EROS and MACHO Combined Limits on Planetary Mass Dark Matter in the Galactic Halo
arXiv:astro-ph/9803082 · doi:10.1086/311355
Abstract
The EROS and MACHO collaborations have each published upper limits on the amount of planetary mass dark matter in the Galactic Halo obtained from gravitational microlensing searches. In this paper the two limits are combined to give a much stronger constraint on the abundance of low mass MACHOs.
8 pages, 4 figures, submitted to ApJ Letters
References in corpus (2)
Cited by in corpus (131)
- The James Webb Space Telescope
- Direct Imaging of Multiple Planets Orbiting the Star HR 8799
- New cosmological constraints on primordial black holes
- Primordial Black Holes as Dark Matter
- The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations
- Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds
- Massive Primordial Black Holes from Hybrid Inflation as Dark Matter and the seeds of Galaxies
- Gravitational wave background as a probe of the primordial black hole abundance
- Effect of Primordial Black Holes on the Cosmic Microwave Background and Cosmological Parameter Estimates
- MACHO Project Limits on Black Hole Dark Matter in the 1-30 Solar Mass Range
- Extragalactic Results from the Infrared Space Observatory
- Galactic Searches for Dark Matter
- Constraints on primordial black holes as dark matter candidates from capture by neutron stars
- Gravitational waves at interferometer scales and primordial black holes in axion inflation
- Testing LMC Microlensing Scenarios: The Discrimination Power of the SuperMACHO Microlensing Survey
- Generalised constraints on the curvature perturbation from primordial black holes
- Microlensing and dynamical constraints on primordial black hole dark matter with an extended mass function
- The Tensor-Vector-Scalar theory and its cosmology
- Experimental Limits on Primordial Black Hole Dark Matter from the First Two Years of Kepler Data
- The End of the MACHO Era: Limits on Halo Dark Matter from Stellar Halo Wide Binaries
- The Monitor project: Rotation of low-mass stars in the open cluster NGC 2516
- Constraints on the induced gravitational wave background from primordial black holes
- Extra-Solar Planets
- Primordial Black Holes as Dark Matter: Almost All or Almost Nothing
- Subaru through a different lens: microlensing by extended dark matter structures
- Black Hole Metamorphosis and Stabilization by Memory Burden
- Binary Microlensing Events from the MACHO Project
- A 5D view of the Alpha Per, Pleiades, and Praesepe clusters
- Rotation of Late-Type Stars in Praesepe with K2
- Coronagraphic Survey for Companions of Stars within 8 pc
- Primordial black holes dark matter from inflection point models of inflation and the effects of reheating
- Limits on the Mass and Abundance of Primordial Black Holes from Quasar Gravitational Microlensing
- Gravitational microlensing by dark matter in extended structures
- Primordial black holes as dark matter and gravitational waves from bumpy axion inflation
- Constraining Primordial Black-Hole Bombs through Spectral Distortions of the Cosmic Microwave Background
- TeVeS Cosmology : Covariant formalism for the background evolution and linear perturbation theory
- Variability of the Infrared Excess of Extreme Debris Disks
- Tidal capture of a primordial black hole by a neutron star: implications for constraints on dark matter
- Stellar activity with LAMOST. I. Spot configuration in Pleiades
- Probing Dark Matter Substructure with Pulsar Timing
- Theory of pixel lensing towards M31 I: the density contribution and mass of MACHOs
- A new detailed examination of white dwarfs in NGC3532 and NGC2287
- Gravastars with higher dimensional spacetimes
- Rotation periods for very low mass stars in the Pleiades
- Discovery and Characterization of a Caustic Crossing Microlensing Event in the SMC
- Search for Small-Mass Black Hole Dark Matter with Space-Based Gravitational Wave Detectors
- Observation of Microlensing towards the Galactic Spiral Arms. EROS II 3 year survey
- Searching for primordial black hole dark matter with pulsar timing arrays
- Adiabatic contraction revisited: implications for primordial black holes
- The lithium depletion boundary and the age of NGC 2547
- No observational constraints from hypothetical collisions of hypothetical dark halo primordial black holes with galactic objects
- Getting the astrophysics and particle physics of dark matter out of next-generation direct detection experiments
- New Constraints on Macroscopic Compact Objects as a Dark Matter Candidate from Gravitational Lensing of Type Ia Supernovae
- Search for Kilogram-scale Dark Matter with Precision Displacement Sensors
- Applications of Microlensing to Stellar Astrophysics
- Cosmological implications of Primordial Black Holes
- The first direct detection of a gravitational micro-lens toward the Galactic bulge
- Background discrimination capabilities of a heat and ionization germanium cryogenic detector
- Gravitational Waves from Sub-lunar Mass Primordial Black Hole Binaries - A New Probe of Extradimensions
- Exploring the astrophysics of dark atoms
- Microlensing of Kepler Stars as a Method of Detecting Primordial Black Hole Dark Matter
- Chemical Abundances in the Secondary Star of the Neutron Star Binary Centaurus X-4
- Transient solar oscillations driven by primordial black holes
- Confirmation of Planet-Mass Objects in Extragalactic Systems
- Observational Constraints on the Primordial Curvature Power Spectrum
- Using LISA-like Gravitational Wave Detectors to Search for Primordial Black Holes
- Can Microlensing Explain the Long-Term Optical Variability of Quasars?
- Microlensing constraints on axion stars including finite lens and source size effects
- Physics Beyond the Standard Model and Dark Matter
- Detectable seismic consequences of the interaction of a primordial black hole with Earth
- The Red Halo Phenomenon
- Mesolensing Explorations of Nearby Masses: From Planets to Black Holes
- A near-infrared survey for new low-mass members in Alpha Per
- Simple Cosmological Solution to the Higgs Instability Problem in the Chaotic Inflation and Formation of Primordial Black Holes
- A framework for the next generation of stationary cosmological models
- Short-timescale Fluctuations in the Difference Light Curves of QSO 0957+561A,B: Microlensing or Noise?
- Light weakly interacting massive particles
- Detecting the gravitational wave background from primordial black hole dark matter
- Constraining the properties of spots on Pleiades very low mass stars
- Phenomenological study of neutrino mass, dark matter and baryogenesis within the framework of minimal extended seesaw
- The stellar mass to light ratio in the isolated spiral NGC 4414
- Constraints on Cold H_2 Clouds from Gravitational Microlensing Searches
- Constraining axion and compact dark matter with interstellar medium heating
- Interacting black holes on the brane: the seeding of binaries
- Not enough stellar mass Machos in the Galactic halo
- Snowmass-2013 Cosmic Frontier 3 (CF3) Working Group Summary: Non-WIMP dark matter
- Exploring the planetary-mass population in the Upper Scorpius association
- A Reanalysis of Public Galactic Bulge Gravitational Microlensing Events from OGLE-III and IV
- Re-examination of the possible tidal stream in front of the LMC
- The dark halo of the main lens galaxy in QSO 0957+561
- Unambiguous quasar microlensing
- Photometric Confirmation of MACHO Large Magellanic Cloud Microlensing Events
- A Distant Sample of Halo Wide Binaries from SDSS
- The Cloudy Universe
- Cosmological implications of a Dark Matter self-interaction energy density
- Microlensing signatures of extended dark objects using machine learning
- Gravipulsons
- Schrödinger equation in a general curved space-time geometry
- New Light on Dark Extended Lenses with the Roman Space Telescope
- Gravitational wave constraints on extended dark matter structures
- Interpreting the M22 Spike Events
- The Dark Matter problem
- Repository for extended dark matter object constraints
- Detecting Dark Compact Objects in Gaia DR4: A Data Analysis Pipeline for Transient Astrometric Lensing Searches
- Nanolensing of gamma-ray bursts
- Improved Theoretical Predictions of Microlensing Rates for the Detection of Primordial Black Hole Dark Matter
- Gravitational hydrodynamics of large scale structure formation
- The Galactic Halo from Microlensing
- Cosmic microwave background constraints on extended dark matter objects
- Neutron Stars and Black Holes as MACHOs
- Search for the sub-stellar lithium depletion boundary in the open star cluster Coma Berenices
- Non-collider searches for stable massive particles
- Outlook: The Next Twenty Years
- Stochastic gravitational wave background from accreting primordial black hole binaries during early inspiral stage
- Passage of test particles through oscillating spherically-symmetric dark matter configurations
- Dark Classification Matters: Searching for Primordial Black Holes with LSST
- Microlensing planets in M22: free-floating or bound?
- Model for common growth of supermassive black holes, bulges and globular star clusters: ripping off Jeans clusters
- Dark haloes as seen with gravitational lensing
- Free-floating "planets'' in the macrolensed quasar Q2237+0305
- Observations from Australasia using the Gravitational Microlensing Technique
- The Brown Dwarf Mass Function from Pixel Microlensing
- Fluid Mechanics Explains Cosmology, Dark Matter, Dark Energy, and Life
- Chameleon Gravity as an Alternative to Dark Matter
- Detecting cold H2 globules in the outer Galactic disc by microlensing towards the Maffei 1 elliptical
- Primordial Planet Formation
- Prospects for Reconstructing the Free-floating Planet Mass Function at the Population Level with the Nancy Grace Roman Space Telescope
- A new probe of dark matter-baryon interactions in compact stellar systems
- Theoretical and phenomenological consequences of active and sterile neutrino within Beyond Standard Model framework
- A partially occulting MACHO-microlensing event in the Twin Quasar Q0957+561
- Two close binaries across the hydrogen-burning limit in the Praesepe open cluster