Shapelet Space STEP

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Shapelet Space Shapelet Space STEP STEP F. William High F. William High , , Research Assistant Research Assistant Caltech Caltech Tuesday, July 26, 2005 Tuesday, July 26, 2005

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Shapelet Space STEP. F. William High , Research Assistant Caltech Tuesday, July 26, 2005. Overview. Set σ γ / n 1/2 ~ 0.1% n g ~ 100/arcmin 2 σ γ ~ 0.3 n im = 50 or 100 Various θ px HDF Galaxies (mostly) Raytraced PSFs FOV 200”x200” SNAP 160”x160” ACS. T exp 1 ks SNAP wide - PowerPoint PPT Presentation

Transcript of Shapelet Space STEP

Page 1: Shapelet Space STEP

Shapelet Space Shapelet Space STEPSTEPF. William HighF. William High,,Research AssistantResearch AssistantCaltechCaltech

Tuesday, July 26, 2005Tuesday, July 26, 2005

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7/26/20057/26/2005 Shapelet Space STEPShapelet Space STEP F. William High, CaltechF. William High, Caltech

OverviewOverview

Set Set σσγγ//nn1/21/2 ~ 0.1% ~ 0.1% nngg ~ 100/arcmin ~ 100/arcmin22

σσγγ ~ 0.3 ~ 0.3 nnimim = 50 or 100 = 50 or 100

Various Various θθpxpx

HDF Galaxies (mostly)HDF Galaxies (mostly) Raytraced PSFsRaytraced PSFs FOVFOV

200”x200” SNAP200”x200” SNAP 160”x160” ACS160”x160” ACS

HDFHDF

Raytraced Raytraced PSFsPSFs

Measure Measure ShapeletsShapelets

Change Change orientation, orientation, size, flux, size, flux, ShapeletsShapelets

ShearShear PSF PSF convolveconvolve

TTexpexp

1 ks SNAP wide1 ks SNAP wide 2 ks ACS WFPC22 ks ACS WFPC2

Uniform across “chip”:Uniform across “chip”: DepthDepth NoiseNoise Input shearInput shear PSFPSF

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The StarsThe Stars

Label: Label: psf*psf*

PSFPSF SourceSource

A, BA, B SNAP SNAP BaselineBaseline

Steve Kent’s Steve Kent’s `raytrace` `raytrace` softwaresoftware

CC 1.4 meter 1.4 meter “SNAP”“SNAP”

Also Also `raytrace``raytrace`

D-LD-L ACSACS TinyTimTinyTim

Our PSFs account for:Our PSFs account for:

• Diffraction, including strutsDiffraction, including struts

• Charge diffusionCharge diffusion One globular cluster per psf*One globular cluster per psf*

Convolve in Shapelet spaceConvolve in Shapelet space

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The GalaxiesThe Galaxies

Label: Label: psf*psf*

PSFPSF θθpxpx Object Object TypeType

AA SNAP SNAP BaselineBaseline

0.05”0.05” ShapeletShapelet

BB 0.10”0.10”

CC 1.4 meter 1.4 meter “SNAP”“SNAP”

0.040.04

DD ACSACS 0.04”0.04”

EE 0.10”0.10”

FF 0.04”0.04” ExponentialExponential

GG 0.10”0.10”

H-LH-L 0.04”0.04” ShapeletShapelet

Lo

garith

mic

Lo

garith

mic

grayscale

grayscale

Shear to 4Shear to 4thth order order in Shapelet spacein Shapelet space

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The NoiseThe Noise

Shot noiseShot noise: readout, zodiacal (but : readout, zodiacal (but background subtracted)background subtracted) Exposure timeExposure time ttexpexp = ~1 ks SNAP, ~2 ks ACS = ~1 ks SNAP, ~2 ks ACS

Larger Larger θθpxpx @ fixed t @ fixed texpexp ↔ larger noise ↔ larger noise &&

signal-to-noisesignal-to-noise

Perfect Perfect Charge Transfer EfficiencyCharge Transfer Efficiency UncorrelatedUncorrelated: pre-: pre-drizzledrizzle

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The ResultThe Result

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ConclusionConclusion

962 images, 7-11 arcmin962 images, 7-11 arcmin22, 40 Gb total, 40 Gb total ftp://ftp://www.astro.caltech.edu/pub/fwh/SpaceSTEPwww.astro.caltech.edu/pub/fwh/SpaceSTEP//

100+ parallel processors @ NERSC/LBL100+ parallel processors @ NERSC/LBL Email Will (Email Will ([email protected]@astro.caltech.edu) and ) and

Richard (Richard ([email protected]@astro.caltech.edu) with ) with questionsquestions

Deadline: mid-SeptemberDeadline: mid-September