Finding the UV-Visible Path Forward: Proceedings of the Community Workshop to Plan the Future of UV/Visible Space Astrophysics
arXiv:1611.09736 · doi:10.1088/1538-3873/129/977/076001
Abstract
We present the science cases and technological discussions that came from the workshop entitled "Finding the UV-Visible Path Forward" held at NASA GSFC June 25-26, 2015. The material presented outlines the compelling science that can be enabled by a next generation space-based observatory dedicated for UV-visible science, the technologies that are available to include in that observatory design, and the range of possible alternative launch approaches that could also enable some of the science. The recommendations to the Cosmic Origins Program Analysis Group from the workshop attendees on possible future development directions are outlined.
Proceedings from Workshop held in June 2015 at NASA GSFC on the Future of UV Astronomy from Space
References in corpus (77)
- Cosmic Star Formation History
- How Do Galaxies Get Their Gas?
- Cosmic Reionization and Early Star-Forming Galaxies: A Joint Analysis of New Constraints from Planck and Hubble Space Telescope
- Radiative Transfer in a Clumpy Universe: III. The Nature of Cosmological Ionizing Sources
- The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years
- The COS-Halos Survey: Physical Conditions and Baryonic Mass in the Low-Redshift Circumgalactic Medium
- The Large, Oxygen-Rich Halos of Star-Forming Galaxies Are A Major Reservoir of Galactic Metals
- Large-scale magnetic topologies of mid-M dwarfs
- The Effect of a Strong Stellar Flare on the Atmospheric Chemistry of an Earth-like Planet Orbiting an M dwarf
- Evidence for Ubiquitous Collimated Galactic-Scale Outflows along the Star-Forming Sequence at z~0.5
- Galaxies at z~6: The UV Luminosity Function and Luminosity Density from 506 UDF, UDF-Ps, and GOODS i-dropouts
- The number density and mass density of star-forming and quiescent galaxies at 0.4 < z < 2.2
- A Budget and Accounting of Metals at z~0: Results from the COS-Halos Survey
- Photochemistry in Terrestrial Exoplanet Atmospheres I: Photochemistry Model and Benchmark Cases
- Spectral Evolution of an Earth-Like Planet
- Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-Line Spectroscopy
- The Stellar Mass Density and Specific Star Formation Rate of the Universe at z~7
- The Ultraviolet Radiation Environment Around M dwarf Exoplanet Host Stars
- The COS-Dwarfs Survey: The Carbon Reservoir Around sub-L* Galaxies
- The escape of heavy atoms from the ionosphere of HD209458b. I. A photochemical-dynamical model of the thermosphere
- Discovery and Characterization of Transiting SuperEarths Using an All-Sky Transit Survey and Follow-up by the James Webb Space Telescope
- The Bimodal Metallicity Distribution of the Cool Circumgalactic Medium at z<1
- The GALEX-VVDS Measurement of the Evolution of the 1500A Luminosity Function
- Abiotic Ozone and Oxygen in Atmospheres Similar to Prebiotic Earth
- The Fate of the First Galaxies. II. Effects of Radiative Feedback
- The Intrinsic Extreme Ultraviolet Fluxes of F5 V to M5 V Stars
- The Antennae Galaxies (NGC 4038/4039) Revisited: ACS and NICMOS Observations of a Prototypical Merger
- Star formation rates and stellar masses of z=7-8 galaxies from IRAC observations of the WFC3/IR ERS and the HUDF field
- High Stellar FUV/NUV Ratio and Oxygen Contents in the Atmospheres of Potentially Habitable Planets
- On the Escape of Ionizing Radiation from Starbursts
- Tracing Inflows and Outflows with Absorption Lines in Circumgalactic Gas
- Detection of Elements at All Three r-process Peaks in the Metal-Poor Star HD 160617
- The impact of feedback on cosmological gas accretion
- HAZMAT I: The Evolution of Far-UV and Near-UV Emission from Early M Stars
- The Hidden Mass and Large Spatial Extent of a Poststarburst Galaxy Outflow
- Biosignature Gases in H2-Dominated Atmospheres on Rocky Exoplanets
- Origin and Loss of nebula-captured hydrogen envelopes from "sub"- to "super-Earths" in the habitable zone of Sun-like stars
- Not Dead Yet: Cool Circumgalactic Gas in the Halos of Early Type Galaxies
- A superconducting focal plane array for ultraviolet, optical, and near-infrared astrophysics
- An Accounting of the Dust-Obscured Star Formation and Accretion Histories Over the Last ~11~Billion Years
- Evidence for a Massive, Extended Circumgalactic Medium Around the Andromeda Galaxy
- A comparison between star formation rate diagnostics and rate of core collapse supernovae within 11 Mpc
- The Extended Hubble Space Telescope Supernova Survey: The Rate of Core Collapse Supernovae to z~1
- Primary and secondary eclipse spectroscopy with JWST: exploring the exoplanet parameter space
- The GALEX Arecibo SDSS survey: III. Evidence for the Inside-Out Formation of Galactic Disks
- Polarized reflected light from the exoplanet HD189733b: First multicolor observations and confirmation of detection
- A Monte Carlo simulation of the intergalactic absorption and the detectability of the Lyman continuum from distant galaxies
- Transmission spectrum of Earth as a transiting exoplanet - from the ultraviolet to the near-infrared
- The Extended Star Formation History of the Andromeda Spheroid at 35 Kpc on the Minor Axis
- Spatially Resolved Velocity Maps of Halo Gas Around Two Intermediate-redshift Galaxies
- Gas Accretion is Dominated by Warm Ionized Gas in Milky Way-Mass Galaxies at z ~ 0
- Low-metallicity Absorbers Account for Half of the Dense Circumgalactic Gas at z < 1
- Fluctuations and Flares in the Ultraviolet Line Emission of Cool Stars: Implications for Exoplanet Transit Observations
- An IMF Study of the Dwarf Starburst Galaxy NGC 4214
- Winds of low-metallicity OB-type stars: HST-COS spectroscopy in IC1613
- Non-Detection of Polarized, Scattered Light from the HD 189733b Hot Jupiter
- The Location of the Nucleus of NGC 1068 and the Three-dimensional Structure of Its Nuclear Region
- No breakdown of the radiatively-driven wind theory in low-metallicity environments
- On the Mass-Loss Rates of Massive Stars in the Low-Metallicity Galaxies IC 1613, WLM and NGC 3109
- A Method for Measuring Variations in the Stellar Initial Mass Function
- HST/COS Spectra of Three QSOs That Probe The Circumgalactic Medium of a Single Spiral Galaxy: Evidence for Gas Recycling and Outflow
- Paramagnetic alignment of small grains: a novel method for measuring interstellar magnetic fields
- Atomic alignment and Diagnostics of Magnetic Fields in Diffuse Media
- Effects of stellar rotation on star formation rates and comparison to core-collapse supernova rates
- Big Fish in Small Ponds: Massive Stars in the Low Mass Clusters of M83
- V444 Cyg X-ray and polarimetric variability: Radiative and Coriolis forces shape the wind collision region
- UV Extinction Towards a Quiescent Molecular Cloud in the SMC
- How the diffuse Universe cools
- The History of Star Formation in Galaxy Disks in the Local Volume as Measured by the ACS Nearby Galaxy Survey Treasury
- The Kinematics of CIV in Star-Forming Galaxies at z~1.2
- The high-field polar RX J1007.5-2017
- UVMag: stellar formation, evolution, structure and environment with space UV and visible spectropolarimetry
- Building galaxies, stars, planets and the ingredients for life between the stars. A scientific proposal for a European Ultraviolet-Visible Observatory (EUVO)
- Cosmic Dawn: Studies of the Earliest Galaxies and Their Role in Cosmic Reionization
- Scientific Objectives for UV/Visible Astrophysics Investigations: A Summary of Responses by the Community (2012)
- Project Lyman
- Project Lyman: Quantifying 11 Gyrs of Metagalactic Ionizing Background Evolution
Cited by in corpus (4)
- Conditions for Reionizing the Universe with A Low Galaxy Ionizing Photon Escape Fraction
- The World Space Observatory Ultraviolet (WSO-UV), as a bridge to future UV astronomy
- The Polstar High Resolution Spectropolarimetry MIDEX Mission
- CHESS: an Innovative Concept for High-Resolution, Far-UV Spectroscopy