Science Impacts of the SPHEREx All-Sky Optical to Near-Infrared Spectral Survey II: Report of a Community Workshop on the Scientific Synergies Between the SPHEREx Survey and Other Astronomy Observatories
arXiv:1805.05489
Abstract
SPHEREx is a proposed NASA MIDEX mission selected for Phase A study. SPHEREx would carry out the first all-sky spectral survey in the near infrared. At the end of its two-year mission, SPHEREx would obtain 0.75-to-5m spectra of every 6.2 arcsec pixel on the sky, with spectral resolution R>35 and a 5- sensitivity AB19 per spectral/spatial resolution element. More details concerning SPHEREx are available at http://spherex.caltech.edu. The SPHEREx team has proposed three specific science investigations to be carried out with this unique data set: cosmic inflation, interstellar and circumstellar ices, and the extra-galactic background light. Though these three themes are undoubtedly compelling, they are far from exhausting the scientific output of SPHEREx. Indeed, SPHEREx would create a unique all-sky spectral database including spectra of very large numbers of astronomical and solar system targets, including both extended and diffuse sources. These spectra would enable a wide variety of investigations, and the SPHEREx team is dedicated to making the data available to the community to enable these investigations, which we refer to as Legacy Science. To that end, we have sponsored two workshops for the general scientific community to identify the most interesting Legacy Science themes and to ensure that the SPHEREx data products are responsive to their needs. In February of 2016, some 50 scientists from all fields met in Pasadena to develop these themes and to understand their implications for the SPHEREx mission. The 2016 workshop highlighted many synergies between SPHEREx and other contemporaneous astronomical missions, facilities, and databases. Consequently, in January 2018 we convened a second workshop at the Center for Astrophysics in Cambridge to focus specifically on these synergies. This white paper reports on the results of the 2018 SPHEREx workshop.
arXiv comment50 pages, 24 figures, more details at http://spherex.caltech.edu
Cited by in corpus (36)
- Data Analysis for Precision 21 cm Cosmology
- Accurate precision Cosmology with redshift unknown gravitational wave sources
- The eROSITA Final Equatorial-Depth Survey (eFEDS): Identification and characterization of the counterparts to the point-like sources
- The GIGANTES dataset: precision cosmology from voids in the machine learning era
- SPHEREx: NASA's Near-Infrared Spectrophotmetric All-Sky Survey
- Astrophysics & Cosmology from Line Intensity Mapping vs Galaxy Surveys
- Signatures of primordial black holes in gravitational wave clustering
- Extracting bias using the cross-bispectrum: An EoR and 21 cm-[CII]-[CII] case study
- DEMNUni: disentangling dark energy from massive neutrinos with the void size function
- The universal multiplicity function: counting halos and voids
- Identification of AKARI infrared sources by Deep HSC Optical Survey: Construction of New Band-Merged Catalogue in the NEP-Wide field
- Cosmic Near-infrared Background Tomography with SPHEREx Using Galaxy Cross-correlations
- Mid-infrared Variability of Low-redshift Active Galactic Nuclei : Constraints on a Hot Dust Component with a Variable Covering Factor
- Measuring Model-independent Masses and Radii of Single-Lined Eclipsing Binaries: Analytic Precision Estimates
- Fundamental physics using the temporal gravitational wave background
- Mitigating the noise of DESI mocks using analytic control variates
- Constraining extended cosmologies with GWLSS cross-correlations
- A new probe of the high-redshift Universe: nulling CMB lensing with interloper-free "LIM-pair" lensing
- How Gaussian can the Sky be? Primordial Non-Gaussianity from Quantum Information
- Warm inflation with a heavy QCD axion
- Deep learning reconstruction of three-dimensional galaxy distributions with intensity mapping observations
- Estimating the Feasibility of 21cm-Ly Synergies using the Hydrogen Epoch of Reionization Array
- Small Bodies Science with Twinkle
- The HalfDome Multi-Survey Cosmological Simulations: N-body Simulations
- Flat-sky Angular Power Spectra Revisited
- Euclid preparation. XXXIV. The effect of linear redshift-space distortions in photometric galaxy clustering and its cross-correlation with cosmic shear
- Baryon acoustic oscillations from HI intensity mapping: the importance of cross-correlations in the monopole and quadrupole
- Massive s through the CNN lens: interpreting the field-level neutrino mass information in weak lensing
- The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
- A Mid-infrared Flare in the Seyfert Galaxy NGC 3786: A Changing-look Event Triggered by an Obscured Tidal Disruption Event?
- Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
- Evolution of Dust and Water Ice in Cometary Comae by Radiative Torques
- Escape from the swamp with spectator
- Searching for axion-like particles with SPHEREx
- Euclid: Constraining ensemble photometric redshift distributions with stacked spectroscopy
- Testing the growth of cosmic structures during the Dark Ages