Mr. Yatrik Patel Profile

Yatrik Patel

at NOIRLab

SPIE Involvement:

Author

Publications (1)

This will count as one of your downloads.

You will have access to both the presentation and article (if available).

DOWNLOAD NOW

This content is available for download via your institution's subscription. To access this item, please sign in to your personal account.

Email or Username Forgot your username?

Password Forgot your password?

Show

Keep me signed in

No SPIE account? Create an account

Proceedings Article | 25 July 2024 Presentation + Paper

Running a modern queue: lessons learned from the first three years of NEID operations

Heidi Schweiker, Sarah Logsdon, Mark Everett, Jayadev Rajagopal, Erik Timmermann, Eli Golub, Diego Gomez, Pipa Fernandez, Jesus Higuera, Yatrik Patel

Proceedings Volume 13098, 1309808 (2024) https://doi.org/10.1117/12.3020650

KEYWORDS: Equipment, Databases, Telescopes, Observatories, Automation, Calibration, Windows, Target acquisition, Stars, Exoplanets

Read Abstract +

NEID is an optical, Extreme-Precision Radial Velocity (EPRV) spectrometer installed at the WIYN 3.5 m Telescope at Kitt Peak National Observatory near Tucson, AZ, USA. Primarily designed to find, confirm, and characterize planets outside of the solar system, NEID was built as part of the joint NASA-NSF Exoplanet Observational Research Program (NN-EXPLORE). Through the NN-EXPLORE program, ~50% of WIYN science time is made available to the public through standard NOIRLab bi-annual proposal calls. The other approximately 50% of WIYN science time is available to WIYN institutional partners. NEID entered full science operations in 2021B and is operated in queue mode, with a team of dedicated NEID Queue Observers carrying out nighttime operations. Currently, the NEID queue makes up approximately 70-80% of the available WIYN telescope time, with the other approximately 20-30% of the time made up of a combination of classically and queue scheduled time on other instruments. Operating NEID in queue mode is crucial for executing high cadence programs such as the publicly available NEID Standard Star program. Here we discuss the lessons learned in the early years of instituting and running a modern queue at a telescope that maintains some classical observing. We will give an overview of the software and staffing required to effectively run the queue and how we have both upgraded the software and modified operational procedures to increase efficiencies.

My Library

You currently do not have any folders to save your paper to! Create a new folder below.

Folder Name

Folder Description

View contact details

UPDATE YOUR PROFILE

Is this your profile? Update it now.

Sign into your SPIE.org account

Don’t have a profile and want one?

Create an account on SPIE.org

Access to the requested content is limited to institutions that have purchased or subscribe to SPIE eBooks. You are receiving this notice because your organization may not have SPIE eBooks access.*

*Shibboleth/Open Athens users─please sign in to access your institution's subscriptions.

To obtain this item, you may purchase the complete book in print or electronic format on SPIE.org.

ORGANIZATIONAL
Sign in with credentials provided by your organization.

Organizational Username

Organizational Password

Show/Hide Password

INSTITUTIONAL
Select your institution to access the SPIE Digital Library.

SELECT YOUR INSTITUTION

PERSONAL
Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.

PERSONAL SIGN IN

No SPIE Account? Create one

PURCHASE THIS CONTENT

SUBSCRIBE TO DIGITAL LIBRARY

50 downloads per 1-year subscription

Members: $195

Non-members: $335 ADD TO CART

25 downloads per 1 - year subscription

Members: $145

Non-members: $250 ADD TO CART

PURCHASE SINGLE ARTICLE

Includes PDF, HTML & Video, when available

Members:

Non-members: ADD TO CART

Keywords/Phrases

Search In:

Publication Years