ECHMAP --- Echelle Wavelength Coverage Simulator

THIS SOFTWARE IS EXPERIMENTAL

This is unlikely to work at all unless you are running an X11 compatible windowing system (including OpenWindows) that implements the xterm application or something very similar. You also need to be able to run program ssh (secure replacement for rsh) to make this connection.


The program ECHMAP draws a map of how the orders from the 4m echelle spectrograph will fit onto the CCD detector. It allows you to interactively experiment with different grating tilts, gratings, cameras, etc. so that you can determine the best setup for your project.

The map includes:

Users can interactively:


USE

Due to our efforts to improve computer system security here at CTIO, you'll need to use a secure login, ssh, to access the echmap program. If you have questions about ssh, see our CTIO Computer Security page.

NOTICE: The solution to the problems we were having with echmap running from GNOME/linux machines seems to be working. Let us know of any anomalies that show up...


EXAMPLE OF ANSWERS TO SETUP QUESTIONS:

This example is for the blue long camera + Tek2048, providing almost complete coverage from about

me@timbuktu% ssh ctios0.ctio.noao.edu -l echelle
echelle@ctios0's password: echmapper
Last login: Wed Mar 28 12:57:19 2001 from timbuktu
Welcome to ECHMAP (Local version)
 
[1] 10595
 

echelle grating? (1 = 31.6, 2 = 79): 2
x disperser l/mm: 316
x disp order: 1
camera (1 = short f.l., 2 = long f.l.): 2
port (1=right, 2=left): 2

Note: The red long camera always is on the right port, the 
blue long camera is always on the left. The air schmidt and 
folded schmidt can be used on either port.

ccd nx,ny,dx(mm),dy(mm): 2048 2048 .024 .024
central wavelengths: echelle, xdisp: 4982 4982
 name of file containing wavelengths (or none)?
none
 redshift?
0

Note that the wavelength file and redshift are not implemented for remote connections (sorry!), so the responses "none" and "0" are required as shown above.

The graph should look something like this (click for larger view)...


CURSOR COMMANDS

e = change echelle grating.

x = change cross disperser (and order).

c = change camera.

p = change port.

d = change detector size, pixel size (e.g., for binning)

w = move to new central wavelengths which you will be asked to enter.

m,m = move to new central wavelengths by moving the CCD from the position marked with the first m to the position marked with the second m.

q = quit program.

space = mark cursor position with *, print out x and y coords.

? or h = print out help menu.


Chris Smith: csmith@noao.edu