APT ETC

User's Guide
Contents
Return to ETC
Welcome
SYNPHOT
SNR and Exposure Time
SNR
Time
Optimal SNR
Spectroscopy
Target Acquisition
Basic Use
Page Heirarchy
Reference
Extraction Regions
Spectral Distribution
User Spectra
Other Spectra
Extinction
Normalization
Background
CCD Parameters
ID Number
Calculations
SYNPHOT Calls
Call Descriptions
Call Parameters
NICMOS Spectroscopic Extraction Regions
Tables
Spectral Elements
NICMOS Filters
NICMOS Dispersers
ACS Filters and Dispersers
COS Dispersers
WFC3 Filters and Dispersers
STIS Filters and Dispersers
NICMOS Tables
COS Tables
STIS Tables and Topical Help

Welcome to the Exposure Time Calculator (ETC)

Welcome to the Astronomer Proposal Tool (APT) Exposure Time Calculator. The ETC is a web-based application developed in Java that assists Hubble astronomers and engineers in preparing Phase I and Phase II observing proposals for submission to the Space Telescope Science Institute (STSci). The ETC’s sole purpose is to calculate the following:

  1. Signal-To-Noise (SNR) Ratio (for a given Exposure Time)

  2. Exposure Time (given a desired SNR Ratio)

The ETC calculates SNR or Exposure Time for a simulated astronomical observation using one of Hubble’s primary instruments:

  • Advanced Camera for Surveys (ACS)

  • [future] Cosmic Origions Spectro (COS)

  • Near Infrared Camera and Multi Object Spectrometer (NICMOS)

  • Space Telescope Imaging Spectrograph (STIS)

  • [future] Wide Field Camera 3 (WFC3)

Since each instrument onboard Hubble is unique with its own image capturing modes, a separate ETC input web page must be created for every combination of instrument and science image modality. A single server shared by all of the instruments, however, handles all the SNR calculations and output pages.