Showing 2014 · astro-ph.IMShow all

48 papers · 2 filters

astro-ph.IM2014

All Sky Survey Mission Observing Scenario Strategy

Sara C. Spangelo, Raj M. Katti, Stephen C. Unwin +1

This paper develops a general observing strategy for missions performing all-sky surveys, where a single spacecraft maps the celestial sphere subject to realistic constraints. The…

astro-ph.IM2014★ 7 cited

Dark Ages Radio Explorer Mission: Probing the Cosmic Dawn

Dayton L. Jones, T. Joseph W. Lazio, Jack O. Burns

The period between the creation of the cosmic microwave background at a redshift of ~1000 and the formation of the first stars and black holes that re-ionize the intergalactic medi…

astro-ph.IM2014★ 4 cited

Annular Groove Phase Mask coronagraph in diamond for mid-IR wavelengths: manufacturing assessment and performance analysis

Christian Delacroix, Pontus Forsberg, Mikael Karlsson +7

Phase-mask coronagraphs are known to provide high contrast imaging capabilities while preserving a small inner working angle, which allows searching for exoplanets or circumstellar…

astro-ph.IM2014★ 8 cited

Normal Metal Hot-Electron Nanobolometer with Johnson Noise Thermometry Readout

Boris S. Karasik, Christopher B. McKitterick, Theodore J. Reck +1

The sensitivity of a THz hot-electron nanobolometer (nano-HEB) made from a normal metal is analyzed. Johnson Noise Thermometry (JNT) is employed as a readout technique. In contrast…

astro-ph.IM2014★ 3 cited

Digital Signal Processing using Stream High Performance Computing: A 512-input Broadband Correlator for Radio Astronomy

J. Kocz, L. J Greenhill, B. R. Barsdell +16

A "large-N" correlator that makes use of Field Programmable Gate Arrays and Graphics Processing Units has been deployed as the digital signal processing system for the Long Wavelen…

astro-ph.IM2014★ 47 cited

Modelling the Transfer Function for the Dark Energy Survey

C. Chang, M. T. Busha, R. H. Wechsler +40

We present a forward-modelling simulation framework designed to model the data products from the Dark Energy Survey (DES). This forward-model process can be thought of as a transfe…

astro-ph.IM2014★ 27 cited

Astrometry of Cassini with the VLBA to Improve the Saturn Ephemeris

Dayton L. Jones, William M. Folkner, Robert A. Jacobson +4

Planetary ephemerides have been developed and improved over centuries. They are a fundamental tool for understanding solar system dynamics, and essential for planetary and small bo…

astro-ph.IM2014★ 30 cited

The Overlooked Potential of Generalized Linear Models in Astronomy-II: Gamma regression and photometric redshifts

J. Elliott, R. S. de Souza, A. Krone-Martins +3

Machine learning techniques offer a precious tool box for use within astronomy to solve problems involving so-called big data. They provide a means to make accurate predictions abo…

astro-ph.IM2014★ 39 cited

The Overlooked Potential of Generalized Linear Models in Astronomy - I: Binomial Regression

R. S. de Souza, E. Cameron, M. Killedar +6

Revealing hidden patterns in astronomical data is often the path to fundamental scientific breakthroughs; meanwhile the complexity of scientific inquiry increases as more subtle re…

astro-ph.IM2014★ 154 cited

Strong Lens Time Delay Challenge: II. Results of TDC1

Kai Liao, Tommaso Treu, Phil Marshall +23

We present the results of the first strong lens time delay challenge. The motivation, experimental design, and entry level challenge are described in a companion paper. This paper…

astro-ph.IM2014★ 6 cited

Prime Focus Instrument of Prime Focus Spectrograph for Subaru Telescope

Shiang-Yu Wang, David F. Braun, Mark A. Schwochert +18

The Prime Focus Spectrograph (PFS) is a new optical/near-infrared multi-fiber spectrograph design for the prime focus of the 8.2m Subaru telescope. PFS will cover 1.3 degree diamet…

astro-ph.IM2014★ 14 cited

Fiber Optical Cable and Connector System (FOCCoS) for PFS/Subaru

Antonio Cesar de Oliveira, Lígia Souza de Oliveira, Márcio V. de Arruda +29

FOCCoS, Fiber Optical Cable and Connector System, has the main function of capturing the direct light from the focal plane of Subaru Telescope using optical fibers, each one with a…

astro-ph.IM2014★ 24 cited

Developing Engineering Model Cobra fiber positioners for the Subaru Telescope Prime Focus Spectrometer

Charles Fisher, Chaz Morantz, David Braun +19

The Cobra fiber positioner is being developed by the California Institute of Technology (CIT) and the Jet Propulsion Laboratory (JPL) for the Prime Focus Spectrograph (PFS) instrum…

astro-ph.IM2014★ 4 cited

Progress with the Prime Focus Spectrograph for the Subaru Telescope: a massively multiplexed optical and near-infrared fiber spectrograph

Hajime Sugai, Naoyuki Tamura, Hiroshi Karoji +81

The Prime Focus Spectrograph (PFS) is an optical/near-infrared multi-fiber spectrograph with 2394 science fibers, which are distributed in 1.3 degree diameter field of view at Suba…

astro-ph.IM2014★ 2 cited

On-sky low order non-common path correction of the GPI Calibration Unit

Markus Hartung, Bruce Macintosh, Paul Langlois +12

The Gemini Planet Imager (GPI) entered on-sky commissioning phase, and had its First Light at the Gemini South telescope in November 2013. Meanwhile, the fast loops for atmospheric…

astro-ph.IM2014★ 54 cited

Low-rank approximations for large stationary covariance matrices, as used in the Bayesian and generalized-least-squares analysis of pulsar-timing data

Rutger van Haasteren, Michele Vallisneri

Many data-analysis problems involve large dense matrices that describe the covariance of stationary noise processes; the computational cost of inverting these matrices, or equivale…

astro-ph.IM2014★ 7 cited

Proper Motions of Young Stellar Outflows in the Mid-Infrared with Spitzer. II. HH 377/Cep E

A. Noriega-Crespo, A. C. Raga, A. Moro-Martin +2

We have used multiple mid-infrared observations at 4.5 micron obtained with the Infrared Array Camera, of the compact (~1.4 arcmin) young stellar bipolar outflow Cep E to measure t…

astro-ph.IM2014★ 86 cited

BICEP3: a 95 GHz refracting telescope for degree-scale CMB polarization

Z. Ahmed, M. Amiri, S. J. Benton +29

BICEP3 is a 550 mm-aperture refracting telescope for polarimetry of radiation in the cosmic microwave background at 95 GHz. It adopts the methodology of BICEP1, BICEP2 and the Keck…

astro-ph.IM2014★ 23 cited

Attitude determination for balloon-borne experiments

N. N. Gandilo, P. A. R. Ade, M. Amiri +64

An attitude determination system for balloon-borne experiments is presented. The system provides pointing information in azimuth and elevation for instruments flying on stratospher…

astro-ph.IM2014★ 5 cited

Automated Real-Time Classification and Decision Making in Massive Data Streams from Synoptic Sky Surveys

S. G. Djorgovski, A. A. Mahabal, C. Donalek +4

The nature of scientific and technological data collection is evolving rapidly: data volumes and rates grow exponentially, with increasing complexity and information content, and t…

astro-ph.IM2014★ 26 cited

Pre-flight integration and characterization of the SPIDER balloon-borne telescope

A. S. Rahlin, P. A. R. Ade, M. Amiri +45

We present the results of integration and characterization of the SPIDER instrument after the 2013 pre-flight campaign. SPIDER is a balloon-borne polarimeter designed to probe the…

astro-ph.IM2014★ 377 cited

Fundamental limitations of high contrast imaging set by small sample statistics

Dimitri Mawet, Julien Milli, Zahed Wahhaj +9

In this paper, we review the impact of small sample statistics on detection thresholds and corresponding confidence levels (CLs) in high contrast imaging at small angles. When look…

astro-ph.IM2014★ 4 cited

BLASTbus electronics: general-purpose readout and control for balloon-borne experiments

S. J. Benton, P. A. Ade, M. Amiri +66

We present the second generation BLASTbus electronics. The primary purposes of this system are detector readout, attitude control, and cryogenic housekeeping, for balloon-borne tel…

astro-ph.IM2014★ 14 cited

Pointing control for the SPIDER balloon-borne telescope

Jamil A. Shariff, Peter A. R. Ade, Mandana Amiri +45

We present the technology and control methods developed for the pointing system of the SPIDER experiment. SPIDER is a balloon-borne polarimeter designed to detect the imprint of pr…