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The MODS Pipeline Kevin Croxall - OSU Reduction and Calibration of MODS Data LBT Users Meeting - March 23, 2014

Reduction and Calibration of MODS Data

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Page 1: Reduction and Calibration of MODS Data

The MODS Pipeline

Kevin Croxall - OSU

Reduction and Calibration of MODS Data

LBT Users Meeting - March 23, 2014

Page 2: Reduction and Calibration of MODS Data

MODS Data ReductionGoals and Vision

• High Quality Reduced Data Product

• Balance Automation Against Interaction

• Ease of Use

• Efficient & Rapid Execution

• Well Integrated Output Data

Page 3: Reduction and Calibration of MODS Data

Raw MODS

DatamodsCCDRed

MODS_REDUCESky Subtraction

Generate Sensitivity Function

Extract Spectra

MODS OTF Data

Python

IDL

MODS 2D

Spectra

MODS 1D

Spectra

MODS Reduction WorkFlow

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All Data flow through the same

Pipeline

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Prism Mode

Identify Slit Locations

MOS Mask

Long-Slit

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Wavelength Calibration Maps

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B-Spline Sky Subtraction

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B-Spline Sky SubtractionGrating Mode

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B-Spline Sky SubtractionPrism Mode

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Extracted 1D SpectraTraditional Row-Stacked Spectra Format

Sensfunc

Aperture 1

Aperture N

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We plan on having MODS Quick Look Tools release at LBT starting in the 2014B semester

Final on-site testing in April.

Longslit 1 slit ~70s / Longslit 5 slits ~380s / MOS ~40 slits ~1000s

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ManualAvailable April 15th

http://www.astronomy.ohio-state.edu/MODS/

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DistributionAvailable April 15th

The MODS pipeline will be available for Beta testing on the MODS webpage after April 15th.

It requires XIDL which can be obtained from the UCOLICK site (linked from MODS webpage).

Please report any bugs you find or other feedback.

http://www.astronomy.ohio-state.edu/MODS/http://www.ucolick.org/~xavier/IDL/

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Summary - 2D

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Summary - 1D

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Wavelength Zero-PointA.K.A. Flexure Correction

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Wavelength Zero-PointA.K.A. Flexure Correction

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Wavelength Calibration

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Wavelength Calibration

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Contours: 5577.34 + Shift

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Page 24: Reduction and Calibration of MODS Data

OTF

RAW

modsCCDRedBias correctionOverscan trimFlat-fielding

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We need to have a robust trace of each slit irregardless of position on the mask.

We mapped the system using an innovative Sudoku mask.

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Sudoku

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Sudoku

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Sudoku

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Mapping .MMS Files

Sudoku Mask

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Mapping .MMS Files

Sudoku Mask

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Wavelength Calibration

Sudoku Solution

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Wavelength Calibration

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Wavelength Calibration

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Wavelength Calibration Maps

Measured Map from arc Lamps

Empirical Map derived from Sudoku transforms

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B-Spline Sky Subtraction

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B-Spline Sky Subtraction

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B-Spline Sky Subtraction

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Dispersion Correction

Page 39: Reduction and Calibration of MODS Data

B-Spline Sky Subtraction

Page 40: Reduction and Calibration of MODS Data

B-Spline Sky Subtraction

Page 41: Reduction and Calibration of MODS Data

B-Spline Sky Subtraction

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Quick Look ToolsWe plan on having MODS Quick Look Tools release at LBT starting in the 2014B semester

Final on-site testing in April.

Page 43: Reduction and Calibration of MODS Data

Future Plans

• Better Documentation

• Bug Fixes

• Overall Wrapper

• Onsite Implementation of QuickLook for 2014B

• Your Input is Welcome