papers

Publications (17)

astro-ph.IM2019

Binospec: A Wide-field Imaging Spectrograph for the MMT

Daniel Fabricant, Robert Fata, Harland Epps +14

Binospec is a high throughput, 370 to 1000 nm, imaging spectrograph that addresses two adjacent 8' by 15' fields of view. Binospec was commissioned in late 2017 at the f/5 focus of…

astro-ph.IM2020

Getting Ready for LISA: The Data, Support and Preparation Needed to Maximize US Participation in Space-Based Gravitational Wave Science

Kelly Holley-Bockelmann, :, Jillian Bellovary +20

The NASA LISA Study Team was tasked to study how NASA might support US scientists to participate and maximize the science return from the Laser Interferometer Space Antenna (LISA)…

astro-ph.SR2018

A quantitative spectral analysis of 14 hypervelocity stars from the MMT survey

Andreas Irrgang, Simon Kreuzer, Ulrich Heber +1

Hypervelocity stars (HVSs) travel so fast that they may leave the Galaxy. The tidal disruption of a binary system by the supermassive black hole in the Galactic center is widely as…

astro-ph.IM2015

Data Reduction Pipeline for the MMT and Magellan Infrared Spectrograph

Igor Chilingarian, Yuri Beletsky, Sean Moran +3

We describe the new spectroscopic data reduction pipeline for the multi-object MMT/Magellan Infrared Spectrograph. The pipeline is implemented in idl as a stand-alone package and i…

astro-ph.IM2021

Faint objects in motion: the new frontier of high precision astrometry

Fabien Malbet, Céline Boehm, Alberto Krone-Martins +83

Sky survey telescopes and powerful targeted telescopes play complementary roles in astronomy. In order to investigate the nature and characteristics of the motions of very faint ob…

astro-ph.IM2017

Theia: Faint objects in motion or the new astrometry frontier

The Theia Collaboration, Celine Boehm, Alberto Krone-Martins +96

In the context of the ESA M5 (medium mission) call we proposed a new satellite mission, Theia, based on relative astrometry and extreme precision to study the motion of very faint…

astro-ph.SR2025

The Emerging Class of Double-Faced White Dwarfs

Adam Moss, Mukremin Kilic, Pierre Bergeron +2

We report our findings on a spectroscopic survey of seven unresolved DA+DB binary white dwarf candidates. We have discovered extreme spectroscopic variations in one of these candid…

astro-ph.IM2012

Data reduction pipeline for the MMT Magellan Infrared Spectrograph

Igor Chilingarian, Warren Brown, Daniel Fabricant +3

We describe principal components of the new spectroscopic data pipeline for the multi-object MMT/Magellan Infrared Spectrograph (MMIRS). The pipeline is implemented in IDL and C++.…

astro-ph.GA2025

Hypervelocity Stars Trace a Supermassive Black Hole in the Large Magellanic Cloud

Jiwon Jesse Han, Kareem El-Badry, Scott Lucchini +5

Hypervelocity stars (HVSs) are produced by the Hills mechanism when a stellar binary is disrupted by a supermassive black hole (SMBH). The HVS Survey detected 21 unbound B-type mai…

astro-ph.IM2023

NANCY: Next-generation All-sky Near-infrared Community surveY

Jiwon Jesse Han, Arjun Dey, Adrian M. Price-Whelan +206

The Nancy Grace Roman Space Telescope is capable of delivering an unprecedented all-sky, high-spatial resolution, multi-epoch infrared map to the astronomical community. This oppor…

astro-ph.CO2009

Properties of Dark Matter Revealed by Astrometric Measurements of the Milky Way and Local Galaxies

Edward Shaya, Robert Olling, Massimo Ricotti +19

The fact that dark matter (DM), thus far, has revealed itself only on scales of galaxies and larger, again thrusts onto astrophysics the opportunity and the responsibility to confr…

astro-ph.SR2018

A Serendipitous Pulsar Discovery in a Search for a Companion to a Low-Mass White Dwarf

Jeff J. Andrews, Marcel A. Agüeros, Fernando Camilo +4

We report the discovery of a previously unidentified pulsar as part of a radio campaign to identify neutron star companions to low-mass white dwarfs (LMWDs) using the Robert C.\ By…

astro-ph2008

Hypervelocity Stars: Young and Heavy or Old and Light?

Uli Heber, Heiko Hirsch, Heinz Edelmann +4

The first three hyper-velocity stars (HVS) unbound to the Galaxy were serendipitously discovered in 2005. The only suggested origin of hyper-velocity stars is the Galactic Centre a…

astro-ph.SR2023

Signs of Binary Evolution in 7 Magnetic DA White Dwarfs

Adam Moss, Mukremin Kilic, P. Bergeron +2

We present our findings on the spectral analysis of seven magnetic white dwarfs that were presumed to be double degenerates. We obtained time-resolved spectroscopy at the Gemini Ob…

astro-ph.SR2014

The Most Distant Stars in the Milky Way

John J. Bochanski, Beth Willman, Nelson Caldwell +4

We report on the discovery of the most distant Milky Way (MW) stars known to date: ULAS J001535.72015549.6 and ULAS J074417.48253233.0. These stars were selected as M giant c…

astro-ph.IM2012

MMT & Magellan Infrared Spectrograph

Brian McLeod, Daniel Fabricant, George Nystrom +19

The MMT and Magellan infrared spectrograph (MMIRS) is a cryogenic multiple slit spectrograph operating in the wavelength range 0.9-2.4 micron. MMIRS' refractive optics offer a 6.9…

astro-ph.IM2019

Building A Field: The Future of Astronomy with Gravitational Waves, A State of The Profession Consideration for Astro2020

Kelly Holley-Bockelmann, Joey Shapiro Key, Brittany Kamai +28

Harnessing the sheer discovery potential of gravitational wave astronomy will require bold, deliberate, and sustained efforts to train and develop the requisite workforce. The next…