Title: Photometric Redshifts in Astro-Wise
1Photometric Redshifts inAstro-Wise
Jan Snigula, MPE
Astro-Wise Workshop Leiden 2008
2Introduction
- Photometric redshiftsdeducing redshifts from
photometry in multiple optical and NIR filter
bands
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Astro-Wise Workshop Leiden 2008
3Photometric redshifts
- Redshift estimation and source identification
- Luminoisty function
- Galaxy clusters
- Large scale structures
- Search for special objects (AGNs, L-stars)
4Introduction
SEDs convolved with observed filters Stepped
in redshift
Astro-Wise Workshop Leiden 2008
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5Introduction
- Best fitting z and SED are determinded by
minimizing - The probability of a a source being at a given
redshift is
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Astro-Wise Workshop Leiden 2008
6Input files
- Galactic and stellar SEDs - PhotRedSED
- Filter transmission curves - PhotRedFilter
- Photoz configuration - PhotRedConfig
- Sourcelists
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Astro-Wise Workshop Leiden 2008
7PhotRedSED
- Galactic and stellar SEDs
Wavelength and flux
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8PhotRedFilter
- Filter transmission curve
Wavelength and transmission
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9PhotRedConfig
- Convolves SEDs with filter curves
- Needs only to be created once for a combination
of SEDs/filters - Supports up to 15 filters
- The filters used for the photoz run can be a
subset of the filters used for config
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10PhotRedCatalog
- Calculates the photometric reshifts from several
sourcelists and a PhotRedConfig - Uses one master detection sourcelist and
photometry from the other sourcelists
(associating them by their position) - The use of sourcelists created using the
sextractor double image mode is recommended.
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11PhotRedCatalog
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12PhotRedCatalog
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Astro-Wise Workshop Leiden 2008
13PhotRedCatalog
from astro.recipes.PhotRedCatalog import
PhotRedCatalogTask
awegt
awegt
taskPhotRedCatalogTask(
master_sl1122110,
...
sls1122110,1122111,1122112,1122113,
...
config'WFI_all_filters',
min_num_sources5,
namez_test)
awegt
task.execute()
awegt
p(PhotRedCatalog.namez_test)0
awegt
p.plot(23)
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14Caveats
- Adequate spectral coverage is needed, i.e. at
least 4-5 filters, including NIR - Only works on aperture photometry obtained on PSF
matched images - SEDs degenerate for certain redshifts
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15News
- Photoz code and FDF SED set available in the
federated AW system - Recipe now available,parallel version planned
- Move of photoz code to new codebase this summer
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