Detection of a Lyman-alpha Emission-Line Companion to the z=4.69 QSO BR1202-0725
arXiv:astro-ph/9512165 · doi:10.1086/309958
Abstract
We report the detection of a nearby emission-line companion to the z=4.695 quasar BR1202-0725. Deep narrow-band exposures on this field from the UH 2.2 m show a Ly alpha flux of 1.5\times\ten{-16} ergs cm^{-2} s^{-1}. High-resolution HST WFC2 imaging in the F814W filter band shows continuum structure near the emission position, at 2.6" NW of the quasar, corresponding to a projected separation of ~7.5 h^{-1} kpc for \qnought=0.5, where h=\hnought/100\kms Mpc^{-1}. We discuss possible explanations for the combined line and color properties. The ionization is most likely produced by the quasar, but if due to underlying star formation would require a star formation rate of ~7 h^2 solar masses per yr.
12 pages LaTeX (aastex4.0 macros: aasms4.sty, flushrt.sty) plus 3 figures. To appear in the Astrophysical Journal Letters. Typo in original submission ("2" should have been "7" in luminosity: 7e42 h^{-2} ergs and in the star formation rate: 7 h^{-2} \msun per yr). Resubmitted with figures
References in corpus (2)
Cited by in corpus (56)
- High-z Lyman-alpha Emitters. I. A Blank-Field Search for Objects Near Redshift z=3.4 in and around the Hubble Deep Field and the Hawaii Deep Field SSA22
- The Density of Lyman-alpha Emitters at Very High Redshift
- Molecular gas and dust around a radio-quiet quasar at redshift 4.7
- CO(1-0) in z >/~ 4 Quasar Host Galaxies: No Evidence for Extended Molecular Gas Reservoirs
- Superwind model of extended Lyman alpha emitters at high redshift
- A Galaxy at z=5.34
- Detection of Lyman-alpha Emitting Galaxies at Redshift z=4.55
- Extended Lyman Alpha Emission Around Young Quasars: a Constraint on Galaxy Formation
- High resolution imaging of molecular line emission from high redshift QSOs
- A 250 GHz Survey of High Redshift QSOs from the Sloan Digital Sky Survey
- MApping the Most Massive Overdensities (MAMMOTH) II -- Discovery of an Extremely Massive Overdensity BOSS1441 at
- An Extremely Luminous Galaxy at z=5.74
- ALMA Observation of 158 micron [CII] Line and Dust Continuum of a z=7 Normally Star-forming Galaxy in the Epoch of Reionization
- Molecular gas at high redshift: jet-induced star formation?
- A Detection of [CII] line emission in the z=4.7 QSO BR1202-0725
- Extended Lyman alpha emission around bright quasars
- Strongly star-forming rotating disks in a complex merging system at z = 4,7 as revealed by ALMA
- MApping the Most Massive Overdensities Through Hydrogen (MAMMOTH) I: Methodology
- The anatomy of an extreme starburst within 1.3Gyr of the Big Bang revealed by ALMA
- The extended Lyman-alpha emission surrounding the z=3.04 radio-quiet QSO1205-30: Primordial infalling gas illuminated by the quasar?
- The Photometric Redshift Distribution and Evolutionary Properties of Galaxies up to z= 4.5 in the Field of the Quasar BR1202-0725
- Galaxies at z=4 and the Formation of Population II
- Search Techniques for Distant Galaxies
- An Imaging and Spectroscopic Study of the z=3.38639 Damped Lyman Alpha System in Q0201+1120: Clues to Star Formation Rate at High Redshift
- Varying [CII]/[NII] line ratios in the interacting system BR1202-0725 at z=4.7
- Sensitive Radio Observations of High Redshift Dusty QSOs
- A Search for Lyman alpha Emitters at Redshift 3.7
- On the Origin of Lyman Blobs at High Redshift: Submillimetric Evidence for a Hyperwind Galaxy at z=3.1
- The Mysterious Absence of Neutral Hydrogen within One Mpc of a Luminous Quasar at Redshift 2.168
- Detection of CO(3-2) Emission at z=2.64 from the Gravitationally Lensed Quasar MG 0414+0534
- BR1202-0725: An Extreme Multiple Merger at z = 4.7
- Detection of CO (2-1) and Radio Continuum Emission from the z = 4.4 QSO BRI 1335-0417
- Detection of a CMB decrement towards the z = 3.8 quasar pair PC1643+4631A&B
- A QSO host galaxy and its Lyalpha emission at z=6.43
- Spitzer Observations of High Redshift QSOs
- Close companions to two high-redshift quasars
- On the Connection Between Metal Absorbers and Quasar Nebulae
- Herschel/PACS far-infrared photometry of two z>4 quasars
- Sensitive VLBI Observations of the z = 4.7 QSO BRI 1202-0725
- Resolving the Interstellar Medium in Ultraluminous Infrared QSO Hosts with ALMA
- The Ionised- and Cool-Gas Content of The BR1202-0725 System as seen by MUSE and ALMA
- Fluorescent Lyman-alpha Emission from Gas Near a QSO at Redshift 4.28
- Karl G. Jansky Very Large Array observations of cold dust and molecular gas in starbursting quasar host galaxies at z~4.5
- ALMA [NII] 205 micron Imaging Spectroscopy of the Interacting Galaxy System BRI 1202-0725 at Redshift 4.7
- An Intermediate-band imaging survey for high-redshift Lyman Alpha Emitters: The Mahoroba-11
- A coronagraphic absorbing cloud reveals the narrow-line region and extended Lyman- emission of QSO J0823+0529
- Subaru Deep Spectroscopy of a Star-forming Companion Galaxy of BR 1202-0725 at
- First [NII]122m line detection in a QSO-SMG pair BRI 1202-0725 at
- Emission Line Galaxies in the STIS Parallel Survey I: Observations and Data Analysis
- Dense and warm neutral gas in BR1202-0725 at z = 4.7 as traced by the [O I] 145 um line
- Star-formation at z=4.7 in the environment of the QSO BR1202-07
- New Constraints on the Molecular Gas in the Prototypical HyLIRGs BRI1202-0725 & BRI1335-0417
- Etching glass in the early Universe: Luminous HF and water emission in a QSO-SMG pair at z=4.7
- Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
- New High-Redshift Galaxies at = 5.8 - 6.5 in the Subaru Deep Field
- Measuring the Virial Temperature of Galactic Halos Through Electron Scattering of Quasar Emission Lines