Census of the Star-forming
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Transcript of Census of the Star-forming
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Duilia de Mello
Some results presented are unpublished. If you need to referto this work contact me. Don’t use it without emailingme before, please, [email protected]
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Steidel et al. 1999
Extinction corrected
LBGs
| | | | 8.8 6 3.3 1.6 Gyr Duilia de Mello
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Lyman Break Technique
UV dropouts – z~2.6-3.4 [UV is detected in the optical]Steidel et al. 2004, Shapley et al. 2003, Pettini et al. 2000
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Rest-frame 1000 1200 1450 1925
LBGs spectra are similar to starbursts at low-z starbursts.
What are their morphologies?
Are they the building blocksof larger galaxies?
Need a large sample of LBGs!Deep images with high resolution.
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Giavalisco et al. 2004
HSTACS (B, V, i, z)Multi-epoch2 fields SouthNorth (CDF-SHDF-N) –316 arcmin2
0.03”/pixSpatial resolution 0.1’’
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B-dropouts : LBGs at z = 4
Ravindranath et al. (2005; in preparation)
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Steidel et al. 1999
Extinction corrected
LBGs
| | | | 8.8 6 3.3 1.6 Gyr Duilia de Mello
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Rest-frame UV
• 1500 Å at z~0.5 is observed at 2250 Å
• 0.8 2700
• 1.0 3000
• 1.2 3300
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1500 Å at z=1
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• WFPC2 (F300W) observations of GOODS/HST are shallow but cover large area.
• WFPC2 (F300W) observations of the Ultra Deep Field (UDF) - Deep but cover small area.
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Magnitude_Auto (F300W)
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UDF
GOODS
84 700 s orient 310238 400 s orient 314= 323 100 s
278.9 ks
Resolution = 0.06”/pixel
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de Mello, Wadadekar, Casertano, Gardner 2005 (submitted)
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Photometric Redshifts
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Templates: early- to late-type Coleman et al.Starbursts Kinney et al.
E Sbc Scd
Im Starburst Starburst
Dahlen et al. 2005, Mobasher et al. 2004
Coleman et al. 80, Kinney et al. 96
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Results – GOODS shallow U-band
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E Sbc Scd Im Sb1 Sb2
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E Sbc Scd Im Sb1 Sb2
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Gallery of starbursts with spectroscopicredshifts:
Late-types, Interacting, Tidal tails,Compacts,tadpoles
zphot=0.36 zphot=0.42 zphot=0.57
zphot=1.12 zphot=0.55 zphot=0.69
zphot=0.7 zphot=1.12 zphot=1.31
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Results – GOODS shallow U-band
• 35% are starbursts (81/227 – 43 stars)
• 75% of starbursts have tidal tails or peculiarities/interaction
• 50% of starbursts have another galaxy within 5x5”
• 36% of starbursts show tadpole morphology
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Blue are starbursts Circles HDF-N Triangles CDF-S
Luminous blueCompact galsBlue nucleated,Compact narrowemission line,Small blue galsBershady etal 00
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Blue are starbursts Circles HDF-N Triangles CDF-S
Bluest are mostly Starbursts, #2 is Im
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BluestObjects
CompactsTidal tailsTadpolesBut...
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BluestObjects
CompactsTidal tailsTadpolesBut...Are we lookingat the SFregion shapeor overallMorphology?
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BluestObjects
CompactsTidal tailsTadpolesBut...Are we lookingat the SFregion shapeor overallMorphology?Is GOODS goodEnough?? Depth Of ACS and WFPC2 enough??
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Results – GOODS deep U-band
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E-Sa
SB1
SB2
1. E2. Sbc3. Scd4. Im5. Starburst 16. Starburst 2
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Cyan 0.2<z<0.6Yellow 0.6<z<0.8Green 0.8<z<1.0Magenta 1.0<z<1.2
Scd/Sdm/IrrSab/SbcE/S0
Locals:
Measured on rest-frame B band
Papovich et al 05
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At 0.8<z<1.2 mostof objects are: -compact, LSB, tadpoles
- Have spectraltypes of starbursts
- and have small and have small sizes rsizes rhh~2kpc~2kpc
LBGs at z~4<rh>~1.7kpcFerguson etal. 2004 – measuredat rest-frame UV1200-2000Å
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Young clusters (Antennae)Intermediate 0.25-1GyrOld Globulars
B-V
V-I
108 – 1010 yr
New Starburst99Vazquez &Leitherer 05
Cyan 0.2<z<0.6Yellow 0.6<z<0.8Green 0.8<z<1.0Magenta 1.0<z<1.2
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• UV-selected galaxies at intermediate-z when seen in redder wavelenghts are:- spirals, peculiars, compact, tadpoles, lsb, and
even early-types ! • Majority of them have spectral types of starbursts,
have neighbors, show signs of interaction. Bluest are compact, tadpole.
• At 0.8<z<1.2 most of UV-selected objects are compact, LSB, blue dots, tadpole, with small sizes rh~2kpc, and spectral types of starbursts.
• When compared to clusters and models, most of the UV-selected have mixed ages ranging from 108 to 1010 yr.
• Next: increase UV sample: GALEX, UDF ACS-UV
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BluestObjects
CompactsTidal tailsTadpolesBut...Are we lookingat the SFregion shapeOr overallMorphology?Is GOODS goodEnough?? Depth Of ACS and WFPC2 problem??
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Zphot=1.28
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Zphot=1.48
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Zphot=1.74
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Local Universe – multiwavelength view (K-correction)
• Late-type (Sc and later) are similar in the optical and UV (star-forming regions dominate).
• Early-type spirals (Sa-Sbc) tend to be classified as later-types in the UV (disk dominates).
• Ellipticals retain smooth profile, but appear more compact.
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Morphological K-correction (ACS/SBC, WFPC2, NICMOS)Teplitz et al. 2005 in preparation
FUV NUV300 I874 H160 FUV NUV300 I874 H160
z0.09
0.321
0.321
0.475
0.555
0.682
HDF-N
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Comparison of Structural Parameters from GOODS and HUDF:
Ravindranath et al. (2005; in preparation)
Triangles are LBGsBlue z=3Green z=4Red z=5
Dots are all galaxies
GOODS depth is goodEnough for bright LBGs
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Results – GOODS shallow U-band
• 95 objects with spectroscopy
• Objects of all types (35% Starbursts)
• 66% of the starbursts have tidal effects and/or close companions, but only
• 33% of the other types have tidal effects
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Cyan 0.2<z<0.6Yellow 0.6<z<0.8Green 0.8<z<1.0Magenta 1.0<z<1.2
LBGs are moreluminous withMB ~ -23 ± 1
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Cyan 0.2<z<0.6Yellow 0.6<z<0.8Green 0.8<z<1.0Magenta 1.0<z<1.2
Scd/Sdm/IrrSab/SbcE/S0
Locals:
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CAS in the ACS
1134 galaxies identified in the ACS field within0.24<z<1.3 RAB<24 – Mobasher et al. 2003
65% are late-types (C=2.65, A=0.27)21% are early-types (C=2.35, A=0.23)14% are starbursts (C=2.53, A=0.33)
UV selected galaxies are on average moreasymmetric (C=2.63, A=0.35)
AAS Atlanta 2004
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Chandra=460 arcmin2
Duilia de Mello
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Which objects cause the decline in the SFR density?
| | | | 8.8 6 3.3 1.6 Gyr
Connolly et al. 97Lilly et al. 96
Fading dwarfs or decline in SF in disks?
Duilia de Mello
Steidel et al. 1999
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Multi-wavelength: B, V, i, z (3700 – 11000 Å)
Multi-epoch: every 45 days (5 epochs)
Area: 316 arcmin2 – two fields
Resolution: 0.03”/pixel – spatial resolution 0”.11
Duilia de Mello
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Models – Starburst99
Vazquez & Leitherer 2005
Young clustersIntermediateOld Globulars
NGC4038/39 Whitmore et al. 99
solar metal.20% solar2% solar
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• 88% of the two GOODS ACS fields
• 741 WFPC2 images: 30 GOODS-S, 25 GOODS-N drizzled images.
• Source Extractor (1.5σ sky threshold – 5 contiguous pixels)
• Match WFPC2 and ACS catalogs (1.5”): 130 objects in the GOODS-S and 138 in the GOODS-N, total of 268 objects
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U-dropouts : LBGs at z = 3
<----------->3"Ravindranath et al. (2005; in preparation)
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V-dropouts : LBGs at z = 5
Ravindranath et al. (2005; in preparation)