The Star Formation History of Galaxies Measured from Individual Pixels. I. The Hubble Deep Field North
arXiv:astro-ph/0307470 · doi:10.1086/378598
Abstract
We analyze the photometric information contained in individual pixels of galaxies in the Hubble Deep Field North (HDFN) using a new technique, _pixel-z_, that combines predictions of evolutionary synthesis models with photometric redshift template fitting. Each spectral energy distribution template is a result of modeling of the detailed physical processes affecting gas properties and star formation efficiency. The criteria chosen to generate the SED templates is that of sampling a wide range of physical characteristics such as age, star formation rate, obscuration and metallicity. A key feature of our method is the sophisticated use of error analysis to generate error maps that define the reliability of the template fitting on pixel scales and allow for the separation of the interplay among dust, metallicity and star formation histories. This technique offers a number of advantages over traditional integrated color studies. As a first application, we derive the star formation and metallicity histories of galaxies in the HDFN. Our results show that the comoving density of star formation rate, determined from the UV luminosity density of sources in the HDFN, increases monotonically with redshift out to at least redshift of 5. This behavior can plausibly be explained by a smooth increase of the UV luminosity density with redshift coupled with an increase in the number of star forming regions as a function of redshift. We also find that the information contained in individual pixels in a galaxy can be linked to its morphological history. Finally, we derive the metal enrichment rate history of the universe and find it in good agreement with predictions based on the evolving HI content of Lyman-alpha QSO absorption line systems.
arXiv commentAccepted for publication in the Astronomical Journal. Full resolution figures available at http://www.stsci.edu/~aconti/pixelz.html
References in corpus (38)
- Star Formation in Galaxies Along the Hubble Sequence
- The Dust Content and Opacity of Actively Star-Forming Galaxies
- High Redshift Galaxies in the Hubble Deep Field. Color Selection and Star Formation History to z=4
- New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
- The Star Formation History of Field Galaxies
- The CANADA-FRANCE REDSHIFT SURVEY XIII: The luminosity density and star-formation history of the Universe to z ~ 1
- The Hubble Deep Field: Observations, Data Reduction, and Galaxy Photometry
- The CANADA-FRANCE REDSHIFT SURVEY VI: Evolution of the galaxy luminosity function to z ~ 1
- Reddening and Star Formation in Starburst Galaxies
- Spectroscopy of Lyman Break Galaxies in the Hubble Deep Field
- The Evolution of the Global Star Formation History as Measured from the Hubble Deep Field
- Autofib Redshift Survey - I. Evolution of the Galaxy Luminosity Function
- The Luminosity Function of Galaxies in the Las Campanas Redshift Survey
- Cosmic Histories of Stars, Gas, Heavy Elements, and Dust
- Evolution of the Galaxy Population Based on Photometric Redshifts in the Hubble Deep Field
- Towards a resolution of the discrepancy between different estimators of star formation rate
- Star-forming galaxies at very high redshifts
- Spectral Classification of Galaxies: An Orthogonal Approach
- Photometric redshifts from evolutionary synthesis with PEGASE: the code ZPEG and the z=0 age constraint
- The Star Formation History of the Hubble Sequence: Spatially Resolved Colour Distributions of Intermediate Redshift Galaxies in the Hubble Deep Field
- The Star Formation Rate Intensity Distribution Function--Implications for the Cosmic Star Formation Rate History of the Universe
- Chemical Properties of Star-Forming Emission Line Galaxies at z=0.1 - 0.5
- The Redshift Distribution and Luminosity Functions of Galaxies in the Hubble Deep Field
- A blind test of photometric redshift prediction
- Spectral Templates from Multicolor Redshift Surveys
- Creating Spectral Templates from Multicolor Redshift Surveys
- Photometric Redshifts of Quasars
- AN IMAGING K-BAND SURVEY - II: THE REDSHIFT SURVEY AND GALAXY EVOLUTION IN THE INFRARED
- The nature of the faint galaxies in the Hubble Deep Field
- Metal Abundances of KISS Galaxies. I. Coarse Metal Abundances and the Metallicity-Luminosity Relation
- A Bayesian Classifier for Photometric Redshifts: Identification of high redshift clusters
- On the compared accuracy and reliability of spectroscopic and photometric redshift measurements
- Photometric redshifts from reconstructed QSO templates
- Cloning Hubble Deep Fields I: A Model-Independent Measurement of Galaxy Evolution
- Cloning Hubble Deep Fields: A Model-Independent Measurement of Galaxy Evolution
- New Improved Photometric Redshifts of Galaxies in the HDF
- Luminosity Density of Galaxies and Cosmic Star Formation Rate from Lambda-CDM Hydrodynamical Simulations
- Quasar Candidates in the Hubble Deep Field
Cited by in corpus (25)
- On the normalisation of the cosmic star formation history
- Galaxy And Mass Assembly: Stellar Mass Estimates
- The Sydney-AAO Multi-object Integral field spectrograph (SAMI)
- Resolved stellar mass maps of galaxies. I: method and implications for global mass estimates
- A census of metals and baryons in stars in the local Universe
- The Dawes Review 8: Measuring the Stellar Initial Mass Function
- The Rapid Decline in Metallicity of Damped Ly-alpha Systems at z~5
- A Groundbased Imaging Study of Galaxies Causing DLA, subDLA, and LLS Absorption in Quasar Spectra
- Star Formation from DLA Gas in the Outskirts of Lyman Break Galaxies at z~3
- The Supernova Relic Neutrino Backgrounds at KamLAND and Super-Kamiokande
- Galaxy Sizes Since from the Perspective of Stellar Mass Distribution within Galaxies
- Spatially Resolved Galaxy Star Formation and its Environmental Dependence I
- The star formation history of damped Lyman alpha absorbers
- Anatomy of a post-starburst minor merger: a multi-wavelength WFC3 study of NGC 4150
- Evidence for Reduced Specific Star Formation Rates in the Centers of Massive Galaxies at z = 4
- Morphological classification of galaxies and its relation to physical properties
- Young, UV-bright Stars Dominate Dust Heating in Star Forming Galaxies
- Removing biases in resolved stellar mass-maps of galaxy disks through successive Bayesian marginalization
- Spatially Resolved Galaxy Star Formation and its Environmental Dependence II. Effect of the Morphology-Density Relation
- Bayesian isochrone fitting and stellar ages
- Hubble Space Telescope Pixel Analysis of the Interacting Face-on Spiral Galaxy NGC 5194 (M51A)
- Unveiling Multiple Physical Processes on a Cluster Galaxy at z=0.3 Using JWST
- Pixel Color-Magnitude Diagram Analysis of the Brightest Cluster Galaxies in Dynamically Young and Old Clusters, Abell 1139 and Abell 2589
- Euclid preparation. Spatially resolved stellar populations of local galaxies with Euclid: a proof of concept using synthetic images with the TNG50 simulation
- Generating on-the-fly large samples of theoretical spectra through N-dimensional grid