[go: up one dir, main page]

Drake et al., 2015 - Google Patents

Evolution of star formation in the UKIDSS Ultra Deep Survey Field–II. Star formation as a function of stellar mass between z= 1.46 and 0.63

Drake et al., 2015

View HTML
Document ID
10530742412266623237
Author
Drake A
Simpson C
Baldry I
James P
Collins C
Ouchi M
Yuma S
Dunlop J
Smith D
Publication year
Publication venue
Monthly Notices of the Royal Astronomical Society

External Links

Snippet

We present new results on the evolution of the cosmic star formation rate as a function of stellar mass in the Subaru/XMM-Newton Deep Survey–Ultra Deep Survey field. We make use of narrow-band-selected emission line galaxies in four redshift slices between z= 1.46 …
Continue reading at academic.oup.com (HTML) (other versions)

Classifications

    • GPHYSICS
    • G06COMPUTING; CALCULATING; COUNTING
    • G06QDATA PROCESSING SYSTEMS OR METHODS, SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES; SYSTEMS OR METHODS SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES, NOT OTHERWISE PROVIDED FOR
    • G06Q50/00Systems or methods specially adapted for a specific business sector, e.g. utilities or tourism
    • G06Q50/10Services
    • G06Q50/20Education
    • GPHYSICS
    • G06COMPUTING; CALCULATING; COUNTING
    • G06QDATA PROCESSING SYSTEMS OR METHODS, SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES; SYSTEMS OR METHODS SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES, NOT OTHERWISE PROVIDED FOR
    • G06Q10/00Administration; Management
    • G06Q10/06Resources, workflows, human or project management, e.g. organising, planning, scheduling or allocating time, human or machine resources; Enterprise planning; Organisational models
    • G06Q10/063Operations research or analysis
    • GPHYSICS
    • G06COMPUTING; CALCULATING; COUNTING
    • G06QDATA PROCESSING SYSTEMS OR METHODS, SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES; SYSTEMS OR METHODS SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES, NOT OTHERWISE PROVIDED FOR
    • G06Q30/00Commerce, e.g. shopping or e-commerce
    • G06Q30/02Marketing, e.g. market research and analysis, surveying, promotions, advertising, buyer profiling, customer management or rewards; Price estimation or determination
    • G06Q30/0202Market predictions or demand forecasting
    • GPHYSICS
    • G06COMPUTING; CALCULATING; COUNTING
    • G06QDATA PROCESSING SYSTEMS OR METHODS, SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES; SYSTEMS OR METHODS SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES, NOT OTHERWISE PROVIDED FOR
    • G06Q50/00Systems or methods specially adapted for a specific business sector, e.g. utilities or tourism
    • G06Q50/01Social networking
    • GPHYSICS
    • G06COMPUTING; CALCULATING; COUNTING
    • G06QDATA PROCESSING SYSTEMS OR METHODS, SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES; SYSTEMS OR METHODS SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES, NOT OTHERWISE PROVIDED FOR
    • G06Q10/00Administration; Management
    • G06Q10/10Office automation, e.g. computer aided management of electronic mail or groupware; Time management, e.g. calendars, reminders, meetings or time accounting
    • GPHYSICS
    • G06COMPUTING; CALCULATING; COUNTING
    • G06QDATA PROCESSING SYSTEMS OR METHODS, SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES; SYSTEMS OR METHODS SPECIALLY ADAPTED FOR ADMINISTRATIVE, COMMERCIAL, FINANCIAL, MANAGERIAL, SUPERVISORY OR FORECASTING PURPOSES, NOT OTHERWISE PROVIDED FOR
    • G06Q40/00Finance; Insurance; Tax strategies; Processing of corporate or income taxes

Similar Documents

Publication Publication Date Title
Saintonge et al. Molecular and atomic gas along and across the main sequence of star-forming galaxies
Popesso et al. The main sequence of star-forming galaxies–I. The local relation and its bending
Bolliet et al. Dark energy constraints from the thermal Sunyaev–Zeldovich power spectrum
Matsuda et al. Diffuse Lyα haloes around Lyα emitters at z= 3: do dark matter distributions determine the Lyα spatial extents?
Magdis et al. On the stellar masses of IRAC detected Lyman Break Galaxies at z∼ 3
Rollinde et al. Sample variance and Lyman α forest transmission statistics
Koprowski et al. A direct calibration of the IRX–β relation in Lyman-break Galaxies at z= 3–5
Narayanan et al. Galaxy gas fractions at high redshift: the tension between observations and cosmological simulations
Miville-Deschênes et al. Herschel-SPIRE observations of the Polaris flare: Structure of the diffuse interstellar medium at the sub-parsec scale
Montero-Dorta et al. The SDSS DR6 luminosity functions of galaxies
Cristiani et al. The spectral slope and escape fraction of bright quasars at z∼ 3.8: the contribution to the cosmic UV background
Popping et al. The inferred evolution of the cold gas properties of CANDELS galaxies at 0.5< z< 3.0
Zhang et al. Estimating the H i gas fractions of galaxies in the local Universe
Buat et al. Measures of star formation rates from infrared (Herschel) and UV (GALEX) emissions of galaxies in the HerMES fields
Lada et al. HP2 survey-III. The California Molecular Cloud: A sleeping giant revisited
Bonavera et al. Statistics of the fractional polarization of compact radio sources in Planck maps
Drake et al. Evolution of star formation in the UKIDSS Ultra Deep Survey Field–II. Star formation as a function of stellar mass between z= 1.46 and 0.63
Efstathiou et al. A simple empirically motivated template for the thermal Sunyaev–Zel’dovich effect
Guo et al. The Milky Way system in Λ cold dark matter cosmological simulations
Ho A machine learning artificial neural network calibration of the strong-line oxygen abundance
Guimaraes et al. Evidence for overdensity around z em> 4 quasars from the proximity effect
Bernhard et al. Modelling the connection between ultraviolet and infrared galaxy populations across cosmic times
Grand et al. Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way
Ellison et al. The infrared luminosities of∼ 332 000 SDSS galaxies predicted from artificial neural networks and the Herschel Stripe 82 survey
DeGraf et al. Early black holes in cosmological simulations: luminosity functions and clustering behaviour