Proposals: Call, Preparation, and Submission

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1. Eligibility and Responsibility

All registered users agree to act according to Observatory policies and procedures, as defined in this document and in the Call for Proposals documentation. In particular, all users accept the limitations of the observing capabilities and operational restrictions applicable for the call for which they submit a proposal. Any registered user may submit a proposal for the supported facilities.

Each proposal must identify an individual who will serve as Principal Investigator (PI). Proposals submitted by a consortium are not valid. Instead, a person within the consortium should submit the proposal and act as PI and any other consortium members are co-Investigators (co-Is). The PI or a co-I is required to be specified as the official contact between the Observatory and the proposing team for all proposal correspondence. By default, the PI is the official contact. The PI and all co-Is are responsible for ensuring that their respective profiles registered for the NRAO user account are correct (e.g., email address, affiliation). Proposals may include any number of co-Is.

By submitting a proposal, the PI takes full responsibility of its contents. The PI is responsible to ensure that all co-Is have agreed to be included on a proposal. Including a user as co-I in a proposal without their consent may lead to the proposal being canceled. Co-I names cannot be added to or be withdrawn from the proposal after the proposal deadline.

PIs and co-Is may all view, edit and submit proposals in the PST. Additionally, they all may create, modify, and submit Scheduling Blocks in the relevant workflow (e.g., Observation Preparation Tool; OPT). They are all entitled to receive help from, or discuss project details with, Observatory staff and receive the outcome of the review process.

2. Proposing Opportunities

There are two types of calls for proposals at the Observatory: semester and Director’s Discretionary Time (DDT).

2.1. Semester Observing Opportunities

Semester proposing opportunities are announced through a Call for Proposals. The observing proposal submission deadlines for Observatory facilities are the closest date to 01 February and 01 August that fall on a Wednesday1 each year. The February deadline applies to requests for observing time from 1 August–31 January; the August deadline applies to requests for time from 1 February–31 July. Proposals for the Semester Observing Opportunities must be submitted between the announcement of the Call for Proposals and the proposal deadline. The Call for Proposals contains the implementation parameters and procedures and is available online at https://science.nrao.edu/observing/call-for-proposals.

In response to a semester Call for Proposals, three proposal types can be submitted for the standard semester deadlines each year:

  • Regular proposals are for modest total time requests on Observatory facilities. The Call for Proposals specifies the maximum number of hours a Regular proposal is allowed, which may depend on the capabilities of a facility.
  • Triggered proposals are for pre-planned observations of transients whose event times are unknown a priori.
  • Large proposals are for large total time requests on Observatory facilities. The Call for Proposals specifies the maximum number of hours a Large proposal is allowed, which may depend on the capabilities of a facility.

Triggered Proposals

For a Triggered proposal that is not considered Large, users shall specify the proposal type as "Triggered" in the PST. If a proposal is partially Triggered, the entire proposal is considered a Triggered proposal. If the proposal is also Large, users should specify the proposal type as "Large" in the PST and provide clear triggering criteria in the scientific justification.

Joint Proposals

Joint proposals with non-AUI facilities and commensal observing are proposed for within the scope of these proposal types, see Section 3.2.3 and Section 7.4, respectively. Note, Large proposals can have triggering criteria; users should specify the proposal type as “Large” in the PST. When determining whether a joint proposal qualifies for as a Large Proposal, the total time requests are evaluated per facility and not as an aggregate sum. When a facility, such as the VLA or GBT, is requested as part of the VLBI/HSA or GMVA, its time is categorized under the VLBI/HSA or GMVA facility for the purpose of meeting the criteria of a Large Proposal. However, if the same facility (like VLA or GBT) is simultaneously requested as a joint resource apart from being an element of the aforementioned facilities, their respective time requests remain distinct and are not compounded when assessing against the Large Proposal threshold.

Requests for Future Capabilities

Proposals submitted to a semester call must contain capabilities offered in that semester call. An exception is for a PI who is a graduate student, who may propose up to one semester in advance for capabilities offered on the GBT, HSA, and VLBA. For the VLA, a PI who is a graduate student may propose for any array within one VLA configuration cycle (see Section 7.1 for definition). For other exceptional cases, please seek guidance from the NRAO Science Helpdesk. Submission of such cases will be subject to the NRAO's discretion.


1 The exact call period will be announced in the Call for Proposal.

2.2. Director’s Discretionary Time

DDT may be requested at any time and is appropriate for the following cases:

  • Target of Opportunity (ToO) proposals are for unexpected or unpredicted phenomena such as, but not limited to, extreme X-ray or radio flares. ToO proposals are evaluated rapidly, with scheduling done as quickly as possible and as warranted by the nature of the transient phenomenon.
  • Exploratory Time proposals are normally for requests of small amounts of time, typically a few hours or less, in response to a recent discovery, possibly to facilitate a future submission of a larger proposal. In general, there will not be a need for immediate scheduling with these proposals but, for example, they may need to be observed in the current VLA configuration rather than waiting 16 months.
  • Proposals may be submitted for the purpose of education and public outreach - for example, to image an iconic source or to support a educational opportunity for students. These proposals must involve the Observatory’s Education and Public Outreach program.
  • Proposals for other science opportunities deemed sufficiently urgent to justify prompt action.
  • Proposals may be submitted in response to a Special Call announced by the Observatory. The announcement for the Special Call is available online at https://science.nrao.edu/observing/call-for-proposals.

While there is not an a priori limit to time that can be requested via DDT, it is expected that no more than 5% of the Open Skies time on each facility will be allocated for this purpose. DDT proposals cannot be joint proposals that request external telescope time; however, joint proposals between the Observatory’s facilities are allowed. For example, a DDT proposal cannot request HST orbits, but a DDT proposal can request joint observations with the VLA and VLBA.

2.3. Joint Proposing Opportunities

There are a number of opportunities for joint proposals with external (non-Observatory) facilities and between the Observatory’s facilities. The time will be awarded only for proposals that require use of both observatories and shall not apply to usage of archival data. The observations are not required to be coordinated or simultaneous, and the programs may be subject to basic feasibility reviews. All joint proposals submitted through the PST must indicate the joint facility, specify the requested time for the joint facilities, and additional details. The Call for Proposals contains the most up-to-date opportunities and requirements for joint proposals.

Joint proposals between the Observatory’s facilities consist of observing programs that require combinations of the GBT, VLBA, and/or the VLA. For such requests, proposers should submit a proposal for each of the requested telescopes. The same Scientific Justification should be submitted with each proposal, and it should contain a clear justification for each telescope requested. VLBI proposals which request the GBT or VLA (or any other HSA telescope) as elements of the VLBI array do not need separate proposals as those telescopes can be selected as separate VLBI stations from a VLBA/HSA proposal. When determining whether a joint proposal qualifies for as a Large Proposal, the total time requests are evaluated per facility and not as an aggregate sum. For example when a facility is requested as an element of the VLBI array, its time is categorized under the VLBI facility for the purpose of meeting the criteria of a Large Proposal. However, if the same facility is simultaneously requested as a joint resource apart from being an element of the aforementioned facilities, their respective time requests remain distinct and are not compounded when assessing against the Large Proposal threshold.

For joint proposing opportunities with external facilities, one proposal should be submitted to the facility where more observing time is being requested; authors should not duplicate their request across the observatories in this case. Authors may re-submit the proposal if their previous submission was rejected (partially or fully), or if the outcome of the previous submission is unknown.

If the latter and a positive disposition is eventually received, it is expected that the duplicate proposal be withdrawn promptly. Proposing teams that are awarded time through an external Telescope Time Allocation Committee (TAC) must adhere to the policies of this document when applicable. If the policies of this document conflict with that of another facility, the Observatory will work with the proposing team and external facility to reach a suitable resolution.

Detailed information about the external joint proposing opportunities can be found within their corresponding Memorandum of Understanding. These documents are accessible online at https://science.nrao.edu/observing/proposal-types/joint-proposal-opportunities. Note, the agreements for Joint Observations with external facilities were made at different times across the boundaries when the Observatory was split into multiple observatories (NRAO, GBO, and LBO) in 2017, and when the Long Baseline Observatory (LBO) was reintegrated back into the NRAO in 2019. Therefore, the Memorandum of Understandings will sometimes mention various combinations of the NRAO, GBO, and LBO.

Table 2.1 summarizes the amount of time that may be awarded from either the Observatory TAC or the External TAC to an external joint proposal. Column 2 gives the amount of time an External TAC may award on an Observatory facility, and column 3 gives the amount of time the Observatory TAC may award on the external facility. Proposing teams should consult the Call for Proposals for the specific guidelines when preparing a joint proposal.

Table 2.1: Summary of Joint Proposing Opportunities
External Facility External TAC (Observatory Time)a Observatory TAC (External Time)
ALMA 5% 50 hrs per cycleb
Chandrac 3% 120 ks per year
Fermi 5%d 300 ks per year
HSTe 3% 30 orbits per year
JWST 5% 50 hrs per year
NICER 5%f 250 ks per year
Swift 5%f 300 ks per year
XMM-Newton 3%

150 ks per year

a Percentage of observing time that is considered Open Skies.
b The Observatory can award up to 50 hours on the ALMA 12-m array, 50 hours on the 7-m array, and 50 hours on the Total Power array per cycle.
c Chandra ToO proposals are not supported under the Chandra-NRAO joint program.
d A maximum of 5% or up to 200-325 hours of Open Skies observing time per year is available on each telescope.
e HST Snapshots observations are not supported under the HST-NRAO Joint program.
f A maximum of 5% or up to 200-300 hours of Open Skies observing time per year is available on each telescope.

3. Proposal Preparation

3.1. Proposal Requirements

Proposals for observing time at any of the Observatory’s facilities must be submitted through the PST. In addition to the VLA, VLBA, and GBT facilities, observing proposals for the following non-AUI telescopes are required to utilize the PST: the VLBI-High Sensitivity Array (HSA) and the Global 3mm proposals (GMVA). A detailed guide for the PST is available online at https://science.nrao.edu/facilities/vla/docs/manuals/proposal-guide.

Proposal preparation in the PST consists of a number of components that must be specified by the user and in compliance with following requirements.

General Information

  • The General Information of a proposal includes the title, abstract, author list, proposal type (DDT, Regular, Large, etc), proposal sponsor, scientific category, declaration of a joint proposal, observing type, and related proposals.
  • A single science category is required per proposal. Proposals that span multiple categories should be split into multiple proposals.

Authors

  • All authors should be listed on the proposal at the time of submission, as it is not possible modify a proposal after submission. As stated Section 3.1, including a user as co-I in a proposal without their consent may lead to the proposal being canceled.
  • If the proposed observations are part of a PhD dissertation, a “Plan of Dissertation Research” is required to be submitted with the proposal. If the observing semester occurs after the student intends to graduate, then it is not appropriate to indicate that the proposal is for a dissertation. See Section 7.2 for more details.

Scientific Justification

  • The Scientific Justification is required to be a Portable Document Format (pdf).
  • There should be a minimum of one inch margins on all sides and pages are US letter sized.
  • The minimum font size is 11 point, which includes the font in figure captions, table captions, table headers, content, and references. Fonts in rescaled figures should be legible.
  • The maximum number of pages includes figure captions, table captions, table headers and content, and references:
    • Regular proposals are allowed a maximum of four (4) one-sided pages.
    • Triggered proposals are allowed a maximum of four (4) one-sided pages.
    • Large proposals are allowed a maximum of six (6) one-sided pages.
    • DDT proposals are allowed a maximum of two (2) one-sided pages.
  • For a Large proposal, a plan for data management and data release is a mandatory part of the Scientific Justification.
  • For a DDT proposal requesting Exploratory Time, proposals must include a clear description of why the proposal could not have been submitted for normal review at a previous semester proposal deadline, and why it should not wait for the next proposal deadline. The possibility that a proposer forgets about or misses a proposal deadline, or just discovered that they were granted time for a particular source on some other telescope, will not constitute sufficient justification for granting observing time by this process.
  • For a DDT proposal requesting time for educational purposes should clearly justify the requirements for the requested time allocation and observing mode on any given instrument and should describe the anticipated impact of the observation.
  • For joint proposals, the Scientific Justification must clearly justify the need for each requested facility.
  • For joint proposals between the Observatory’s facilities, the same Scientific Justification must be submitted with each of the joint proposals.

Technical Justification

  • The PST provides prompts for the author to enter their technical justification. The relevant prompts are required to be fully specified and are required to include any additional requested materials, such as the output from a sensitivity calculator and/or a mapping calculator.

Sources

  • The Observatory requires proposers to specify their source lists in full. It may be the case that the final source list has not been selected at the time a proposal is submitted. In such cases, all potential sources should be listed. The only exceptions to this requirement are for Triggered proposals to observe sources that are unknown a priori. Note, calibrators should not be specified in the source list.

Resources

  • In the PST, proposers are required to specify their requested resources. Depending on the resources requested, additional materials may be required (e.g., spectral line resources), which will be noted in the interface of the PST.

Sessions

  • Proposers are required to specify the Local Sidereal Time (LST) range, which should take into account constraints from calibrators and in addition to sources.

Proposers should also consult the online documentation for guidance and more information about preparing their proposals:

GBT https://greenbankobservatory.org/science/gbt-observers/proposals/
VLA https://science.nrao.edu/facilities/vla/proposing
VLBA https://science.nrao.edu/facilities/vlba/proposing

3.2. Compliance in Proposal Preparation

Proposals that are not in compliance with Observatory policies may be rejected or be reduced in scheduling priority. The following is a non-exhaustive review of common cases of non-compliance.

  • A Regular proposal that is determined to be incorrectly submitted as a Triggered proposal.

  • A Triggered proposal that is incorrectly submitted as a Regular proposal.
  • A Scientific Justification that is not compliant with the formatting requirements described above.

  • Relevant information is missing from the Technical Justification. This includes the additional materials such as the output of the sensitivity calculator or mapping calculator.

  • The information in the output of the sensitivity calculator, mapping calculator, spectral line configuration, etc. is incomplete or incorrect.

  • Proposals that intentionally propose for inaccurate source coordinates with the purpose of obscuring the true positions of the sources.

  • A Large proposal that fails to provide a data management and data release plan.

3.3. Filler Programs

There are opportunities for so-called “filler” programs on all telescopes. Observing programs that exploit frequencies below 10 GHz, do not have scheduling constraints, and could benefit from short scheduling blocks are eligible to be considered for “filler” time. The proposal should make clear in the abstract and in the science justification that “filler” time is being requested. If “filler” time is requested, the proposal will be ineligible for scheduling priority A or B. A proposal requesting filler time should not require fixed time or guaranteed monitoring periods.

3.4. Proposal Science Categories

Proposal science categories are defined to group proposals with similar science intents for consideration by reviewers who are familiar and/or experts in the field. The categories can change, though generally, the science categories do not fluctuate frequently. Currently, proposals for the use of Observatory facilities are organized according to one of the following scientific categories:

SSP Solar system, stars, planetary systems: Sun, planets, comets, IPM; exoplanets; main sequence stars; active stars; stellar winds; AGB and post-AGB stars; PNe; novae
GWT Gravitational waves and energetic transients: supernovae, gravitational wave sources, gamma-ray bursts, tidal disruption events, fast radio bursts, exotic/unknown transients
PCO Pulsars and compact objects: millisecond pulsars, cataclysmic variables, black hole and/or neutron star x-ran binaries, pulsar timing, pulsar proper motion
SFM Star formation: young stellar objects; protostars; jets, outflows; T Tauri stars, circumstellar disks; protoplanetary systems; astrochemistry
ISM Interstellar medium: galactic HI and OH; ISM magnetic field, SNRs; HII regions; astrochemistry
NGA Normal galaxies, clusters, and groups: Galaxies (continuum), including galaxies in groups and clusters: disk emission; star formation; magnetic fields; galactic winds; starbursts; intracluster emission and ICM astrophysics
EGS Extragalactic structure: Galaxies (lines): galaxy structure; galaxy kinematics and dynamics; galaxy chemistry; gas in galaxies
HLA High-Luminosity AGN: AGN, high-luminosity: FR II radio galaxies, quasars, QSOs, blazars, BL Lacs
LLA Low-Luminosity AGN: AGN, low-luminosity: FR I radio galaxies, FR 0 radio galaxies, Seyfert galaxies, quiescent SMBG, Sgr A
HIZ High redshift and source surveys: High-z objects; extragalactic source surveys; galaxy formation; gravitational lenses; large-scale structure and clusters (as cosmological probes); CMB; early universe

Observatory staff reserve the right to change the user selected science category of a proposal to a more appropriate one if warranted without consulting with or notice to the PI.

4. Proposal Submission and the Close of the Call for Proposals

4.1. Compliance in Proposal Submission

Only proposals that are submitted via the online PST, that comply with the technical constraints and restrictions described in the Call for Proposals, that conform to the policies stated in this document, and that are received before the submission deadline will be considered. The Observatory reserves the right to reject proposals that do not adhere to the policies in this document.

For semester proposals, the proposal deadline is strictly enforced: no modifications to the proposal can be made by the author after the close of the call. If before the proposal deadline, it is possible to withdrawal a proposal and submit a new version (see Section 3.4.3). Requests to the Helpdesk for modifications to the proposal after the deadline will not be considered. Such requests include, but are not limited to, modifying the author list, the contents of the proposal, and modifying the requested items, such as source coordinates, requested time, or facility resources. Users should not submit duplicate proposals during a single Call for Proposals with the intention of acquiring a more favorable review.

4.2. Extension of the Close of Call for Proposals

The Observatory encourages users to leverage the NRAO Science Helpdesk and Knowledgebase in preparing their proposals. The Helpdesk is actively monitored to provide timely responses to inquiries, particularly near the close of the Call for Proposals. If an inquiry to the NRAO Science Helpdesk is made sufficiently ahead of the deadline but the issue is not resolved by the deadline, the Observatory will work with the proposers to reach a reasonable solution. The Observatory is not ultimately responsible, however, for late proposal submissions that are a result of inquiries with the Helpdesk - particularly last minute requests. The Observatory encourages users to consult Helpdesk resources far ahead of the deadline and to submit their finished proposals well in advance of the deadline.

There are many third party applications and services (e.g., Overleaf, Google Suite) that may aid a proposer in preparing their proposal. In the event that such a third party application experiences an outage or is otherwise unavailable, the Observatory is not responsible for the impact on a user’s ability to submit a timely proposal.

It is not the policy of the Observatory to extend the deadline for the Call of Proposals without sufficient cause. It is at the discretion of the Assistant Director for Science Support and Research if such an extension is warranted. If an extension is deemed necessary, a banner message will appear on the PST portal to indicate the new deadline.

4.3. Changes to Submitted Observatory Proposals

For semester proposals, proposers have the ability to withdraw their proposal directly through the PST without needing to contact the NRAO Science Helpdesk. If this action is taken prior to the proposal deadline, a new proposal can be submitted. Note that the PST currently permits proposal withdrawal only if it’s initiated a minimum of fifteen (15) minutes before the deadline. Beyond this time frame, proposers will need to contact the NRAO Science Helpdesk to withdrawal a proposal. After the proposal deadline, a submitted proposal may be withdrawn but no longer modified. Requests for withdrawal should be made via the NRAO Science Helpdesk. It is at the discretion of the Observatory to permit withdrawal however; if the review process has begun, the proposal will not be withdrawn.