCE
(Amounts in Thousands)
Scientific Staff & InstruOperations & Support mentation Maintenance NSF
Management
Fee
TOTAL
FY-1990Q)
TOTAL
TO
FY-1989
FY-
FUNDING
Advanced Development Program
$
Cerro Toloto Inter-American
Observatory
Kitt Peak National Observatory
1,256
470
3,510
5,236
4,905
4
1,913
1,485
4,507
7,905
7,519
7
1,737
2,486
2,525
2
National Solar Observatory Sunspot USAF Support
489
Tucson
685
260
211
NASA Support
Global Oscillations Network Group
1,343
60
52
21
235
(600)
1,378
1
(69)
(63)
1,500
1,538
1
841
1,916
1
273
385
196
178
178
182
1,350 1,146
1,350 1,146 1,200
1,156 1,229 1.256
841
Publications & Info. Resources Central Administrative Services
Central Facilities Operations Central Computer Services
(600)
1,500
Telescope Technology Program Central Offices Director's Office
(600) 447 (69)
944
1 1 1
Central Engineering & Technical Services
801
Management Fee
Total NSF Funding NON-NSF
$4.424
$5,054
$14.224
FUNDING
Total Funding
801
646
407
407
405
407
124,109
$24,188
$23,
2,573
3.411
1,
$26,682
$27,599
$24,
467.10
461.81
461
6.75
6.75
9
473.85
468.56
471
STAFFING SCHEDULE
(In Full Time Equivalents) NSF Funded Non-NSF
Funded
Total
(1) (2)
64.00
81.15
321.95
Includes $23,800K new funds, $50K new REU funds, and $259K carryover. Where possible, comparative amounts for ADP have been redistributed to reflect current organization.
TABLE
1-A
ADDENDUM TO FUNDING BY SOURCE TABLE
(Amounts in Thousands)
NSF Funding
Director's Office - Operations & Maintenance
Office of the Director
FY-1990
FY-•1989
$
$
Visiting Committee Travel
Collaborative Projects Indirect Cost and Miscellaneous Credits
$
321
41
4
3
1
2
273
(251)
(469)
22
S
366
15
(177)
Visitor Program-Foreign Travel Total
410
FY •1988
20
16
$
(45)
$
96
TABLE I-B ADDENDUM TO
FUNDING BY SOURCE TABLE
(Amounts in Thousands)
Research Experience for Undergraduates (REU) Program Amounts shown are included in Scientific Staff & Support: Estimated
Kitt Peak National Observatory
Carryover
New
Funds
Funds
Total Funds
$ 18
$ 18
18 4
18 6
4
5
5
1
$
Number of Students
National Solar Observatory Sunspot Tucson
2
Central Computer Services
NOAO Director's Office (unallocated) Total £
2. 4
5
7
$ 50
$ 54
2
TABLE
II
SUMMARY OF NSF FUNDING BY COST CATEGORY (Anounts in Thousands)
NSO
Personnel Costs
Supplies ft Materials Utilities ft Communications Purchased Services Domestic Travel
Foreign Travel Equipment
CTIO
KPNO
SUNSPOT
TUCSON
$3,245 1,073
$6,108 1,025
$1,792
$1,084
297
176
307 298 41 107
287 44
256 71
136 50
21 5
165
255
44
6
GONG
TTP
940 84
548
10
50
18
54
48
10 6
378
44
$
215
13
Management Fee
USAF ft NASA Support Total NSF Funding
(600)
$5.236
$7,905
$1.886
CENTRAL
TOTAL
OFFICES
FY-1990
$3,477 449 345 512 65 44 168 407
i69> $1.274
$17,194 3,319 1,195 1,003 375 225
1,060 407
(669)
$1,500
$
841
$5.467
$24,109
6.25
63.00
13.95 10.10
69.00 32.10 75.50 130.60
STAFFING SCHEDULE
(In Full Time Equivalents) Scientists
16.00
26.25
5.00
9.50
16.00
Engineers & Scientific 1.00
9.00
10.00
17.55 7.00
6.00
Administrators ft Supervisors
3.00
1.00
Clerical Workers Technicians Maintenance ft Service
26.00 38.50
9.45 47.40
4.10 13.00
1.00 2.00 6.50
9.00
1.00 6.00
32.95 10.20 14.00
96.90
20.00
19.00
12.50
87.45
467.10
Programmers
Workers
Total
43.00
30.00
9.90
149.50
137.65
41.00
5.50
TABLE
III
SCIENTIFIC STAFF ft SUPPORT
(Aaounts in Thousands)
NSO CTIO
Personnel Costs
$1,116
KPNO
,637
TUCSON
Supplies ft Materials
35
93
453 12
Purchased Services Domestic Travel
24 4
31 66
14
2 21
Foreign Travel Equipment
55 22
39
5
10
47
Total
$1,256
$1
SUNSPOT
$1
,913
$
5
$ 489
$
615 37
$ 685
CENTRAL
TOTAL
TOTAL
OFFICES
FY-1990
FY- 1989
FY-
$3,895
$3 ,625 90
$3
$
74
177 2 5
$
110
72 87
109 69
41
64
TO
57
81
$4,424
$3 ,972
$4
5
6
STAFFING SCHEDULE
(In Full Time Equivalents) Scientists Clerical Workers Technicians Total
15.00 1.00
24.75 2.00
5.00 1.50
8.50 1.00
1.75
55.00 5.50 3.50
53.95 5.50 3.50
26.75
6.50
9.50
1.75
64.00
62.95
3.50 19.50
TABLE IV
INSTRUMENTATION
(Aaounts in Thousands)
NSO
Personnel Costs
Supplies ft Materials Purchased Services Domestic Travel
Foreign Travel Equipment Total
CTIO
KPNO
$303 126 22
$1,211 219
CENTRAL
TOTAL
SUNSPOT
TUCSON
GONG
TTP
OFFICES
FY-1990
FY-1
$222 26
$129 82
940
548 215
$ 150
$3,503
12 50
$3, 1, 1,
84
TOT
18
9
50 48
19
6 70
378
44
75
764 122 67 12 586
$470
$1.485
841
$ 287
$5,054
$6.
1.00
1.00
1
1.50
32.05 1.00 2.00 45.10
29 1 2 48
2.50
81.15
81.
(30)
12
10 6
$260
$211
$1.500
$
STAFFING SCHEDULE
(In Full Time Equivalents) Scientists
Engineers ft Scientific Programmers
5.00
9.05
1.00
1.00
9.00 1.00
1.00 7.00
17.60
4^00
1.50
9.00
1.00 6.00
13.00
26.65
5.00
2.50
19.00
12.50
Administrators ft Supervisors Clerical Workers Technicians Total
5.50
TABLE V
OPERATIONS ft MAINTENANCE BY COST CATEGORY
(Anounts in Thousands)
NSO
CT10
KPNO
SUNSPOT
TUCSON
CENTRAL
TOTAL
OFFICES
FY-1990
TOTAL FY-1989
$ 9,796 2,378 1,195
$ 8.974 2.413 1,246
$1,826
$3,260
$1,117
$3,253
Supplies ft Materials
912
713
259
437
Utilities ft Communications Purchased Services Domestic Travel
307 252 37
287 43 61
256 54 7
345 460
Personnel Costs
Foreign Travel
Equipment USAF ft NASA Support Total
52
5
124
138
$3.510
$4.507
60 44
44 (600)
93
$4,692
$1.137
817
188
198 104
167 106
405
811
(669)
(663)
$14,224
$13.242
STAFFING SCHEDULE
(In Full Time Equivalents) Scientists
1.00
1.50
Programmers Administrators ft Supervisors
11.00 10.00
8.50 7.00
5.00 3.00
Clerical Workers Technicians
24.00 28.00
7.45 29.80
9.00
1.00
3.50
7.00
6.30
1.00
12.45 10.10
36.95 31.10
1.00 5.00
32.95 10.20
68.00 82.00
38.00 31.00 66.81 78.60
14.00
96.90
96.90
8.00
83.20
321.95
317.61
Engineers ft Scientific
2.60
Maintenance & Service
Workers
43.00
30.00
9.90
Total
117.00
84.25
29.50
F
$
$
TABLE VI
OPERATIONS ft MAINTENANCE BY TYPE OF SERVICE (Anounts in Thousands)
MSIl>
CTIO
KPNO
678
$1,180
Telescope Operations
646
Mountain Operations
SUNSPOT
TUCSON
ItNIKAL
TOTAL
TOTAL
OFFICES
FY-1990
FY-1989
$ 2,906
$ 3.116
2.296
2.303
3,326
3,026
1,146
1.985
2,078
944
944
710
1,623
3,258
178
178
182
(669)
(663)
Engineering ft Technical Services
$
$
219
$ 28
745
667
238
750
1.927
649
583
256
$
801
Central Facilities - Tucson/
La Serena Operations Central Computer Services Administration
853
399
202
181
2,490
Publications ft Information Resources
(600)
USAF ft NASA Support Total O&M
$3.510
$4,507
$ri37
(69) $378
$4.692
$14.224
$13.242
13.85
51.85 59.00
18.50
47.55 13.55
STAFFING SCHEDULE
(In Full Time Equivalents) Engineering ft Technical 14.00
20.00
4 .00
Telescope Operations Mountain Operations
25.00 31.00
18.00 36.20
10 .00 11 .50
Facilities
24.00
5.05
23.00
5.00
4 .00
2.00
37.30
71.30
45.50 58.50 78.20 49.55 15.85 70.01
117.00
84.25
29.50
8.00
83.20
321.95
317.61
Services
6.00
78.70
Central Computer Services Administration Total
13.55
TABLE VII NON-NSF
FUNDING
(Anounts in Thousands)
NSO
CTIO
Personnel Costs
$
KPNO
$
Supplies ft Materials Utilities ft Communications
$
171
$
130
CENTRAL
TOTAL
TOTAL
OFFICES
FY-1990
FY-1989
$
241
139 5 43
Equipment $_
$_
432
$
363
16
242 4
88
782
148 9
125 6
1,194
2,782
58
29 144
271
,424
$
3
2
25
7
9 346
322
$_ 395
$2,573
$3,411
.50
1.50
2.00
.50
2.25
1.75
3.00
3.00
1.00
6.75
6.75
4
$1
720
6
43
Foreign Travel
$
200
4
Purchased Services Domestic Travel
Total
178 20
TUCSON
SUNSPOT
STAFFING SCHEDULE
(In Full Time Equivalents) Scientists
1.00
Engineers ft Scientific Programmers Clerical Workers Technicians Total
1.00
.75
1.00
1.00
3.00
1.75
1.00
1.00
F
