About This Manual#

Purpose#

This document is intended to serve the needs of all users of NGPS including astronomers and observatory support staff.

Scope#

This document contains practical information related to the operation, maintenance, and troubleshooting of NGPS.

Reference Documents#

  1. NGPS Technical Specifications (NGPS.SYS.TEC.005)

  2. NGPS Spare Parts List.xlsx (NGPS.SYS.TEC.003)

Change Record#

Revision

Date

Section

Modifications

Ver 01

5/7/2026

All

NGPS Development Team, initial draft shared at Operations Handover Review

Ver 02, SP Ver (300.0)

7/31/2026

All

Released in response to OHR reviewers report actions

Abbreviations, Definitions and Nomenclature#

Acronyms#

Acronym

Meaning

AO

Adaptive Optics

COO

Caltech Optical Observatories

DRP

Data Reduction Pipeline

ETC

Exposure Time Calculator

FITS

Flexible Image Transport System

FOV

Field of View

GUI

Graphical User Interface

ICS

Instrument Control Software

NGPS

Next Generation Palomar Spectrograph

OTM

Observation Timeline Modeler

POMO

Palomar Observatory Mountain Operation

RD

Reference Document of any kind, typically cited outside of requirements text

SNR

Signal to Noise Ratio

TCS

Telescope Control System

TLE

Target List Editor

NGPS Overview#

Next Generation Palomar Spectrograph (NGPS) is conceived to be a radically more efficient workhorse spectrograph, replacing the 1970s-era Double Spectrograph (DBSP). NGPS achieves these gains via 1) increased optical efficiency from superior design and grating components, 2) a novel focal plane slicer unit that captures most traditional slit losses, 3) increased operational efficiency due to broad spectral coverage with fixed grating format and a minimal set of user-selectable settings, and 4) improved scheduling and observing tools, and feedback.