Project Structure
Project Budget and Schedule
Project ASTEROID has been structured to ensure completion
at the earliest possible date using a conservative engineering
and contracting approach.
Early in the Construction Phase, the Project will
require the selected telescope and imager vendors to
present a Design Review showing how the telescope conforms
to the Functional and Performance Requirements Document
and the Operations Concept Definition Document. They will
also present detailed management plans showing budgets and
schedules for completion of the project.
The major budget items are given below for three funding
options whose performance we have studied. Option 1 is a 1.5-m
telescope located at the current Winer Observatory
Sonoita Field Station. Option 2 is a 1.5-m telescope located
at a new site with better seeing, darker skies, and higher
elevation. Option 3, the baseline to which we are working,
is a 2.5-m telescope also located at a new, better site.
The project schedule is as follows:
| Schedule Item |
Year |
Option 1 |
Option 2 |
Option 3 |
| |
|
(1.5-m Sonoita) |
(1.5-m Mtn) |
(2.5-m Mtn) |
| Fundraising
| 0
| n/a |
n/a |
n/a |
| Design Phase
| 1
| $ 500,000
| $ 700,000
| $ 700,000
|
| Construction Phase - Year 1
| 2
| 1,000,000
| 1,500,000
| 2,500,000
|
| Construction Phase - Year 2
| 3
| 1,500,000
| 1,500,000
| 3,000,000
|
| Construction Phase - Year 3
| 4
| 1,500,000
| 2,500,000
| 3,300,000
|
| Construction Phase - Year 4
| 5
| 1,000,000
| 1,800,000
| 3,500,000
|
| Construction Phase - Year 5
| 6
| 250,000
| 1,000,000
| 1,500,000
|
| Commissioning Phase
| 7
| 250,000
| 1,000,000
| 1,500,000
|
| |
Totals
| $6,000,000
| $10,000,000
| $18,000,000
|
 
The budgets for the major subsystems are as follows:
| Budget Item |
Option 1 |
Option 2 |
Option 3 |
| |
(1.5-m Sonoita) |
(1.5-m Mtn) |
(2.5-m Mtn) |
| Telescope with control system
| $3,000,000
| $ 3,000,000
| $ 6,000,000
|
| Imager, readout electronics, filter wheel, and control system
| 2,500,000
| 2,500,000
| 5,500,000
|
| Study Phase, site modifications and infrastructure enhancements
| 500,000
| 4,500,000
| 6,500,000
|
| Total
| $6,000,000
| $10,000,000
| $18,000,000
|
The third budget item includes the funds needed for
the optical designer, systems engineering that cannot be
performed by the Project Scientist, and other contract
staff not provided by either Winer staff or by the telescope
or imager vendors. The prices are based on:
Telescope:
- Discussions with DFM Engineering, Astronomical Consultants
& Equipment, and EOS Technologies, all vendors of telescopes
of these sizes.
- The price quoted by DFM Engineering for the 1.3-m f/4
1.7-degree USNO telescope.
Imager:
- Discussions with NOAO CCD experts on the cost of detectors
and of mounting them into Dewars.
- Preliminary discussions with Spectral Instruments on the
prices for an imager; this appears to be an area of considerable
price risk, depending on how large an area is covered by the
optical design and whether we include detectors for wavefront
sensing for guiding and focus.
- Comparison with other one-degree imagers. For example, the
One-Degree Imager (ODI) for the WIYN 3.5-m telescope on Kitt
Peak was initially estimated to cost approximately $6.5 million.
This project is now in the construction phase. The Dark Energy
Camera (DECam) being built by the Department of Energy for the
CTIO 4-meter Blanco telescope is estimated to cost approximately
$20 million (including DOE overhead and G&A). We have made some
cost-saving assumptions, such as sacrificing the ultraviolet
and using a conceptual design spanning 360 to 1000 nm instead
of spanning the entire Sloan spectrum of 280 to 1123 nm. This
permits us to use less expensive glass and an all-spherical
design. Furthermore, most large-format imagers use an array of
many (e.g., 60 or more) 2k x 4k CCDs (each of which costs
$80,000). Instead, we assumed in our budget that for the
1.5-m telescope, we would use a single 10600 x 10600 pixel
monolithic detector that costs approximately $150,000 to
cover the greater part of one degree. For the 2.5-m
telescope, we assumed we would use a mosaic of these. These
assumptions greatly reduced the estimated cost of the imager
in the budget projections.
Design Study and Infrastructure:
- Estimate of $75,000 for optical design, $50,000 for systems
engineering, and other engineering study costs for a total Design
Study phase cost of $300,000
- Infrastructure upgrade costs for the 1.5-m telescope located
at the Winer Observatory Sonoita Field Station include
allowances for replacing the current rail/wheel system with
I-beams and castors with custom trucks, raising the roll-off
roof by an appropriate amount to clear the new telescope, and
extending the I-beams to permit the roof to roll far enough north
for all telescopes under the roof to see Polaris. The last item
would permit the installation of a Differential Image Motion
Monitor (DIMM) to obtain continuous seeing measurements in a form
recognized by most astronomers as an accurate representation of
the local seeing. The infrastructure upgrades also include a
higher bandwidth Internet system to send the images from the
observatory to the data reduction specialist's office in Tucson
for analysis.
- Infrastructure upgrade costs for Options 2 and 3 assume
moving to a higher elevation site with better seeing, and building
a new enclosure and site infrastructure, including a road, Internet,
self-sustaining electrical power generation, and other items needed
in a very remote area. If we locate at an existing site, funds not
spent on infrastructure directly will be spent on "buy-in" fees
and other infrastructure charges assessed by the site owner, so the
budget is the same either way.
 
Last modified: October 21, 2008.