Last Update: 1st August 2017
The National Astronomical Observatory of Japan invites proposals for the Nobeyama 45-m telescope.
The Nobeyama 45-m telescope promotes ground-based observations at centimeter to millimeter wavelengths operated by the National Astronomical Observatory of Japan (NAOJ). In this call for observing proposals, single-beam spectroscopy or continuum observations in 20 - 116 GHz bands and four-beam spectroscopy or continuum observations in 80 - 116 GHz bands are offered.
The following information is about observations with the Nobeyama 45-m telescope.
2600 hours and 300 hours are expected to be available for open-use observations and Guaranteed Time Observations, respectively.
Astronomers and researchers in the related fields (including graduate students) can submit proposals.
Besides, undergraduate students, who are already admitted to graduate schools, can also submit proposals.
We only accept proposals written in English.
Applicants are required to refer carefully to the instruction in this web page, Status Report, and A Guide for Preparation and Submission via Web.
|Semester||Category||Submission Deadline||Observing Period|
|Semester 2017A||Regular Program||Friday 1st September 2017,
|Friday 8th December 2017 --
Wednesday 28th February 2018
|Guaranteed Time Observations|
|Large Program||Friday 8th December 2017 --
Tuesday 15th May 2018
|Semester 2017B||Regular Program||Tuesday 12th December 2017,
|Thursday 1st March 2018 --
Tuesday 15th May 2018
|Guaranteed Time Observations|
|Joint Proposal for the Nobeyama 45-m
Telescope and the ASTE Telescope2
|---||Director's Discretionary Time||Anytime after Submission Deadline
for Each Semester3
|Friday 8th December 2017 --
Tuesday 15th May 2018
It is subdivided into two semesters:
Semester 2017A: 8th December 2017 -- 28th February 2018
Semester 2017B: 1st March 2018 -- 15th May 2018
There are seven observing categories available for the Nobeyama 45-m telescope.
Regular Program is a program requiring the observing time less than 200 hours.
Two deadlines are set for the Regular Program for 2017-2018 observing season.
A Large Program must be based on a strong scientific argument and has a potential of leading to projects with significant impact over 200 hours in total over up to 2 years (over 300 hr proposal will be automatically assigned over two years). The PI should request to obtain data in the period of either 1 or 2 years in the Science Justification part. The observatory may ask the PI to change to 2 years dependent on demand of an LST range.
Short programs are for exploratory observations or follow-up of previous observations. Time request for the short programs is limited up to 20 hours.
Backup Programs are for observations at 20 GHz-band and/or 40 GHz-band that do not require good weather conditions. Backup observations are conducted when high-frequency programs give up observations because of insufficient weather conditions. Backup Programs are available for researchers affiliated with Japanese institutes.
Joint Proposals with the ASTE telescope:
Projects that scientifically benefit by observing at both ASTE and Nobeyama 45-m telescopes are encouraged to submit their proposals to this category.
Guaranteed Time Observations (GTO):
Guaranteed Time Observation program is a new category. Proposals for GTO Programs can only be submitted by
- the teams whose "Proposals for Development for Nobeyama 45-m Telescope" have already approved and instruments are decided to be open-use instruments.
- graduate students and posdocs in the observatory who contribute to science operations, commissioning activities or optimisation of the Nobeyam 45-m telescope, and authorized by the observatory.
The total observing time for GTO programs is less than 300 hours.
45-m Semester 2017A (Regular, Large, Short, GTO, and Backup programs):
1st September 2017, 15:00JST [06:00UT]
45-m Semester 2017B (Regular, Short, GTO, and Joint with the ASTE programs):
12th December 2017, 15:00JST [06:00UT]
The observatory only accepts Target of Opportunity observations for Regular, Short, DDT programs.
H22, H40, Z45, T70, and FOREST receivers are available for the open use.
TZ receiver is decommissioned. (Observations in On-On mode can be performed with FOREST receiver, instead.)
Japan domestic remote observation other than Mitaka may be possible as risk-shared, depending on test results.
Remote observation from ASIAA is available as risk-shared.
Requested hours of all submitted proposals vs. Allocated hours for accepted proposals at each LST
A sum of Regular Program and Short Program for the 2016-2017 season.
If you click the figure below, you can see a larger image.
Important notice about the main differences from the previous season is summarised as follows:
|Observing Categories||The observatory calls for proposal for two semesters (Semester A and Semester B). New observing category, Guaranteed Time Observation (GTO) Program, is added. Details for each category are described in Proposal Categories and Submission Deadline section in "A Guide for Proposal Submission via Web".|
|Receivers at 100 GHz||1. TZ receiver is decommissioned.
For the On-On observation, applicants can use Beam 1 and Beam 3 of FOREST receiver (beam separation is ~70 arcsec) instead.
2. The observatory offers new IF for FOREST receiver.
New IF (LSB-H) is available for FOREST receiver which covers a range of 7 GHz to 11 GHz for lower side band.
|Remote Observation||Experienced observers are allowed to perform remote observations in Japan (Not limited to the NAOJ Headquarter in Mitaka, Tokyo) and in Taiwan (from Academia Sinica Institute of Astronomy and Astrophysics [ASIAA]). Those who wish to perform remote observations should state in "Site" section in the Application Form and read carefully instructions summarised in Remote Observation. No compensation of observing time will be made even when your observing time is lost due to trouble, bad weather, or any cases. A preliminary test is needed before your observation.|
|Time Estimator||The time estimator is updated: time estimation with obtaining two polarisations and an improvement of estimation with more realistic system temperature based on measurements of atmospheric opacity.|
|Carried-Over Observations||Due to a malfunction of the master collimator driving system, observing programs of the observing season 2016--2017 (about 400 hours) were cancelled and carried over to the observing season 2017--2018.|
|Helpdesk||NRO offers Helpdesk support. Requests and questions about the open use of the Nobeyama 45-m telescope can be available through the Helpdesk. A trigger of Target of Opportunity observations should be sent to the Helpdesk.|
|Web Submission||We accept the proposal only via web submission form. If you face any difficulty in web submission, please contact us through the Helpdesk.|
|Support for New Users||The NRO staff offers support for observers who are not familiar with observations using the Nobeyama 45-m telescope. We provide support from help getting started to full collaboration. Please contact us via the Helpdesk for questions on proposal preparation, observing techniques and strategies, observation scripts, and data analysis.|
|ToO Observation||Please note that you should submit a proposal for Regular Programs, Short Programs, or GTO Programs for studies of expected ToO (Target of Opportunity) objects such as comets, gamma ray bursts, and extragalactic supernovae. The ToO trigger should be sent to the Helpdesk.|
|Target Duplication Check||Applicants are required to check their targets in the NRO 45-m legacy projects before submission. If the their target already observed and target lines are as same as you desire, the reason why you need to be observed by yourselves must be described in Science Justification.|
|Observational Support for the Open Use||The assistant supports the open use observations, including remote observations. The assistant conducts the receiver tuning and the trouble shoot. In order to shorten communication time between users and the assistant, experienced users can tune the receiver by themselves.|
|Proprietary Period||By default, data obtained as part of the Nobeyama 45-m science program are subject to a proprietary period of 18 months starting when all the observations of each project are complete.|
|Change Request||Major change requests are defined as 1) adding new sources, 2) changing observing lines, and 3) changing mapping areas from the original proposals. Change requests are made through the Helpdesk. After a contact to the Helpdesk, an observer must submit a paper in which reasons are described within 1 page of A4. The paper must include a very clear description of the proposed change along with a clear, substantive justification for the change. The requests will be evaluated by the Time Allocation Committee (TAC) chair and the observatory director and will be approved only if they are fully justified. Change requests duplicating against current NRO proposals will not be approved.|
|Effect by Automotive Millimetre-Wave Radar||Automotive millimetre-wave radar mounted on the car may cause unwanted signals at 76-77 GHz. The observatory suggests users avoid RF setting around 76--77 GHz if possible. Following links represent the results of test observations of receiving automotive millimetre-wave radar emitted from different types of cars: link1 link2|
|Re-allocation||Cancelled observing time due to unexpected instrumentation/telescope failure will be re-allocated. Observing time surrendered to backup programs due to bad weather also will be compensated.|
|Travel Support||(1)The observatory will support travel expenses of domestic transportation in Japan for up to two observers per program is supported if you request financial support from the NAOJ. (2)If you come to NRO by train, the observatory offers transportation service from Nobeyama Station to the observatory. Please describe the need of transportation service and your arrival time on On-line Submission of Observing Plan Sheet.|
|Cooperative Observation||The observatory encourages applicants to study based on observations with the 45-m telescope and the ASTE Telescope and/or the James Clerk Maxwell Telescope (JCMT).|
|Visiting Instruments||The observatory allows to carry-in visiting instruments. Call for Proposals for Development for Nobeyama 45-m Telescope (Already ended for this year). If you are planning to carry-in a new instrument such as a receiver, you are requested to submit a PI instrument proposal to the observatory. The procedure can be asked through our Helpdesk. Especially, we strongly request the PI to contact the observatory via the Helpdesk about your plan before submitting a funding proposal.|
|NRO's policy||NRO's Policy to Exclude Military Researches from the Open Use of the Observing Facilities|
Proposal Preparation Guide:
Proposal Submission Form
If your proposal is approved, PI (a delegate) needs to send an observing plan sheet. Observers who will visit NRO can make a reservation for lodging with the sheet. The observatory will support travel expenses for two domestic observers (two times in total for observations and data reduction).Instructions for Observers (written in English):
A computer account is necessary for your observations. Information of the account will be sent to the principal investigator (or the contact person).