Statistical correlation between the distribution of Ly emitters and IGM HI at mapped by Subaru/Hyper Suprime-Cam
arXiv:2008.01733 · doi:10.3847/1538-4357/abcd93
Abstract
The correlation between neutral Hydrogen (HI) in the intergalactic medium (IGM) and galaxies now attracts great interests. We select four fields which include several coherently strong Ly absorption systems at detected by using background quasars from the whole SDSS/(e)BOSS database. Deep narrow-band and -band imaging are performed using the Hyper Suprime-Cam on the Subaru Telescope. We select out 2,642 Ly emitter (LAE) candidates at down to the Ly luminosity of to construct the galaxy overdensity maps, covering an effective area of 5.39 deg. Combining the sample with the Ly absorption estimated from 64 (e)BOSS quasar spectra, we find a moderate to strong correlation between the LAE overdensity and the effective optical depth in line-of-sights, with -value () when the field that contains a significant quasar overdensity is in(ex)cluded. The cross-correlation analysis also clearly suggests that up to pMpc, LAEs tend to cluster in the regions rich in HI gas, indicated by the high , and avoid the low region where the HI gas is deficient. By averaging the as a function of the projected distance () to LAEs, we find a excess signal at level at pkpc, indicating the dense HI in circumgalactic medium, and a tentative excess at pkpc in IGM regime, corroborating the cross-correlation signal detected at about pMpc. These statistical analyses indicate that galaxyIGM HI correlations exist on scales ranging from several hundred pkpc to several pMpc at .
arXiv comment27 pages, 15 figures; Resubmitted to ApJ after the first referee's report. Comments are welcome
References in corpus (92)
- Planck 2015 results. XIII. Cosmological parameters
- Measuring Reddening with SDSS Stellar Spectra and Recalibrating SFD
- The cosmological simulation code GADGET-2
- Cosmic Star Formation History
- Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey
- The Baryon Oscillation Spectroscopic Survey of SDSS-III
- First results from the IllustrisTNG simulations: matter and galaxy clustering
- Galaxy Bimodality due to Cold Flows and Shock Heating
- SEGUE: A Spectroscopic Survey of 240,000 stars with g=14-20
- How Filaments are Woven into the Cosmic Web
- The Circumgalactic Medium
- The Structure and Kinematics of the Circum-Galactic Medium from Far-UV Spectra of z~2-3 Galaxies
- Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Temperature Analysis
- Spectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey
- The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data
- The large-scale structure of the Universe
- A primer on hierarchical galaxy formation: the semi-analytical approach
- Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program
- Galaxies and Intergalactic Matter at Redshift z~3: Overview
- The Hyper Suprime-Cam Software Pipeline
- An updated analytic model for the attenuation by the intergalactic medium
- The Lyman-alpha Forest in the Cold Dark Matter Model
- Statistical Analysis of Galaxy Surveys - I. Robust error estimation for 2-point clustering statistics
- The Lyman Alpha Forest from Gravitational Collapse in the CDM+Lambda Model
- Ancient Light from Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-Clusters
- The Gaseous Environment of High-z Galaxies: Precision Measurements of Neutral Hydrogen in the Circumgalactic Medium of z ~ 2-3 Galaxies in the Keck Baryonic Structure Survey
- The Connection Between Galaxies and Intergalactic Absorption Lines at Redshift 2<z<3
- Quasar Quartet Embedded in Giant Nebula Reveals Rare Massive Structure in Distant Universe
- A Direct Precision Measurement of the Intergalactic Lyman-alpha Opacity at 2<z<4.2
- The DEIMOS 10k spectroscopic survey catalog of the COSMOS field
- Galaxy Protoclusters as Drivers of Cosmic Star-Formation History in the First 2 Gyr
- Lyman-Alpha-Emitting Galaxies at z = 2.1 in ECDF-S: Building Blocks of Typical Present-day Galaxies?
- A Refined Measurement of the Mean Transmitted Flux in the Ly-alpha Forest over 2 < z < 5 Using Composite Quasar Spectra
- Metal-line absorption around 2.4 star-forming galaxies in the Keck Baryonic Structure Survey
- A massive, distant proto-cluster at z=2.47 caught in a phase of rapid formation?
- First Results from Z-FOURGE: Discovery of a Candidate Cluster at z = 2.2 in COSMOS
- Quasars Probing Quasars VI. Excess HI Absorption Within One Proper Mpc of z~2 Quasars
- Discovery of an Enormous Ly nebula in a massive galaxy overdensity at
- SILVERRUSH. III. Deep Optical and Near-Infrared Spectroscopy for Lya and UV-Nebular Lines of Bright Lya Emitters at z=6-7
- Average Metallicity and Star Formation Rate of Lya Emitters Probed by a Triple Narrow-Band Survey
- First Data Release of the COSMOS Lyman-Alpha Mapping And Tomography Observations: 3D Lyman- Forest Tomography at 2.05 < z < 2.55
- Bright and Faint Ends of Ly Luminosity Functions at Determined by the Subaru Survey: Implications for AGN, Magnification Bias, and ISM HI Evolution
- Probing the IGM-Galaxy Connection at z < 0.5 I: A Galaxy Survey in QSO Fields and a Galaxy-Absorber Cross-Correlation Study
- MApping the Most Massive Overdensities (MAMMOTH) II -- Discovery of an Extremely Massive Overdensity BOSS1441 at
- The CALYMHA survey: Lya luminosity function and global escape fraction of Lya photons at z=2.23
- Modelling the evolution of galaxy clustering
- GOLDRUSH. III. A Systematic Search of Protoclusters at Based on the Area
- Lyman-alpha Forest Tomography from Background Galaxies: The First Megaparsec-Resolution Large-Scale Structure Map at z>2
- Physical Bias of Galaxies From Large-Scale Hydrodynamic Simulations
- A Systematic Survey of Protoclusters at in the CFHTLS Deep Fields
- Predicting QSO Continua in the Ly Alpha Forest
- The BOSS Lyman-alpha Forest Sample from SDSS Data Release 9
- Neutral hydrogen optical depth near star-forming galaxies at z~2.4 in the Keck Baryonic Structure Survey
- Shadow of a Colossus: A z=2.45 Galaxy Protocluster Detected in 3D Ly-a Forest Tomographic Mapping of the COSMOS Field
- A Second Stellar Color Locus: a Bridge from White Dwarfs to M stars
- MApping the Most Massive Overdensities Through Hydrogen (MAMMOTH) I: Methodology
- Identification of the progenitors of rich clusters and member galaxies in rapid formation at z>2
- A comparison of observed and simulated absorption from HI, CIV, and SiIV around star-forming galaxies suggests redshift-space distortions are due to inflows
- Mean-flux Regulated PCA Continuum Fitting of SDSS Lyman-alpha Forest Spectra
- A z=2.5 protocluster associated with the radio galaxy MRC 2104-242: star formation and differing mass functions in dense environments
- Observational Requirements for Lyman-alpha Forest Tomographic Mapping of Large-Scale Structure at z ~ 2
- The Keck Baryonic Structure Survey: Using foreground/background galaxy pairs to trace the structure and kinematics of circumgalactic neutral hydrogen at
- Grism Confirmation of Structures at from the Clusters Around Radio-Loud AGN (CARLA) Survey
- LATIS: The Ly Tomography IMACS Survey
- The HETDEX Pilot Survey. IV. The Evolution of [O II] Emitting Galaxies from z ~ 0.5 to z ~ 0
- On the connection between the intergalactic medium and galaxies: The HI-galaxy cross-correlation at z < 1
- Witnessing galaxy assembly in an extended z~3 structure
- The evolution of rest-frame UV properties, Lya EWs and the SFR-Stellar mass relation at z~2-6 for SC4K LAEs
- Osaka Feedback Model: Isolated Disk Galaxy Simulations
- The VIMOS Ultra Deep Survey: Ly Emission and Stellar Populations of Star-Forming Galaxies at 2<z<2.5
- Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
- Discovery of a Proto-cluster Associated with a Ly- Blob Pair at z=2.3
- Direct evidence for Ly depletion in the protocluster core
- The Stellar Mass, Star Formation Rate and Dark Matter Halo Properties of LAEs at
- How Do Galaxies trace a large scale structure?: A case study around a massive protocluster at
- Ly view around a z=2.84 hyperluminous QSO at a node of the cosmic web
- Cross correlation of Lyman-alpha absorbers with gas-rich galaxies
- Lyman-Alpha Emitter Galaxies at z ~ 2.8 in the Extended Chandra Deep Field-South: I. Tracing the Large-Scale Structure via Lyman-Alpha Imaging
- Enhancement of Galaxy Overdensity around Quasar Pairs at z<3.6 based on the Hyper Suprime-Cam Subaru Strategic Program Survey
- The UV Continuum of z > 1 Star-forming Galaxies in the Hubble Ultraviolet UltraDeep Field
- Characterization of the distribution of the Llyαemitters in the 53W002 field at z = 2.4
- Cosmic Galaxy-IGM HI Relation at Probed in the COSMOS/UltraVISTA deg Field
- The dominant origin of diffuse Ly halos around LAEs explored by SED fitting and clustering analysis
- CHORUS. I. Cosmic HydrOgen Reionization Unveiled with Subaru: Overview
- Redshift Space Distortion of 21cm line at 1<z<5 with Cosmological Hydrodynamic Simulations
- Quasars with PV broad absorption in BOSS data release 9
- Imaging of diffuse HI absorption structure in the SSA22 proto-cluster region at z = 3.1
- 3D Distribution Map of HI Gas and Galaxies Around an Enormous Ly Nebula and Three QSOs at Revealed by the HI Tomographic Mapping Technique
- Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption
- Enhancement of HI absorption associated with the large-scale proto-cluster and characteristic structures with AGNs sculptured over Gpc scale in the SSA22 field
- Are Lyα emitters segregated in protoclusters regions?
- A search for Ly-alpha emitters around a concentrated-region of strong Ly-alpha absorbers at z=2.3
Cited by in corpus (14)
- Probing Feedback via IGM tomography and Ly forest with Subaru PFS, TMT/ELT, and JWST
- Spectroscopic Confirmation of two Extremely Massive Protoclusters BOSS1244 and BOSS1542 at
- SILVERRUSH X: Machine Learning-Aided Selection of LAEs at , , , , , and from the HSC SSP and CHORUS Survey Data
- The physical origin for spatially large scatter of IGM opacity at the end of reionization: the IGM Ly opacity-galaxy density relation
- Interrelation of the environment of Ly emitters and massive galaxies at
- Detecting preheating in proto-clusters with Lyman- Forest Tomography
- Searching for the shadows of giants II: the effect of local ionisation on the Lyman- absorption signatures of protoclusters at redshift
- A Search for Massive Galaxy Population in a Protocluster of LAEs at near the Radio Galaxy 53W002
- How are Lyman absorbers in the cosmic web related to gas-rich galaxies?
- The Role of Dust, UV Luminosity and Large-scale Environment on the Escape of Lya Photons: A Case Study of a Protocluster field at z = 3.1
- LATIS: A Sample of IGM-selected Protoclusters and Protogroups at
- On the Metallicities and Kinematics of the Circumgalactic Media of Damped Ly Systems at
- LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at
- The Lyman- Forest from LBGs: First 3D Correlation Measurement with DESI and Prospects for Cosmology