A GALEX and NDWFS Investigation of Star Forming Galaxies at z=1 and 2
description
Transcript of A GALEX and NDWFS Investigation of Star Forming Galaxies at z=1 and 2
A GALEX and NDWFS Investigation of Star Forming
Galaxies at z=1 and 2
Charles G. Hoopes, Timothy M. Heckman (JHU)
Buell T. Jannuzi, Arjun Dey, Michael J. I. Brown, Alison Ford (NOAO)
and Davis Schiminovich (Columbia)
June 2, 2004
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
The Galaxy Evolution Explorer (GALEX)
• Launched April 28, 2003• Imaging in two UV bands
– FUV: λ=1516Å, Δλ=268Å– NUV: λ=2267Å, Δλ=732Å– Spatial resolution ~5”– FOV ~1.2 deg2
• Slitless Spectroscopy– 1350-2800Å– Spectral resolution R=80-300
• Conducting several surveys of varying depth and area, as well as pointed observations
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
Mapping the History of Star Formation in the Universe
• SF history of universe mapped out to z>5
• Relatively little known about z<3
• Different techniques used for different redshift intervals
(From Giavalisco 2002 and Barger et al 2000)
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
Lyman Break Galaxies at z>3: U-band dropouts
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
Lyman Break Galaxies at z>3: U-band dropouts
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
GALEX Observations of Bootes Region• Deep Imaging Survey
– 80 deg2, including the 9 deg2 Bootes region of the NDWFS.
– Limiting magnitude AB=25– 1 deg2 observed in 2003 (the “00” field - 43 ksec)– 2 more deg2 coming this week
• Ultra-Deep Imaging Survey– 4 deg2, including the “00” field in Bootes– Limiting magnitude AB=26– 200 ksec planned (100 in 2004)
• Deep Spectroscopic Survey– 2 deg2, including the “00” field– Limiting magnitude AB=22.5-24
Supplemented NDWFS data with deep Uobservations (AB=26) in the “00” field
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
z=1: FUV Dropouts
• SExtractor (Bertin & Arnouts 1996) dual band catalog in NUV/FUV matched with U-band
• Spatial resolution difference (~5” for GALEX, <1” for U-band) creates identification problems
• Compare colors to model colors of redshifted starburst spectra (following Steidel et al.)
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
z=2: NUV Dropouts
• SExtractor single-band catalogs matched in Bw, U, NUV
• Spatial resolution problems remains
• Compare colors to model colors of redshifted starburst spectra (following Steidel et al.)
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
UV Luminosity• Luminosities calculatedfrom filter redward of Lyman break
• Fainter z=2 galaxiesselected against, but bright z=1 galaxies wouldbe detected
• Indicates that most luminous galaxies at z=2 have faded by z=1
L* at z=0 from Treyer et al. 2004 in GALEX edition of APJLL* for LBGs from Giavalisco 2002
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
Star Formation and Extinction
• We may be seeing the transition in star formationrates from LBGs to present-daystarbursts(see also Arnouts et al. 2004 inGALEX edition of ApJL)• Mean extinction implied byUV slope isE(B-V)~0.1 for z=1E(B-V)~0.2 for z=2
(but there is a degeneracy between redshift and UV slope,and only sensitive to E(B-V)<0.4)
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
Future Work
• Improved matching techniques, photo-z
• Further GALEX observations
• Spitzer observations of this region are planned
• Spectroscopic follow up
June 2, 2004 GALEX-NDWFS Investigation of Galaxies at z=1-2
Summary
• GALEX-NDWFS collaboration will shed light on galaxy evolution at z=1-2
• Large amount of GALEX data in the Bootes region is coming
• Initial results show the vigorous star formation of Lyman Break Galaxies fading from z=2 to z=1