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Related papers: A Luminosity Function of Lyman Alpha Emitting Gala…

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We report the discovery of a Lyman-alpha-emitting galaxy at redshift z=6.545 serendipitously identified in the course of spectroscopic follow-up of hard X-ray sources on behalf of the Serendipitous Extragalactic X-Ray Source Identification…

We present a new measurement of the Ly$\alpha$ luminosity function at redshift $z=6.9$, finding moderate evolution from $z=5.7$ that is consistent with a fully or largely ionized $z\sim7$ intergalactic medium. Our result is based on four…

We report on deep spectroscopy using LRIS on Keck I and FORS2 on the VLT of a sample of 22 candidate z~6 Lyman Break galaxies (LBGs) selected by the i-z> 1.3 dropout criterion. Redshifts could be measured for eight objects. These redshifts…

We selected 40 candidate Lyman Alpha Emitting galaxies (LAEs) at z ~=3.1 with observed frame equivalent widths >150A and inferred emission line fluxes >2.5x10^-17 ergs/cm^2/s from deep narrow-band and broad-band MUSYC images of the Extended…

We present a spectroscopic redshift measurement of a very bright Lyman break galaxy at z=7.7302+-0.0006 using Keck/MOSFIRE. The source was pre-selected photometrically in the EGS field as a robust z~8 candidate with H=25.0 mag based on…

Using new Keck DEIMOS spectroscopy, we examine the origin of the steep number counts of ultra-faint emission-line galaxies recently reported by Dressler et al. (2011). We confirm six Lyman Alpha emitters (LAEs), three of which have…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Alaina Henry , Crystal Martin , Alan Dressler , Marcin Sawicki , Patrick McCarthy

We present a study on stellar properties of Lyman-alpha (Ly$\alpha$) emitters at 5 $< z <$ 8.2. We use 247 photometrically-selected, lensed, high-redshift, low luminosity galaxy candidates with spectroscopic follow-up. Of these, 38 are…

Strong Lyman-alpha emission is a signpost of young stars and the absence of dust and thus indicates young galaxies. To find such a population of young galaxies at z=4.5 we started the Large Area Lyman Alpha survey (LALA). This survey…

Astrophysics · Physics 2007-05-23 Sangeeta Malhotra , James Rhoads , Arjun Dey , Buell Jannuzi , Daniel Stern , Hyron Spinrad

We report the results from some of the deepest Keck/Multi-Object Spectrometer For Infra-Red Exploration data yet obtained for candidate $z \gtrsim 7$ galaxies. Our data show one significant line detection with 6.5$\sigma$ significance in…

Astrophysics of Galaxies · Physics 2016-08-03 Mimi Song , Steven L. Finkelstein , Rachael C. Livermore , Peter L. Capak , Mark Dickinson , Adriano Fontana

The recent development of large, complete samples which identify high-redshift galaxies at z~5.7 and z~6.5 from deep, wide-field surveys provides detailed information on the earliest galaxies, their numbers, spatial and kinematic…

Astrophysics · Physics 2007-05-23 Esther M. Hu , Lennox L. Cowie , Peter Capak , Yuko Kakazu

We report the discovery of Lyman-alpha emission (Ly$\alpha$) in the bright galaxy EGSY-2008532660 (hereafter EGSY8p7) using the MOSFIRE spectrograph at the Keck Observatory. First reported by Roberts-Borsani et al. (2015), it was selected…

We describe narrowband and spectroscopic searches for emission-line star forming galaxies in the redshift range 3 to 6 with the 10 m Keck II Telescope. These searches yield a substantial population of objects with only a single strong…

Astrophysics · Physics 2009-10-30 Esther M. Hu , Lennox L. Cowie , Richard G. McMahon

We report spectroscopic confirmations of 15 Lyman-alpha galaxies at $z\sim7$, implying a spectroscopic confirmation rate of $\sim$80% on candidates selected from LAGER (Lyman-Alpha Galaxies in the Epoch of Reionization), which is the…

We present Keck spectroscopic observations of z>6 Lyman-break galaxy (LBG) candidates in the Subaru Deep Field (SDF). The candidates were selected as i'-dropout objects down to z'=27 AB magnitudes from an ultra-deep SDF z'-band image. With…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Linhua Jiang , Eiichi Egami , Nobunari Kashikawa , Gregory Walth , Yuichi Matsuda , Kazuhiro Shimasaku , Tohru Nagao , Kazuaki Ota , Masami Ouchi

We report in this work on a project aimed at determining Ly{\alpha} luminosity functions from z=3 to z=6. The project is based on the use of very deep photometry from the SHARDS Survey, in a set of 24 medium band filters in the GOODS-N…

Cosmology and Nongalactic Astrophysics · Physics 2012-01-24 J. M. Rodriguez-Espinosa , O. Gonzalez-Martin , J. A. Lopez-Aguerri , C. Muñoz-Tuñon , P. G. Perez-Gonzalez , A. Cava

We present a study of three Lyman-alpha emitting galaxies (LAEs), selected via a narrow-band survey in the GOODS northern field, and spectroscopically confirmed to have redshifts of z ~ 5.65. Using HST ACS and Spitzer IRAC data, we…

Astrophysics · Physics 2011-02-11 Kamson Lai , Jia-Sheng Huang , Giovanni Fazio , Lennox L. Cowie , Esther M. Hu , Yuko Kakazu

We discovered a sample of 250 Ly-Alpha emitting (LAE) galaxies at z=2.1 in an ultra-deep 3727 A narrow-band MUSYC image of the Extended Chandra Deep Field-South. LAEs were selected to have rest-frame equivalent widths (EW) > 20 A and…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 L. Guaita , E. Gawiser , N. Padilla , H. Francke , N. A. Bond , C. Gronwall , R. Ciardullo , J. J. Feldmeier , S. Sinawa , G. A. Blanc , S. Virani

We discuss new Keck/MOSFIRE spectroscopic observations of four luminous galaxies at z~7-9 selected to have intense optical line emission by Roberts-Borsani et al. (2016). Previous follow-up has revealed Lyman-alpha in two of the four…

Following our previous spectroscopic observations of $z>7$ galaxies with Gemini/GNIRS and VLT/XSHOOTER, which targeted a total of 8 objects, we present here our results from a deeper and larger VLT/FORS2 spectroscopic sample of Wide Field…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 Joseph Caruana , Andrew J. Bunker , Stephen M. Wilkins , Elizabeth R. Stanway , Silvio Lorenzoni , Matt J. Jarvis , Holly Elbert

We present the luminosity function (LF) for ultraluminous Ly$\alpha$ emitting galaxies (LAEs) at z = 6.6. We define ultraluminous LAEs (ULLAEs) as galaxies with logL(Ly$\alpha$) > 43.5 erg s$^{-1}$. We select our main sample using the g',…

Astrophysics of Galaxies · Physics 2020-06-05 Anthony J. Taylor , Amy J. Barger , Lennox L. Cowie , Esther M. Hu , Antoinette Songaila