Crate gmt_lom 

Giant Magellan Telescope Linear Optical Model

Optical linear transformations applied to the rigid body motions of the primary and secondary segmented mirrors of the GMT

The optical sensitivities can be downloaded from here, or they can be recomputed with the makesens binary compiled with the crseo features and run on a computer with a NVIDIA GPU.

Example

use std::iter::once;
use skyangle::Conversion;
use gmt_lom::LOM;

let m1_rbm = vec![vec![0f64; 6]; 7];
let mut m2_rbm = vec![vec![0f64; 6]; 7];
m2_rbm
    .iter_mut()
    .step_by(2)
    .for_each(|str| {
       str[3] = 1f64.from_arcsec();
       str[4] = 1f64.from_arcsec();
 });
m2_rbm[6][3] = 1f64.from_arcsec();
m2_rbm[6][4] = 1f64.from_arcsec();
let lom = LOM::builder()
    .into_iter_rigid_body_motions(once((m1_rbm, m2_rbm)))
    .build()
    .unwrap();
let tt = lom.tiptilt();
println!(" Tiptilt: {:.0?}mas", tt);
let stt = lom.segment_tiptilt();
println!("Segment tiptilt:");
println!(" - x: {:.0?}mas", &stt[..7]);
println!(" - y: {:.0?}mas", &stt[7..]);
let sp = lom.segment_piston();
println!("Segment piston:");
sp.chunks(7).enumerate().for_each(|(k, sp)| println!(" - S{}: {:.0?}nm", k + 1, sp) );

Re-exports

pub use lom::LOMBuilder;

pub use lom::LOM;

Modules

lom

Structs

Loader

Data loader

OpticalSensitivities

Optical sensitivities

RigidBodyMotions

GMT M1 and M2 segment rigid body motions

SegmentPiston

Type holding the segment piston values

SegmentTipTilt

Type holding the segment tip-tilt values

Table

TipTilt

Type holding the tip-tilt values

Enums

Formatting

LinearOpticalModelError

OpticalSensitivity

Optical sensitivity

Traits

Bin

Sensitivities serialization into a bincode file

LoaderTrait

Loader loading interface

OpticalMetrics

Trait for the LOM optical metrics

Stats

Statistics on OpticalMetrics

ToPkl

Functions

from_opticals