papers

Publications (17)

astro-ph.SR2022

Perfecting our set of spectrophotometric standard DA white dwarfs

A. Calamida, T. Matheson, E. W. Olszewski +17

We verified for photometric stability a set of DA white dwarfs with Hubble Space Telescope magnitudes from the near-ultraviolet to the near-infrared and ground-based spectroscopy b…

astro-ph.HE2016

Repetitive Patterns in Rapid Optical Variations in the Nearby Black-hole Binary V404 Cygni

Mariko Kimura, Keisuke Isogai, Taichi Kato +65

How black holes accrete surrounding matter is a fundamental, yet unsolved question in astrophysics. It is generally believed that matter is absorbed into black holes via accretion…

astro-ph.IM2025

DAmodel: Hierarchical Bayesian Modelling of DA White Dwarfs for Spectrophotometric Calibration

Benjamin M. Boyd, Gautham Narayan, Kaisey S. Mandel +17

We use hierarchical Bayesian modelling to calibrate a network of 32 all-sky faint DA white dwarf (DA WD) spectrophotometric standards () alongside three CALSPEC st…

astro-ph.SR2023

All-Sky Faint DA White Dwarf Spectrophotometric Standards for Astrophysical Observatories: The Complete Sample

Tim Axelrod, Abhijit Saha, Thomas Matheson +14

Hot DA white dwarfs have fully radiative pure hydrogen atmospheres that are the least complicated to model. Pulsationally stable, they are fully characterized by their effective te…

astro-ph.IM2014

ANTARES: A Prototype Transient Broker System

Abhijit Saha, Thomas Matheson, Richard Snodgrass +5

The Arizona-NOAO Temporal Analysis and Response to Events System (ANTARES) is a joint project of the National Optical Astronomy Observatory and the Department of Computer Science a…

astro-ph.IM2016

ANTARES: Progress towards building a `Broker' of time-domain alerts

Abhijit Saha, Zhe Wang, Thomas Matheson +13

The Arizona-NOAO Temporal Analysis and Response to Events System (ANTARES) is a joint effort of NOAO and the Department of Computer Science at the University of Arizona to build pr…

astro-ph.IM2016

Improving LSST Photometric Calibration with Gaia Data

Tim Axelrod, Calder Miller

We consider the possibility that the Gaia mission can supply data which will improve the photometric calibration of LSST. After outlining the LSST calibra- tion process and the inf…

astro-ph2002

Statistical Methods for Detecting Stellar Occultations by Kuiper Belt Objects: the Taiwanese-American Occultation Survey

Chyng-Lan Liang, John A. Rice, Imke de Pater +3

The Taiwanese-American Occultation Survey (TAOS) will detect objects in the Kuiper Belt, by measuring the rate of occultations of stars by these objects, using an array of three to…

astro-ph.IM2019

Sub-percent Photometry: Faint DA White Dwarf Spectophotometric Standards for Astrophysical Observatories

Gautham Narayan, Thomas Matheson, Abhijit Saha +18

We have established a network of 19 faint (16.5 mag 19 mag) northern and equatorial DA white dwarfs as spectrophotometric standards for present and future wide-field observ…

astro-ph.EP2019

First Results from the rapid-response spectrophotometric characterization of Near-Earth Objects

Samuel Navarro-Meza, Michael Mommert, David Trilling +6

As part of our multi-observatory, multi-filter campaign, we present \rmi color observations of 82 Near-Earth Objects (NEOs) obtained with the RATIR instrument on the 1.5m robotic t…

astro-ph2005

The Proper Motion of the Large Magellanic Cloud using HST

Nitya Kallivayalil, Roeland P. van der Marel, Charles Alcock +4

We present a measurement of the systemic proper motion of the Large Magellanic Cloud (LMC) from astrometry with the High Resolution Camera (HRC) of the Advanced Camera for Surveys…

astro-ph.EP2017

The Large Synoptic Survey Telescope as a Near-Earth Object Discovery Machine

R. Lynne Jones, Colin T. Slater, Joachim Moeyens +7

Using the most recent prototypes, design, and as-built system information, we test and quantify the capability of the Large Synoptic Survey Telescope (LSST) to discover Potentially…

astro-ph.IM2015

Delivering SKA Science

Peter Quinn, Tim Axelrod, Ian Bird +3

The SKA will be capable of producing a stream of science data products that are Exa-scale in terms of their storage and processing requirements. This Google-scale enterprise is att…

astro-ph.SR2016

Towards a Network of Faint DA White Dwarfs as High-Precision Spectrophotometric Standards

Gautham Narayan, Tim Axelrod, Jay B. Holberg +8

We present initial results from a program aimed at establishing a network of hot DA white dwarfs to serve as spectrophotometric standards for present and future wide-field surveys.…

astro-ph.SR2017

Absolute Magnitudes and Colors of RR Lyrae stars in DECam Passbands from Photometry of the Globular Cluster M5

A. Katherina Vivas, Abhijit Saha, Knut Olsen +10

We characterize the absolute magnitudes and colors of RR Lyrae stars in the globular cluster M5 in the ugriz filter system of the Dark Energy Camera (DECam). We provide empirical P…

astro-ph.IM2026

Attaining Spectral Energy Distributions With Sub-Percent Uncertainties: All-Sky DA White Dwarf Spectrophotometric Standard Stars For Large Telescopes And Surveys

Abhijit Saha, Edward W. Olszewski, Benjamin M. Boyd +14

We present a synopsis of the project to establish thirty-two new faint () DA white dwarfs as spectrophotometric standards distributed over the whole sky. O…

astro-ph.IM2018

Machine Learning-based Brokers for Real-time Classification of the LSST Alert Stream

Gautham Narayan, Tayeb Zaidi, Monika D. Soraisam +20

The unprecedented volume and rate of transient events that will be discovered by the Large Synoptic Survey Telescope (LSST) demands that the astronomical community update its follo…