NOTE: This is just for reference purpose to illustrate the amount of
work involved in writing the proposal. The amateur program has since been
discontinued....sorry
AMATEUR PROPOSAL TO USE
HUBBLE SPACE TELESCOPE
Overview
All amateur proposals to use the Hubble Space Telescope (HST) must
describe a self-contained and well defined scientific program, and must
include a discussion of the methods for obtaining and analyzing data in
order to achieve the scientific goals of the project. The principal
investigator (PI) will be expected to understand the goal(s) of his or
her proposal and to publish the results in the scientific literature.
This program is open to all United States citizens and legal residents
who do not have an advanced degree in astronomy.
Amateur proposals will be judged largely on the basis of scientific
merit, by the method of peer review, by members of the Amateur
Astronomers Working Group (AAWG). This committee of leading U.S.
amateur astronomers consists of representatives of the American
Association of Variable Star Observers (AAVSO), the Association of
Lunar and Planetary Observers (ALPO), Astronomical League (AL),
International Amateur Professional Photoelectric Photometry (IAPPP),
International Occultation Timing Association (IOTA), and jointly the
Corporation for Research Amateur Astronomy and Western Amateur
Astronomers (WAA). After screening by the AAWG, a small group of
finalist recommendations will be sent to the Space Telescope Science
Institute (STScI) for technical feasibility studies, after which those
to observe with HST will be selected. Amateurs receiving time on HST
will be invited to STScI to fine tune their instrument configurations
and operating modes in order to achieve the most meaningful results;
they will also have some support of STScI in the analysis of their
data.
The original news release from NASA and STScI points out that "a few
hours of observing time" has been reserved for amateur astronomers by
the director of STScI. Dr. Riccardo Giacconi, the original director,
further stated that he expected amateurs "to ask refreshingly new
questions." Amateur proposals duplicating proposals already submitted
by professional astronomers will not be considered unless the amateur
has contributed a unique and creative aspect to the observation. It
should be emphasized that duplication of observation will be the
exception rather than the rule.
Information from your proposal will be entered in a database at STScI
to estimate the resources required by the program (e.g. spacecraft
time, data volume, real-time requirements) and to test for duplication
with both Guaranteed Time Observers (GTOs) and General Observers (GOs).
In order to give more amateurs time on the HST, total observing time
will be of prime importance. However, an original, creative proposal
may justify much of the allotted time if it offers a real contribution
to the advancement of astronomy.
Keep in mind that the AAWG attempts to involve as many amateurs in this
program as "time" allows. Just how much time amateurs will be given
will depend on how unique and creative your ideas are. At minimum,
proposals should emphasize the use of HST's special capabilities: its
high angular resolution, extended spectral range, and superior
sensitivity. Only research proposals that cannot be done from the
ground will be considered.
In order for the AAWG to properly evaluate your proposal, you will need
to provide the following information. We recommend you keep photocopies
of all material submitted to the AAWG.
To be considered for Cycle 95, YOUR PROPOSAL PACKAGE (THE ORIGINAL
PLUS
SIX COPIES, ALL ON PAPER) MUST BE POSTMARKED BY 30 APRIL 1995 and
sent
to:
The Astronomical League
Rt. 2, Box 940
Barltesville, OK, 74006
USA
Questions should be sent to this address as well, not to the
Space Telescope Science Institute.
To meet the qualifications for this program you must:
- Be a U.S. citizen or legal resident of the United States.
- Not have, or be currently receiving, a MS or PhD degree in
astronomy or astrophysics.
- Not be employed at a facility involved in professional research in
astronomy or astrophysics.
- Not derive the majority of your income from astronomy or
astrophysics (teaching or research).
The AAWG reserves the right to determine the eligibility of any
proposer.
Amateur astronomers not meeting qualification (1) should contact the
headquarters of the European Space Agency regarding any parallel
program they may have instituted.
Outline
- 1. Title
- Title the proposal such that it contains Keywords. (See
attached list of keywords) The keywords will be used during computer
searches to determine the technical feasibility of your proposal.
- 2. Objective
- Specific scientific goals of your project. What do you
hope to learn from your observation(s)? Why is it important? What do
you base this information on?
- 3. Literature Search
- Bibliography of literature references relating to
your subject and target. Your references should deal with what is known
about your target, what has already been done from ground-based
observatories, and if there are plans for future studies by the
author(s).
Photocopies of one to three of your most recent literature
references, which cannot be returned, should be included with your
detailed proposal.
- 4. Technical Feasibility
- Why is the HST necessary to collect data? Why
can't the observation be made with ground-based telescopes? How do
resolution, magnitude, and specific wavelengths of light influence your
observations?
- 5. Collection of Data with HST
- How do you propose to use HST to
collect the necessary data to complete your observation(s)? Use the
enclosures provided with this packet of material [available only in
hardcopy from HST, AAVSO, 25 Birch St., Cambridge, MA 02138, USA] to
determine scientific instrument (SI) capabilities. (More detailed HST
instrument handbook which pertain to your specific proposal may be
found in university libraries).
- 5.1 Target Name:
-
- The maximum allowable length of a target name is 30 characters and
only upper-case characters should be used.
- No blanks are permitted in target names. Blanks between letters and
numerals should be suppressed (e.g. HD140283, NGC4378), but a hyphen
should replace blanks between two letters or two numerals (e.g.
ALPHA-CEN, NGC224-0040+4058), and should also be used where required
for clarity (e.g. NGC4468-POS 1).
- Only letters and numerals are allowed in target names; punctuation
(other than hyphens and + or -) is not permitted (e.g. BARNARDS-STAR,
not BARNARD'S-STAR). Greek letters should be spelled out (e.g.
ALPHA-BOO, ARCTURUS, ANDROMEDA-GALAXY, ORION-NEB).
- 5.2 Target Position
- A position must be specified for each fixed target. If the target is
not fixed, such as a solar system object or star with large proper
motion, the name of the planet, asteroid, or star with proper motion
will suffice. For fixed targets there are three options: (1) specify
the celestial coordinates (right ascension, declination). Be sure to
specify the epoch (e.g. 1950, 2000, etc.) for the celestial coordinates
you use; (2) specify a positional offset from another target; or (3)
specify an area of the sky. When using right ascension (RA) and
declination (dec) you must include their uncertainties, using the
format RA=+/- or the source of the position.
Include proper motion values if available. A suggested source for fixed
targets is Volumes 1 & 2 of the Sky Catalogue 2000.0 by Alan Hirshfield
and Roger W. Sinnott available from Sky Publishing Corp., P.O. Box
9111, Belmont, MA 02178-9111.
- 6. Primary Observations
- Since all of the science instruments (SIs) are permanently mounted at
the telescope focal plane, it will routinely be possible to operate two
(or more) SI's simultaneously, thereby increasing the scientific
productivity of the HST. Primary observations are defined as those that
determine the telescope pointing. They will always have priority over
parallel observations made with the second SI.
Most primary observations will be scheduled at times that will
provide maximum efficiency. However, special considerations regarding
scheduling and execution of observations may come into play under the
circumstances described in the next two sections.
- 6.1 Time-critical Observations
- Time-critical observations are observations that require a specific
time or date, or within a range of specific dates. Time critical events
that occur over time intervals short compared to the orbital period of
HST (such as occultations or eclipses of very short-period binary
stars) introduce an additional complication because it will not be
known, until a few weeks in advance, where the HST will be in its orbit
at the time of the event, and hence whether it will occur above or
below the spacecraft's horizon. As a result, critical observations
should be avoided if possible.
- 6.2 Real-time Observations
- Real-time observations will be made for the following purposes:
- Interactive target acquisitions, either with the same SI to be used
for the scientific observations, or with a camera followed by an offset
to the required SI.
- Real-time evaluations and reconfiguration. In this case the amateur
will examine the incoming data form the standpoint of its utility in
relation to the SI modes, filters, gratings, etc., in real time, within
a preplanned set of options.
Availability of the Tracking and Data Relay Satellite System (TDRSS)
limits real-time interactions to about 20% of HST observations. Hence,
real-time interactions will be a limited resource, and the scientific
and operations justification for such interactions must be clearly
presented by the amateur.
- 6.3 Parallel Observations
- Parallel observations are observations made with a second SI while
another SI is carrying out a primary observation. However, the
instruments are positioned so that they cannot look at the same point
source at the same time. Use the field diagram in Figure 6 of the
enclosed Chaisson-Villard article, or Figure 11-1, page 14, of the
enclosed excerpt from the professional "Call for Proposals" to
determine if your target would lie in the field of view of another SI
(WF/PC2, FOC, FOS, GHRS, FGS).
- 6.4 Science Instruments on HST
- Science Instrument (SI) Description
WF/PC2 Wide Field Planetary Camera 2
FOC Faint Object Camera (f/48, f/96)
FOS Faint Object Spectrograph
GHRS Goddard High Resolution Spectrograph
FGS Fine Guidance System
COSTAR Corrective Optics Space Telescope Axial
Replacement
- 6.5 Archival Research
- The scientific data collected by the HST will be
archived at STScI so that they will be available for scientific
research by any interested scientist. The amateur is encouraged to use
this mode of research since it does not require any telescope time and
could offer an excellent opportunity for scientific research. A
separate Call for Archival Proposals will be issued by the STScI at
some time in the future.
- 7. Completed Proposal
- Seven complete paper copies of the proposal,
including two 4" x 9.5" (or larger) self-addressed stamped envelopes,
must be postmarked by April 30, 1995 and sent to:
HST Proposal
Astronomical League Rt 2
Box 940
Bartlesville, OK 74006
USA
Note: Questions about the proposal process, the HST observatory, or its
scientific instruments should be directed to the AAWG via the
Astronomical League, not to STScI.
Proposal package cover page follows:
HUBBLE SPACE TELESCOPE AMATEUR ASTRONOMERS WORKING GROUP
PROPOSAL FOR
HUBBLE SPACE TELESCOPE OBSERVATIONS
Seven complete paper copies of this package, including two 4" x 9 1/2"
(or larger) self-addressed stamped envelopes, must be postmarked by
April 30, 1995 and sent to:
HST Proposal
Astronomical League
Rt 2, Box
940, Bartlesville, OK 74006
USA
- Proposal Title:
- Principal Investigator (PI):
- Address: e-mail:
- City: State: Zip Code:
- Telephone: day ( ) night ( ) FAX ( )
- Co-investigator: Telephone: ( )
- Scientific Category: (Select One)
____Solar System
____Variable Stars (including novae & supernovae)
____Interstellar Medium
____Stellar Astrophysics
____Stellar Populations
____Galaxies and Clusters of Galaxies
____Quasars and Active Galactic Nuclei
____Other (describe nature and characteristics of object below)
- Abstract (please confine to this space)
- Scientific Keywords:
- Estimated observing time: hours (primary)
- Number of targets: (primary) (parallel)
- Circle instrument(s) requested: WF/PC-2 FOC FOS GHRS FGS
- Special scheduling requests:
____Real-time observation
____Uninterrupted long exposure
____Time-critical observations
____Special orientations
- Signed Date
The AAWG reserves the right to determine the eligibility of any
proposer.
Instructions for Completing the Proposal Cover Page
- Item 1
- Give a concise title for your proposal using key words (see
attached list).
- Item 2
- Name of the principal investigator (PI).
- Item 3
- Address of the PI. If available, include e-mail address.
- Item 4
- City, State, using two letter postal designation (e.g.
California-CA, Oklahoma-OK, etc.) and zip code.
- Item 5
- Provide both day and night telephone numbers of the PI.
- Item 6
- Name and telephone of co-investigator, if any. Additional
co-investigators and their telephone numbers may be listed on the
reverse of the cover page.
- Item 7
- Select the most appropriate scientific category for your
proposal from those listed.
- Item 8
- Provide a concise abstract for the proposed observations.
Include WHAT, WHY, and HOW for the main scientific goals and justify
the necessity of the HST time. This is only an abstract; your detailed
proposal should be typewritten on the appropriate form included with
this package and returned with this proposal form.
- Item 9
- Provide the most appropriate scientific key words to describe
your project in order of priority (see attached list of key words).
- Item 10
- Give the total observing time (hours) requested for primary
and/or parallel observations. For long-term projects, give the total
time requested for the full duration of the project. It is understood
the amateur may not have sufficient information to determine realistic
exposure and observing times.
- Item 11
- Give the total number of primary and/or parallel targets
requested.
- Item 12
- Circle the instrument(s) which will be used in your project.
- Item 13
- List special constraints relevant to your observations.
(Real-time observations require real-time contact with HST.
Time-critical observations are those that must be made at a definite
absolute time, or at a definite time interval before or after another
exposure. Special orientations of the telescope are considered as time
critical observations.)
- Item 14
- Sign and date your proposal form.
You must send seven copies of your proposal to
HST Proposal
Astronomical League
Rt 2, Box 940
Bartlesville, OK 74006
USA
OUESTIONS
Please answer the following questions on separate sheets of paper and,
if possible, use a word processor (Font = Times, Size = 12), double
spacing (20). State the question as shown below before typing a
response to each.
- Explain in detail WHAT you are proposing to study and the
significance of the investigation to the field of astronomy.
- What are the specific details of the targets to be studied and the
HST instruments and their models to be used? Explain HOW the data from
the instrument/mode are required for your investigation. Provide a
table with columns as follows: Target Name/ID, Target position,
Magnitude (include the wavelength, e.g. B, V, etc), Instrument Mode,
Filter or Spectral Range, Number of exposures needed, Comments. Provide
a separate table listing only the targets you wish to study and the
Exact Positions (Right Ascension and Declination or offset from known
target). Specify the epoch (1950, 2000, e.g.). For solar system
objects, specify the desired observation dates/times and their time
criticality.
- Given HST throughput, motion, and pointing constraints, can you
show
that HST can make the observations your investigation requires? Your
proposal must use appropriate wavelengths and avoid time wasted in
unnecessary or excessive slewing, and objects too near the Earth, Sun,
or Moon. Observations of extremely faint objects, or objects which need
to be observed continuously for longer than a half-orbit will need good
justification.
- Which of HST's unique capabilities are necessary for your
investigation and show WHY your study cannot be made with a groundbased
telescope? [Note: The unique capabilities of the HST are generally
considered to be: (i) low background light and ability to image very
faint background objects; (ii) accessibility of the UV in the region of
1000A; (iii) no atmospheric turbulence.]
- a. What are your plans for analyzing the data you obtain? You can
expect some help from STScI staff where specialized data processing
protocols are available and the answers to technical questions are
required. b. In performing data analysis on your own, in what medium do
you prefer to receive your observations? Hard copy in the form of
tables, graphs, or prints of images? If computer-readable, indicate
computer system you use and the medium of the data; floppy disk (3.5 or
5.25"), tape, CD-ROM, etc. c. What plans do you have to publish your
results? This can include delivered papers, abstracts, or posters.
However, you are expected to publish your results and we need to know
to which journal(s) or other publications (magazines) you will submit
your article. Negative, as will as positive results, contribute to the
science and should be reported
- Supply a bibliography listing relevant scientific publications that
describe your topic. Give the title, author, journal or book, volume
number, page, and year of publication. Supply photocopies of the most
pertinent, and recent articles with your proposal.
BIOGRAPHICAL SKETCH OF HST PROJECT PROPOSER
Name:
Date of Birth: Place of Birth:
Education: Date School, City, State
High School
BS
MS
PhD
Occupation: Current Position:
Brief Career Summary:
Membership(s):
Publications (if any):
Have you submitted a proposal to the AAWG in the past? If so, provide
the date submitted.
Interests
SUGGESTED SOURCES AND LITERATURE REFERENCES
- JOURNALS
- American Journal of Physics (Am. J. Phys.)
- Astronomy and Astrophysics (A & A)
- Astrophysical Journal (Ap. J.)
- Astrophysical Journal Letters (Ap. J. Lett.)
- Icarus
- Nature
- Journal of Geophysical Research (J. Geophys. Res)
- Physical Review (Phys. Rev.)
- Physical Review Letters (Phys. Rev. Lett.)
- Physics Today (Phys. Today)
- Publications of the Astronomical Society of the Pacific (Pub.
A.S.P.)
- Proceeding of the National Academy of Science, U.S. (Proc. Nat.
Acad. Sci. U.S.)
- Science
- MAGAZINES
- Astronomy
- Discover
- Mercury
- Observatory
- Science News
- Scientific American
- Sky and Telescope
- SKY CHARTS AND ATLASES
- William-Bell, Inc., P.O. Box 3125, Richmond, VA 23235
- Kalmbach Publishing Co., P. O. Box 1612, Waukesha, WI 53187
- Sky Publishing Corp., P.O. Box 9111, Belmont, MA 02178-9111
- W. Tirion Sky Atlas 2000.0, Vol 1 (to mag 9.5)
- Uranometria 2000.0, Vol 1 (to mag. 8.0)
- Sky Catalog 2000.0, Vol 1 (to mag. 8.0)
- Sky Catalog 2000.0, Vol 2 (to mag. 8.0)
- GENERAL ASTRONOMY TEXTBOOKS
- George O. Abell, D. Morrison, S.C. Wolff, Exploration of the
Universe, 5th ed., Saunders College Publishing, Philadelphia (1987);
ISBN 0.03-005143-6; Tele. 800-227-TEXT
- George O. Abell, Realm of the Universe, 3rd ed., Saunders College
Publishing, Philadelphia (1984); ISBN 0-03-05804-X; Tele. 800-227-TEXT
- William J. Kaufmann, Universe, W.H. Freeman and Company, N.Y.
(1985); ISBN 0-7167 1673-9; 212-576-9400
- Jay M. Pasachoff, Contemporary Astronomy, 3rd ed., Saunders College
Publishing, Philadelphia (1985); ISBN 0-03-071641-1; 800-227-TEXT
- Jay M. Pasachoff, Astronomy: From the Earth to the Universe, 3rd
ed., Saunders College Publishing, Philadelphia (1986); ISBN
0-03-008114-9
- A.E. Roy & D. Clark, Astronomy: Principles and Practice and
Astronomy: Structure of the Universe, Adam Higler Ltd,. Bristol England
(1982)
- Frank Shu, The Physical Universe, University Science Books, Mill
Valley, CA (1982); ISBN 0-935702-05-9
- Theodore P. Snow, The Dynamic Universe, University Science Books,
Mill Valley, CA (1982); ISBN 0-935702-05-9
- Frank J. Blatt, Principles of Physics, 2nd ed., Allyn & Bacon,
Boston (1986); ISBN 0-205-08555-5
- Gary L. Buckwater and David M. Ribon, College Physics, McGraw-Hill,
N.Y. (1987); ISBN 0-07-052142-52
- Douglas C. Giancoli, Physics: Principles with Applications, 2nd
ed.,
Prentice Hall, Englewood Cliffs, N.J. (1985); ISBN 0-13-672627-5
- Raymond A. Serway and Jerry S. Faughn, College Phyics, Saunders
College Publishing, Philadelphia (1985); ISBN 0-03-062378-2
KEYWORDS
The following is a recommended list of keywords which should be used
for the scientific keywords on your proposal cover page (Item 9). These
keywords are primarily used for archival catalogues and searches. Make
the description as complete and concise as possible. Give any
relationship to parent bodies if relevant. Other keywords than those
listed below can be used if necessary.
- *** SOLAR SYSTEM ***
- Planet name (e.g. Mercury, Venus, Jupiter)
- Satellite of a planet (e.g. Callisto, Titan)
- Moon
- Comet
- Planetary Ring(s)
- Asteroid (e.g. Apollo, Trojan)
- Interplanetary Medium
- Plasma Torus
- Minor Planet
- Feature on planet (e.g. Mons Olympus)
- Zodiacal Light
- *** STARS ***
- Special Type and Luminosity Class
- Star
- Main Sequence Star (MS Star)
- Pre Main Sequence Star (PreMS Star)
- T Tauri Star
- Nebular Variable
- Post main Sequence Star
- Giant
- Supergiant
- Cepheid
- RR Lyr Star
- Long Period Variable
- RV Tauri Star
- R Coronae Borealis Star
- Horizontal Branch Star (HB Star)
- Extragalactic Star
- Chemically Peculiar Star
- Dwarf
- Subdwarf
- White Dwarf
- Brown Dwarf
- Variable
- Irregular Variable
- Regular Variable
- Cataclysmic Variable
- Binary
- Visual Binary
- Eclipsing Binary
- Spectroscopic Binary
- Interacting Binary
- X-ray Star
- Nova
- Recurrent Nova
- Dwarf Nova
- Supernova
- Symbiotic Star
- Neutron Star
- Pulsar
- Black Hole
- Cluster
- Globular Cluster
- Open Cluster
- Association
- POPULATIONS
- Population I
- Population II
- Population III
- *** INTERSTELLAR MEDIUM ***
- Nebula
- Supernova Remnant
- Planetary Nebula
- HII Region
- Bipolar Nebula
- Herbig-Haro Object (HH Object)
- Bok Globule
- Reflection Nebula
- HI Cloud
- Molecular Cloud
- Dark Nebula
- Gas
- Dust
- Extinction
- Cosmic Rays
- *** GALAXIES AND QUASARS ***
- GALAXY TYPE
- Revised Hubble Type: Sec,E5
- Galaxy
- Elliptical Galaxy
- SO Galaxy
- O Spiral Galaxy
- Barred Galaxy
- Irregular Galaxy
- Peculiar Galaxy
- Brightest Galaxy
- Anonymous Galaxy
- Dwarf Galaxy
- Lenticular Galaxy
- ACTIVE GALAXIES
- Active Galactic Nucleus (AGN)
- Seyfert Galaxy
- Radio Galaxy
- Emission Line Galaxy
- Quasar
- BL Lac Object
- GALAXIES IN GROUPS
- Interacting Galaxy
- Binary Galaxy
- Brightest Galaxy
- Galaxy Group
- Local Group
- Nearby Galaxy (z<0.05)
- Distant Galaxy (z>0.2)
- Cluster
- Nearby Galaxy (z<0.2)
- Distant Galaxy (z>0.2)
- Supercluster
- Void
- *** MISCELLANEOUS ***
- SURFACE PHENOMENA
- Surface
- Atmosphere
- Chromosphere
- Corona
- Magnetosphere
- Rotation
- Wind
- Mass Loss
- Accretion
- GALACTIC STRUCTURE
- Jet
- Nucleus
- Halo
- Spiral Arm
- Dust Lane
- Disk
- Bulge
- Region
- Brightest
- Companion
- ASTROPHYSICS
- Formation
- Evolution
- Morphology
- Kinematics
- Dynamics
- Stellar Population
- Luminosity Function
- Mass Function
- Nucleosynthesis
- Abundance
- OBSERVING TECHNIQUE
- Spectroscopy
- Photometry
- Imaging
- Polarimetry
- Occultation
- Lunar occultation
- Planetary occultation
- POSITION AND MOTION
- Astrometry
- Parallaxes
- Proper Motion
- Radial Velocity
- Redshift
- SPECTRAL REGIONS
- Radio
- Millimeter
- Infrared
- Optical
- UV
- X-ray
- Gamma Ray
- RADIATION
- Emission
- Absorption
- Radiation
- Background
- Line
- Profile
- Continuum
- PHYSICAL PROPERTIES
- Luminosity
- Mass
- Rotation
- Temperature
- Density
- Pressure
- Diameter
- Magnetic Field
- LOCATION
- Circumplanetary
- InterpLanetary
- Interstellar
- Circumstellar
- Galactic
- Intergalactic
- Extragalactic
- TYPES
- Early Type
- Late Type
- Type I
- Type II
- Special Sources
- IRAS Source
- Einstein Source
- Unidentified
- Blank Sky
- Calibration
- Offset Star
- Astronomic Reference Star
- Calibration Target