- Gemini Home
- Telescopes and Sites
- Science Visitors at Gemini
- Observing With Gemini
- Retired Instruments
- Visiting Instrument Policy
- DSSI Speckle Camera (North)
- TEXES (North)
- Integration Time Calculators
- Adaptive Optics
- Magnitudes and Fluxes
- Near-IR Resources
- Mid-IR Resources
- Observing Condition Constraints
- Performance Monitoring
- SV/Demo Science
- Future Instrumentation
- Queue and Schedules
- Data and Results
- Image Library
Change page style:
Integration Time Calculators
Available integration time calculators:
GMOS North (optical imaging and long-slit spectroscopy) - v5.0
GMOS South (optical imaging and long-slit spectroscopy) - v5.0
|GSAOI (near-IR AO imager for GeMS) - v1.0
NIFS (near-IR integral field spectrograph) - v5.0
Flamingos-2 (near-iR imaging and long-slit spectroscopy) - v5.0
Michelle (mid-IR imager and spectrometer) - v5.0
T-ReCS (mid-IR imager and spectrometer) - v5.0
|GNIRS (near-IR spectroscopy) - v5.0||Acquisition Camera (optical imaging, instrument retired) - v5.0|
Occasionally the ITCs will display duplicate plots on the spectroscopy mode results page instead of both flux and S/N plots. A workaround while the problem is being investigated is to refresh the page with the browser Reload button.
January 2012 - Default GMOS-N CCD type set to "EEV DD array", inactive options removed
September 2011 Default GMOS-N CCD type set to "EEV array"
February 2011 Changed CC90 to CC80. Added GMOS-N Hamamatsu CCD options.
September 2012 - GSAOI ITC initial release
January 2012 - F2 ITC initial release, inactive options removed
February 2011 Changed CC90 to CC80.
The Gemini Integration Time Calculator (ITC) consists of a web form in which the user defines the principal aspects of the observation and a Java servlet, resident on a Gemini Observatory computer, which performs the calculation and generates the results.
The web form is divided into four sections: (1) the spatial profile, spectral shape and brightness of the astronomical source, (2) the instrument and telescope configuration, (3) the observing conditions and (4) methods of how the observation will be carried out and the results analysed. There are additional help pages in each section that provide further information (e.g. see the more info links within the form).
Within the form, the desired characteristics are defined by selecting radio buttons (e.g. to choose between point or extended source), pull-down menus (e.g. to select the units for source brightness) and text boxes to enter numerical values (e.g. for source brightness). Clicking on the calculate button will post the user-defined values to the servlet and create an output web page containing the results. Unavailable features are indicated by red crosses.
The ITC is built around re-usable modules (e.g. for definition of the astronomical source) and specific elements for individual instruments. There is a separate web form for each instrument. Only the facility instruments listed above are supported; sensitivity tables are available for visiting instruments on the relevant web pages.
Caution: the ITCs make some as yet unverified assumptions about telescope and instrument performance and approximations for computational simplicity. Estimated accuracies will be posted as they become available. The calculated integration times do not take overheads into account.
ITC performance: imaging calculations typically take 4s, spectroscopic calculations take 10-20s, longer for large IFU calculations. (The calculation is the same in the spectroscopic case as for imaging but generating the graphics consumes 10-15s).
Last update 22 August, 2012; Bryan Miller