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PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields

arXiv:astro-ph/0412343v2 14 Dec 2004

emission selected galaxies.Here we will discuss i) selection of Ly- emitting starbursts through deep narrow band imaging,and ii) localisation of gamma-ray burst (GRB) host galaxies.2.Ly-selection of high redshift starbursts The idea to use Ly- to search for primordial galaxies dates back to the 1960s (Partridge Peebles 1967)._ - doc.xuehai.netTranslate this page:0.5g5ml100ml20.2g100mlW.M.Keck Observatory 1998 BibliographyIdentification of a Host Galaxy at Redshift z = 3.42 for the Gamma-Ray Burst of 14 December 1997 Nature 393 35 1998 May LRIS.Kulkarni,S.; van Kerkwijk,M.Optical Observations of the Isolated Neutron Star RX J0720.4-3125 ApJ 507 L49 1998 November LRIS.Lehnert,M.; Becker,R.Spectroscopy of the extended emission associated with two high-z

Type IIn supernovae at redshift z 2 from archival data

The three z 2 type IIn supernovae are detected in the Deep component of the CanadaFranceHawaii Telescope Legacy Survey (CFHT-LS),which consists of four fields,each of area one degree Type IIn supernovae at redshift z 2 from archival data The three z 2 type IIn supernovae are detected in the Deep component of the CanadaFranceHawaii Telescope Legacy Survey (CFHT-LS),which consists of four fields,each of area one degree Transient High Energy Sky and Early Universe Surveyor addition the GRB phenomenon will be better characterized) In order to identify,classify and study the high-z GRB counterparts,an near-infrared (due to cosmological Ly-alpha suppression) telescope is needed on board.It will provide accurate positions,GRB redshifts,and GRB

The Sloan Digital Sky Survey From Asteroids to Cosmology

One of them is non-stellar Balmer absorption lines.By near-infrared spectroscopy,we discovered three FeLoBALs with Balmer absorption lines among 11 FeLoBALs (three at 1.3 z 1.65 and eight at 2.1 z 2.8).Two z 1 FeLoBALs have been confirmed to have Balmer absorption lines.Balmer absorption lines have similar line widths and velocity shifts to THESEUS A key space mission concept for Multi-Messenger Aug 01,2018 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#0183;The instrumentation foreseen on board,illustrated in Fig.2,includes:.Soft X-ray Imager (SXI,0.36 keV) a set of 4 lobster-eye telescopes units,covering a total FoV of 1 sr with source location accuracy PDF Deep Ly imaging of two z 2 04 GRB host galaxy fieldslt; 1 arcmin;.X-Gamma ray Imaging Spectrometer (XGIS,2 keV-20 MeV) a set of coded-mask cameras using monolithic X-gamma ray detectors based on bars of Silicon Drift Diodes coupled with THE SWIFT GAMMA-RAY BURST HOST GALAXY LEGACYJan 19,2016 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#0183;GRB 070223Spectroscopy of the host galaxy with LRIS shows two strong emission lines at wavelengths of and corresponding to Ly and the [O ii] doublet at a common redshift of z = 1.6295.GRB 080319AWe imaged this field extensively with Keck/LRIS (UBgRiZ) and Keck/MOSFIRE (YJHK).The host is well detected in every band (and with IRAC).

THE AFTERGLOW AND ULIRG HOST GALAXY OF THE DARK SHORT GRB

Feb 26,2013 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#0183;The host galaxy observations identify it as an ultraluminous infrared galaxy (ULIRG) at a photometric redshift of z 1.3,making GRB 120804A one of the most distant short bursts known to date.This is the first ULIRG host in the short GRB sample,exceeding even the luminous infrared galaxy (LIRG) likely host of GRB 100206A (Perley et al.2012).Some results are removed in response to a notice of local law requirement.For more information,please see here.Previous123456NextA magnetar-powered X-ray transient as the aftermath of a Apr 10,2019 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#0183;Its X-ray and host-galaxy properties allow several possible explanations including a short -ray burst seen off-axis,a low-luminosity -ray burst at high redshift,or a tidal disruption event Some results are removed in response to a notice of local law requirement.For more information,please see here.12345NextDiscovery of the afterglow and host galaxy of the low From the detected emission lines we measure the redshift of the GRB host galaxy to be z= 0.1218 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#177; 0.0003.3 HOST GALAXY PROPERTIES 3.1 Host morphology.Visual inspection of the images in R and K bands shows the host to be a nearly face-on galaxy,with clear bulge,disc and spiral arm components.At least two spiral arms can be distinguished

Some results are removed in response to a notice of local law requirement.For more information,please see here.Search for the host galaxy of GRB 050904 at z=6.3

Request PDF Search for the host galaxy of GRB 050904 at z=6.3 We present the results of deep imaging of the field of GRB 050904 with Suprime-Cam onQuora - A place to share knowledge and better understand Quora is a place to gain and share knowledge.It's a platform to ask questions and connect with people who contribute unique insights and quality answers.This empowers people to learn from each other and to better understand the world.

Paul Martini Publications - Astronomy

Jun 07,2018 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#0183;The Photometric Redshift Survey and the Rest-frame R-band Galaxy Luminosity Function at Redshift 0.5 z 1.5 [ Abstract PDF (660 kb) ] Forschini,L.,et al.(14 authors including P.Martini ),2002,AA,396,787NASA EarthdataNASA's Jet Propulsion Laboratory (JPL) Multi-angle Imaging SpectroRadiometer (MISR) project and the Atmospheric Science Data Center (ASDC) announce the release of new versions of the Multi-angle Imaging SpectroRadiometer (MISR) Level 2 (L2) Aerosol Product,the MISR L2 Land Surface Product,and the Level 3 (L3) Component Global Aerosol and Land Long-Duration Gamma-Ray Burst Host Galaxies in Emission PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#0183;The Photometric Redshift Survey and the Rest-frame R-band Galaxy Luminosity Function at Redshift 0.5 z 1.5 [ Abstract PDF (660 kb) ] Forschini,L.,et al.(14 authors including P.Martini ),2002,AA,396,787

Gamma-ray bursts and their use as cosmic probes Royal

In contrast with GRB 980425,the host galaxy of the peculiar,supernovaless GRB 111005A (see PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#167;2.4) has a near-solar metallicity,and the MUSE data show no indication that the GRB occurred within an especially metal-poor region of its host (M Tanga 2017,personal communication).Gamma-ray burst investigation via polarimetry and Jul 29,2008 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#0183;The primary scientific goal of the GRIPS mission is to revolutionize our understanding of the early universe using -ray bursts.We propose a new generation gamma-ray observatory capable of unprecedented spectroscopy over a wide range of -ray energies (200 keV50 MeV) and of polarimetry (2001000 keV).The -ray sensitivity to nuclear absorption features enables the measurement of Gamma-ray Burst 080503Gamma-ray Burst 080503 (All information courtesy of the instrument teams.) we report analysis of additional imaging taken between 1.0-2.5 hours after the burst in g,r,i,and z filters. ,consistent with the lack of a coincident host galaxy down to 28.5 mag in deep HST imaging.Our observations reinforce the notion that short GRBs

Discovery of the afterglow and host galaxy of the low

Aug 02,2010 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#0183;From the detected emission lines we measure the redshift of the GRB host galaxy to be z= 0.1218 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#177; 0.0003.3 HOST GALAXY PROPERTIES 3.1 Host morphology.Visual inspection of the images in R and K bands shows the host to be a nearly face-on galaxy,with clear bulge,disc and spiral arm components.At least two spiral arms can be distinguished Diffuse Ly haloes around galaxies at z = 2.26.6 We use large photometric samples of LAEs at z = 2.2,3.1,3.7,5.7,and 6.6 made by the large-area NB imaging surveys of Subaru telescope.Our z = 2.2 sample consists of 3556 LAEs found in five deep fields of COSMOS,GOODS-N,GOODS-S,SSA22,and SXDS (Nakajima et al.2012).Diffuse Ly haloes around galaxies at z = 2.26.6 We use large photometric samples of LAEs at z = 2.2,3.1,3.7,5.7,and 6.6 made by the large-area NB imaging surveys of Subaru telescope.Our z = 2.2 sample consists of 3556 LAEs found in five deep fields of COSMOS,GOODS-N,GOODS-S,SSA22,and SXDS (Nakajima et al.2012).

Deep submillimeter and radio observations in the SSA22

We study the heating mechansims and Ly escape fractions of 35 Ly blobs (LABs) at z3.1 in the SSA22 field,using the submillimeter (submm) data from the Atacama Large Millimeter/Submillimeter Array (ALMA) and the Submillimetre Common-User Bolometer Array-2 (SCUBA-2) on the James Clerk Maxwell Telescope (JCMT),and the radio data from the Karl G.Jansky Very Large Array (VLA).WithDeep Ly-alpha imaging of two z=2.04 GRB host galaxy fields We report on the results of deep narrow-band Ly-alpha,U and I imaging of the fields of two GRBs at z=2.04 (GRB 000301C and GRB 000926).We find that the host galaxy of GRB 000926 is an extended,strong Ly-alpha emitter with a rest-frame equivalent width of 71+20-15 AA.The galaxy consists of two main components and several fainter knots.Cited by 88Publish Year 2010Author A.Rowlinson,K.Wiersema,A.J.Levan,N.R.Tanvir,P.T.O'Brien,E.Rol,J.Hjorth,C.C.Th PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#246;ne,UV star-formation rates of GRB host galaxies2.GRB host galaxy sample Our own multi-colour imaging studies of GRB host galax-ies have been presented elsewhere (Gorosabel et al.2003a,b; Christensen et al.2004).The present work is based on a com-pilation of photometry already available in the literature (in-cluding our own observational work).

CiteSeerX

CiteSeerX - Document Details (Isaac Councill,Lee Giles,Pradeep Teregowda) Astronomy Astrophysics manuscript no.(will be inserted by hand later) Deep Ly imaging of two z=2.04 GRB host galaxy fields ,A magnetar-powered X-ray transient as the aftermath of a Apr 10,2019 PDF Deep Ly imaging of two z 2 04 GRB host galaxy fields#0183;Its X-ray and host-galaxy properties allow several possible explanations including a short -ray burst seen off-axis,a low-luminosity -ray burst at high redshift,or a tidal disruption event 2 SCIENCE GOALS AND TECHNICAL REQUIREMENTS2.1.3 Observations of Magnetic Fields in Galaxy Clusters Clusters of galaxies are filled with turbulent hot gas,relativistic particles,and magnetic fields.The hot gas is best observed by its thermal X-ray emission,but the relativistic components (fields and particles)

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Translate this pageDeep Ly-alpha imaging of two z=2.04 GRB host galaxy fields; ; ; ; ; 20100A4.docx; 26; 2012- () (PDF) HST narrow-band search for extended Ly-alpha We search for extended Ly-alpha emission around two z PDF Deep Ly imaging of two z 2 04 GRB host galaxy fieldsgt;6 quasars,SDSS J1030+0524 (z=6.309) and SDSS J1148+5251 (z=6.419) using WFC3 narrow-band filters on board the Hubble Space Telescope.

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