papers

Publications (27)

physics.acc-ph2021

Developing a 50 MeV LPA-based Injector at ATHENA for a Compact Storage Ring

E. Panofski, C. Braun, J. Dirkwinkel +22

The laser-driven generation of relativistic electron beams in plasma and their acceleration to high energies with GV/m-gradients has been successfully demonstrated. Now, it is time…

astro-ph.HE2015

Search for Gamma-Ray Emission from DES Dwarf Spheroidal Galaxy Candidates with Fermi-LAT Data

LAT Collaboration, The DES Collaboration, A. Drlica-Wagner +123

Due to their proximity, high dark-matter content, and apparent absence of non-thermal processes, Milky Way dwarf spheroidal satellite galaxies (dSphs) are excellent targets for the…

astro-ph.GA2015

DES J0454-4448: Discovery of the First Luminous z > 6 Quasar from the Dark Energy Survey

S. L. Reed, R. G. McMahon, M. Banerji +59

We present the first results of a survey for high redshift, z 6, quasars using izY multi-colour photometric observations from the Dark Energy Survey (DES). Here we report the…

astro-ph.CO2026

Dark Energy Survey Year 6 Results: Redshift Calibration of the Weak Lensing Source Galaxies

B. Yin, A. Amon, A. Campos +95

Determining the distribution of redshifts for galaxies in wide-field photometric surveys is essential for robust cosmological studies of weak gravitational lensing. We present the…

astro-ph2003

CCD Photometry of the Globular Cluster omega Centauri. II. Stellar Populations and Age-Metallicity Relation

S. -C. Rey, Y. -W. Lee, C. Ree +3

We present wide-field and high-precision BV and Ca & Stromgren by photometry of omega Centauri, which represents one of the most extensive photometric surveys to date for this clus…

astro-ph.SR2020

Chemical Analysis of the Ultra-Faint Dwarf Galaxy Grus~II. Signature of high-mass stellar nucleosynthesis

T. T. Hansen, J. L. Marshall, J. D. Simon +59

We present a detailed abundance analysis of the three brightest member stars at the top of the giant branch of the ultra-faint dwarf galaxy Grus~II. All stars exhibit a higher than…

astro-ph.IM2013

Searching for pulsars using image pattern recognition

W. W. Zhu, A. Berndsen, E. C. Madsen +41

In this paper, we present a novel artificial intelligence (AI) program that identifies pulsars from recent surveys using image pattern recognition with deep neural nets---the PICS…

hep-ex2013

Measurement of the branching ratio of the decay

J. R. Batley, G. E. Kalmus, C. Lazzeroni +110

From the 2002 data taking with a neutral kaon beam extracted from the CERN-SPS, the NA48/1 experiment observed 97 candidates with a back…

astro-ph.IM2011

DECam integration tests on telescope simulator

M. Soares-Santos, J. Annis, M. Bonati +31

The Dark Energy Survey (DES) is a next generation optical survey aimed at measuring the expansion history of the universe using four probes: weak gravitational lensing, galaxy clus…

astro-ph.IM2012

PreCam, a Precursor Observational Campaign for Calibration of the Dark Energy Survey

K. Kuehn, S. Kuhlmann, S. Allam +40

PreCam, a precursor observational campaign supporting the Dark Energy Survey (DES), is designed to produce a photometric and astrometric catalog of nearly a hundred thousand standa…

hep-ex2016

ChPT tests at the NA48 and NA62 experiments at CERN

NA48/2, NA62 Collaborations, : +159

The NA48/2 Collaboration at CERN has accumulated unprecedented statistics of rare kaon decays in the Ke4 modes: Ke4(+-) () and Ke4(00) ($K^\pm \to π^…

hep-ex2024

First observation and study of the decay

2 Collaboration, J. R. Batley, G. Kalmus +121

The NA48/2 experiment at CERN reports the first observation of the decay based on a sample of 2437 candidates with 15% background co…

hep-ex2014

Recent NA48/2 and NA62 results

F. Ambrosino, A. Antonelli, G. Anzivino +156

The NA48/2 Collaboration at CERN has accumulated and analysed unprecedented statistics of rare kaon decays in the modes: () and…

astro-ph.IM2013

PEACE: Pulsar Evaluation Algorithm for Candidate Extraction -- A software package for post-analysis processing of pulsar survey candidates

K. J. Lee, K. Stovall, F. A. Jenet +41

Modern radio pulsar surveys produce a large volume of prospective candidates, the majority of which are polluted by human-created radio frequency interference or other forms of noi…

astro-ph.IM2009

Thirty Meter Telescope Site Testing I: Overview

M. Schoeck, S. Els, R. Riddle +15

As part of the conceptual and preliminary design processes of the Thirty Meter Telescope (TMT), the TMT site testing team has spent the last five years measuring the atmospheric pr…

astro-ph.IM2014

Photometric redshift analysis in the Dark Energy Survey Science Verification data

C. Sánchez, M. Carrasco Kind, H. Lin +74

We present results from a study of the photometric redshift performance of the Dark Energy Survey (DES), using the early data from a Science Verification (SV) period of observation…

astro-ph.SR2012

Photometric Maps Based on the OGLE-III Shallow Survey in the Large Magellanic Cloud

K. Ulaczyk, M. K. Szymanski, A. Udalski +8

We present photometric maps based on data from the shallow survey in the Large Magellanic Cloud performed as the supplementary project during the third phase of the Optical Gravita…

astro-ph2008

The Araucaria Project. The Distance to the Sculptor dwarf spheroidal galaxy from infrared photometry of RR Lyrae stars

G. Pietrzynski, W. Gieren, O. Szewczyk +8

We have obtained single-phase near-infrared magnitudes in the J and K bands for a sample of 78 RR Lyrae stars in the Sculptor dSph galaxy. Applying different theoretical and empiri…

astro-ph2004

The Araucaria Project. An improved distance to the Sculptor spiral galaxy NGC 300 from its Cepheid variables

W. Gieren, G. Pietrzynski, A. Walker +8

In a previous paper, we reported on the discovery of more than a hundred new Cepheid variables in the Sculptor Group spiral NGC 300 from wide-field images taken in the B and V phot…

astro-ph.CO2015

Mass and galaxy distributions of four massive galaxy clusters from Dark Energy Survey Science Verification data

P. Melchior, E. Suchyta, E. Huff +89

We measure the weak-lensing masses and galaxy distributions of four massive galaxy clusters observed during the Science Verification phase of the Dark Energy Survey. This pathfinde…

astro-ph.CO2015

Photometric redshifts and clustering of emission line galaxies selected jointly by DES and eBOSS

S. Jouvel, T. Delubac, J. Comparat +65

We present the results of the first test plates of the extended Baryon Oscillation Spectroscopic Survey. This paper focuses on the emission line galaxies (ELG) population targetted…

astro-ph.SR2014

On the kinematic separation of field and cluster stars across the Bulge globular NGC 6528

E. P. Lagioia, A. P. Milone, P. B. Stetson +12

We present deep and precise multi-band photometry of the Galactic Bulge globular cluster NGC6528. The current dataset includes optical and near-infrared images collected with ACS/W…

astro-ph.GA2010

The Araucaria Project. First Cepheid Distance to the Sculptor Group Galaxy NGC 7793 from Variables discovered in a Wide-Field Imaging Survey

G. Pietrzynski, W. Gieren, M. Hamuy +12

We have detected, for the first time, Cepheid variables in the Sculptor Group spiral galaxy NGC 7793. From wide-field images obtained in the optical V and I bands on 56 nights in 2…

hep-ex2010

Empirical parameterization of the K+- -> pi+- pi0 pi0 decay Dalitz plot

J. R. Batley, A. J. Culling, G. Kalmus +118

As first observed by the NA48/2 experiment at the CERN SPS, the $\p0p0$ invariant mass (M00) distribution from $\kcnn$ decay shows a cusp-like anomaly at M00=2m+, where m+ is the c…

astro-ph2006

The Araucaria Project. The Distance to the Sculptor Group Galaxy NGC 55 from a Newly Discovered Abundant Cepheid Population

G. Pietrzynski, W. Gieren, I. Soszynski +10

We have detected, for the first time, Cepheid variables in the Sculptor Group SB(s)m galaxy NGC 55. From wide-field images obtained in the optical V and I bands during 77 nights in…

astro-ph.GA2014

The globular cluster NGC 6528 the ferrous side of the Galactic Bulge

E. P. Lagioia, A. P. Milone, G. Bono +12

We present new and accurate optical photometry of the Bulge globular cluster NGC 6528. The images were collected with ACS at HST and together with WFC3 (UVIS, IR) allowed us to mea…

astro-ph2008

The Araucaria Project: The Distance to the Sculptor Group Galaxy NGC 247 from Cepheid Variables Discovered in a Wide-Field

A. Garcia-Varela, G. Pietrzynski, W. Gieren +9

We report on the discovery of a Cepheid population in the Sculptor Group spiral galaxy NGC 247 for the first time. On the basis of wide-field images collected in photometric survey…