The Pristine survey XXVIII. Journey to the Galactic outskirts: Mapping the outer halo red giant stars down to the very metal-poor end
arXiv:2408.17250 · doi:10.1051/0004-6361/202452073
Abstract
Context: In the context of Galactic archaeology, the outer halo remains relatively unexplored with respect to its metallicity distribution, merger debris, and the abundance of known very/extremely metal-poor ([Fe/H]<-2.5) stars. Aim: We utilize the Pristine survey's publicly available, Pristine data release 1 (PDR1) and Pristine-Gaia synthetic (PGS) catalogues of photometric metallicities, to select Red Giant Branch (RGB) stars in the outer halo. Methods: The RGB selection pipeline selects giants based on the absence of a well-measured parallax in the brightness range where dwarfs have reasonable parallax estimate from Gaia DR3 data. The photometric distances are calculated using a BaSTI-isochrone fitting code and the photometric metallicities. Results: Photometric distances derived from PDR1- and PGS-giants show typical uncertainties of 12% and a scatter of up to 20% and 40% respectively, when validated against inverted-parallax and Starhorse-code distances. The PDR1-giants catalogue provides a low-to-no bias view of the metallicity structure versus distance compared to the PGS-giants catalogue (with a distance-metallicity selection bias), while the PGS-giants catalogue provides an all-sky view of the outer halo, especially in the VMP end. The PDR1-giants catalogue is used to study the metallicity distribution function of the halo out to ~100 kpc, using Gaussian Mixture Model decomposition. Additionally, we use the PDR1-giants with radial velocities from spectroscopic surveys to map the metallicity view of the integrals-of-motion space where accreted dwarf galaxy debris conserve their orbital parameters for a long time. Using the PGS-giants catalogue, we associate 41 stars tentatively to the stellar counterpart of the Magellanic stream in the VMP end, out to 70 kpc. Conclusions: We publish two RGB catalogues between -4.0<[Fe/H]<+0.1 with reliable photometric distances and metallicities.
arXiv commentPublished version. Pristine DR1 and Pristine-Gaia synthetic catalogues of red giants are available at the CDS via https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/706/A195
References in corpus (145)
- XGBoost: A Scalable Tree Boosting System
- The NumPy array: a structure for efficient numerical computation
- The Sloan Digital Sky Survey: Technical Summary
- On the variation of the Initial Mass Function
- The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package
- PARSEC: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code
- Gaia Data Release 3: Summary of the content and survey properties
- MESA Isochrones and Stellar Tracks (MIST). I: Solar-Scaled Models
- Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3
- MESA Isochrones and Stellar Tracks (MIST) 0: Methods for the construction of stellar isochrones
- Local Kinematics and the Local Standard of Rest
- The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems
- The Apache Point Observatory Galactic Evolution Experiment (APOGEE)
- Estimating distances from parallaxes IV: Distances to 1.33 billion stars in Gaia Data Release 2
- A large stellar evolution database for population synthesis studies. I. Scaled solar models and isochrones
- The merger that led to the formation of the Milky Way's inner stellar halo and thick disk
- SEGUE: A Spectroscopic Survey of 240,000 stars with g=14-20
- The mass distribution and gravitational potential of the Milky Way
- The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey
- Tracing Galaxy Formation with Stellar Halos I: Methods
- Co-formation of the Galactic disc and the stellar halo
- Gaia Early Data Release 3: Parallax bias versus magnitude, colour, and position
- Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole
- The Radial Velocity Experiment (RAVE): first data release
- Gaia Early Data Release 3: Photometric content and validation
- Stellar Chemical Signatures And Hierarchical Galaxy Formation
- Kinematics of Metal-Poor Stars in the Galaxy. III. Formation of the Stellar Halo and Thick Disk as Revealed from a Large Sample of Non-Kinematically Selected Stars
- Two Stellar Components in the Halo of the Milky Way
- The GALAH+ Survey: Third Data Release
- Debris streams in the solar neighbourhood as relicts from the formation of the Milky Way
- The Milky Way Tomography with SDSS: II. Stellar Metallicity
- Two distinct halo populations in the solar neighborhood. Evidence from stellar abundance ratios and kinematics
- AGAMA: Action-based galaxy modelling architecture
- Near-Field Cosmology with Metal-Poor Stars
- A stellar relic from the early Milky Way
- Evidence for Two Early Accretion Events That Built the Milky Way Stellar Halo
- Structure and Kinematics of the Stellar Halos and Thick Disks of the Milky Way Based on Calibration Stars from SDSS DR7
- Building up the Stellar Halo of the Galaxy
- The Stellar Abundances for Galactic Archeology (SAGA) Database - Compilation of the Characteristics of Known Extremely Metal-Poor Stars
- Evidence from the H3 Survey that the Stellar Halo is Entirely Comprised of Substructure
- The Role of Dwarf Galaxy Interactions in Shaping the Magellanic System and Implications for Magellanic Irregulars
- The Updated BaSTI Stellar Evolution Models and Isochrones: I. Solar Scaled Calculations
- The Proper Motion of the Large Magellanic Cloud using HST
- The Milky Way stellar halo out to 40 kpc : Squashed, broken but smooth
- The Biggest Splash
- The Magellanic Stream, High-Velocity Clouds and the Sculptor Group
- Tango for three: Sagittarius, LMC, and the Milky Way
- Stars beyond Galaxies: The Origin of Extended Luminous Halos around Galaxies
- Is the SMC Bound to the LMC? The HST Proper Motion of the SMC
- The Origin of the Magellanic Stream and Its Leading Arm
- The birth of the Milky Way as uncovered by accurate stellar ages with Gaia
- The Pristine survey I: Mining the Galaxy for the most metal-poor stars
- Multiple retrograde substructures in the Galactic halo: A shattered view of Galactic history
- Mapping the substructure in the Galactic halo with the next generation of astrometric satellites
- The PASTEL catalogue: 2016 version
- Gaia Data Release 3: Processing and validation of BP/RP low-resolution spectral data
- The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
- From dawn till disk: Milky Way's turbulent youth revealed by the APOGEE+Gaia data
- Gaia reveals a metal-rich in-situ component of the local stellar halo
- Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud
- Chemical Evolution in Hierarchical Models of Cosmic Structure II: The Formation of the Milky Way Stellar Halo and the Distribution of the Oldest Stars
- Ghostly Tributaries to the Milky Way: Charting the Halo's Stellar Streams with the Gaia DR2 catalogue
- Gaia Data Release 3: External calibration of BP/RP low-resolution spectroscopic data
- One large blob and many streams frosting the nearby stellar halo in Gaia DR2
- Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud
- The Shape and Profile of the Milky Way Halo as Seen by the CFHT Legacy Survey
- The Hercules-Aquila Cloud
- The Global Dynamical Atlas of the Milky Way mergers: Constraints from Gaia EDR3 based orbits of globular clusters, stellar streams and satellite galaxies
- The -Process Alliance: First Release from the Southern Search for -Process-Enhanced Stars in the Galactic Halo
- Where are the most ancient stars in the Milky Way?
- Mapping the Stellar Halo with the H3 Spectroscopic Survey
- Overview of the DESI Milky Way Survey
- Dynamical Relics of the Ancient Galactic Halo
- Formation of In Situ Stellar Haloes in Milky Way-Mass Galaxies
- Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra
- The chemical characterisation of halo substructure in the Milky Way based on APOGEE
- The shape of the Galactic halo with DR2 RR Lyrae. Anatomy of an ancient major merger
- The radial profile and flattening of the Milky Way's stellar halo to kpc from the SEGUE K-giant Survey
- The Stellar Metallicity Distribution Function of the Galactic Halo from SDSS Photometry
- Elemental Abundances and their Implications for the Chemical Enrichment of the Boötes~I Ultra-Faint Galaxy
- Quantifying the impact of the Large Magellanic Cloud on the structure of the Milky Way's dark matter halo using Basis Function Expansions
- The Overdensity in Virgo, Sagittarius Debris, and the Asymmetric Spheroid
- The Southern Stellar Stream Spectroscopic Survey (): Overview, Target Selection, Data Reduction, Validation, and Early Science
- The Poor Old Heart of the Milky Way
- Resolving the Metallicity Distribution of the Stellar Halo with the H3 Survey
- All-Sky Dynamical Response of the Galactic Halo to the Large Magellanic Cloud
- Timing the Early Assembly of the Milky Way with the H3 Survey
- Mapping the Galactic Halo VIII: Quantifying substructure
- StarHorse results for spectroscopic surveys + Gaia DR3: Chrono-chemical populations in the solar vicinity, the genuine thick disk, and young-alpha rich stars
- The Pristine survey X: a large population of low-metallicity stars permeates the Galactic disk
- The oldest and most metal poor stars in the APOSTLE Local Group simulations
- Vaex: Big Data exploration in the era of Gaia
- The Pristine Survey IV: Approaching the Galactic metallicity floor with the discovery of an ultra metal-poor star
- The Gaia DR3 view of dynamical substructure in the stellar halo near the Sun
- GASTRO library I: the simulated chemodynamical properties of several GSE-like stellar halos
- The Pristine Survey -- VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates
- The chemical evolution of the Bootes I ultra-faint dwarf galaxy
- The kpc Distant Spur of the Sagittarius Stream and the Outer Virgo Overdensity, as Seen in PS1 RR Lyrae Stars
- The Pristine survey VIII: The metallicity distribution function of the Milky Way halo down to the extremely metal-poor regime
- Nitrogen enrichment and clustered star formation at the dawn of the Galaxy
- The Geometry of Sagittarius Stream from Pan-STARRS1 3 RR Lyrae
- Characterising stellar halo populations I: An extended distribution function for halo K giants
- Evidence of a dwarf galaxy stream populating the inner Milky Way Halo
- The Progenitors of the Milky Way Stellar Halo: Big Bricks Favoured over Little Bricks
- The Pisces Plume and the Magellanic Wake
- The Pristine survey III: Spectroscopic confirmation of an efficient search for extremely metal-poor stars
- Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars
- The Origin of the Microlensing Events Observed Towards the LMC and the Stellar Counterpart of the Magellanic Stream
- The Profile of the Galactic Halo from Pan-STARRS1 3 RR Lyrae
- Beyond spectroscopy. I. Metallicities, distances, and age estimates for over twenty million stars from SMSS DR2 and Gaia EDR3
- A panoramic landscape of the Sagittarius stream in Gaia DR2 revealed with the STREAMFINDER spyglass
- A-type stars in the Canada-France Imaging Survey I. The stellar halo of the Milky Way traced to large radius by blue horizontal branch stars
- Stellar halo substructure generated by bar resonances
- The Pristine survey -- XXIII. Data Release 1 and an all-sky metallicity catalogue based on Gaia DR3 BP/RP spectro-photometry
- Insights into Pre-Enrichment of Star Clusters and Self-Enrichment of Dwarf Galaxies from their Intrinsic Metallicity Dispersions
- Substructure in the stellar halo near the Sun. I. Data-driven clustering in Integrals of Motion space
- Substructure in the stellar halo near the Sun. II. Characterisation of independent structures
- The Pristine survey -- XII: Gemini-GRACES chemo-dynamical study of newly discovered extremely metal-poor stars in the Galaxy
- The Outer Halo of the Milky Way as Probed by RR Lyr Variables from the Palomar Transient Facility
- Discovery of the Magellanic Stellar Stream Out to 100 Kiloparsecs
- Probing the Galactic Halo with RR Lyrae Stars. II. The Substructures of the Milky Way
- Radial halo substructure in harmony with the Galactic bar
- DESI Early Data Release Milky Way Survey Value-Added Catalogue
- Distant Echoes of the Milky Way's Last Major Merger
- The Pristine survey -- VII. A cleaner view of the Galactic outer halo using blue horizontal branch stars
- To the Galactic Virial Radius with Hyper Suprime-Cam
- The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers
- The Unmixed Debris of Gaia-Sausage/Enceladus in the Form of a Pair of Halo Stellar Overdensities
- The Cetus-Palca stream: A disrupted small dwarf galaxy. A prequel to the science possible with WEAVE with precise spectro-photometric distances
- Probing the Galactic halo with RR Lyrae stars III. The chemical and kinematic properties of the stellar halo
- The Pristine survey -- XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations
- The Pristine survey -- XVII. The C-19 stream is dynamically hot and more extended than previously thought
- The Pristine survey II: a sample of bright stars observed with FEROS
- Discovery of Magellanic Stellar Debris in the H3 Survey
- The Pristine survey XIV: chemical analysis of two ultra-metal-poor stars
- The Metallicity Gradient and Complex Formation History of the Outermost Halo of the Milky Way
- What is the Milky Way outer halo made of? High resolution spectroscopy of distant red giants
- Gaia's brightest very metal-poor (VMP) stars. Metallicity catalogue of a thousand VMP stars from Gaia's radial velocity spectrometer spectra
- Stellar streams around the Magellanic Clouds in 4D
- Chemodynamical Analysis of Metal-rich High-eccentricity Stars in the Milky Way's Disk
- The Pristine Inner Galaxy Survey (PIGS) X. Probing the early chemical evolution of the Sagittarius dwarf galaxy with carbon abundances
- Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function
- The Pristine survey: XXV. The very metal-poor Galaxy: Chemodynamics through the follow-up of the Pristine-Gaia synthetic catalogue
- Hidden deep in the halo: selection of a reduced proper motion halo catalogue and mining retrograde streams in the velocity space
- Deciphering the Kinematic Substructure of Local Dark Matter with LAMOST K Giants