activity
20242026
most citedLATIS: A Sample of IGM-selected Protoclusters and Protogroups at

4 citations · 12 across the 12 of their papers we have counts for

collaborators

14 papers

astro-ph.SR2026

The long period radio transient ASKAP J1448-68 is a cataclysmic variable

Geoffrey Mo, Akash Anumarlapudi, Iris de Ruiter +8

Wide-field time-domain radio surveys have recently unveiled a new class of Galactic radio emitter: long period radio transients (LPTs). Despite the rapid pace of discovery, their o…

astro-ph.IM2026

Update on the Magellan InfraRed Multi-Object Spectrograph (MIRMOS)

Maren Cosens, Nicholas P. Konidaris, Gwen C. Rudie +21

The Magellan InfraRed Multi-Object Spectrograph (MIRMOS) will be a next generation multi-object (MOS) and integral field spectrograph (IFS) for the 6.5m Magellan telescopes at Las…

astro-ph.IM2026

Update on the slicer IFU for the Magellan InfraRed Multi-Object Spectrograph (MIRMOS)

Maren Cosens, Patricio Schurter, Nicholas P. Konidaris +18

The Magellan InfraRed Multi-Object Spectrograph (MIRMOS) is a planned next generation multi-object and integral field spectrograph for the 6.5m Magellan telescopes at Las Campanas…

astro-ph.HE2026

A spectacular multi-wavelength transient associated with an off-axis relativistic jet

Delina Levine, Gregg Hallinan, Jean J. Somalwar +10

Many of the most luminous extragalactic transients originate from the accretion of material onto a black hole (BH) via core-collapse, stellar mergers, or the tidal disruption of a…

astro-ph.HE2026

A sample of short-lived Galactic radio transients from ASKAP VAST

Akash Anumarlapudi, David L. Kaplan, Natasha Hurley Walker +6

Galactic radio transients (GRTs) are mysterious short-lived (~days to months) radio transients that are quiet at all other wavelengths. Until now, roughly half a dozen such sources…

astro-ph.GA2025★ 1 cited

LATIS Data Release: Spectra of Galaxies, Redshifts, and Intergalactic Medium Tomography Maps

Andrew B. Newman, Gwen C. Rudie, Guillermo A. Blanc +8

We present the data release of the Ly Tomography IMACS Survey (LATIS), one of the largest optical spectroscopic surveys of faint high-redshift galaxies. The survey provides 7408…

astro-ph.GA2025

LATIS: Galaxy-Environment Relations at Cosmic Noon and the Role of Sample Selection

Nima Chartab, Andrew B. Newman, Gwen C. Rudie +6

We investigate the environmental dependence of galaxy properties at using the Ly Tomography IMACS Survey (LATIS), which provides high-resolution three-dimensional map…

astro-ph.HE2025★ 1 cited

A fast powerful X-ray transient from possible tidal disruption of a white dwarf

Dongyue Li, Wenda Zhang, Jun Yang +97

Stars captured by black holes (BHs) can be torn apart by strong tidal forces, producing electromagnetic flares. To date, more than 100 tidal disruption events (TDEs) have been obse…

astro-ph.GA2025★ 3 cited

LATIS: Comparing Galaxy and IGM Tomography Maps as Tracers of Large-scale Structure and Protoclusters at

Andrew B. Newman, Nima Chartab, Mahdi Qezlou +11

We investigate the consistency of intergalactic medium (IGM) tomography and galaxy surveys as tracers of the cosmic web and protoclusters at . We use maps from the Ly$α…

astro-ph.GA2025★ 4 cited

LATIS: A Sample of IGM-selected Protoclusters and Protogroups at

Andrew B. Newman, Mahdi Qezlou, Gwen C. Rudie +11

The Ly Tomography IMACS Survey (LATIS) has produced large 3D maps of the intergalactic medium (IGM), providing a new window on the cosmic web at . A key advantage of L…

astro-ph.HE2025

ASKAP J144834-685644: a newly discovered long period radio transient detected from radio to X-rays

Akash Anumarlapudi, David L. Kaplan, Nanda Rea +13

Long-period radio transients (LPTs) are an emerging group of radio transients that show periodic polarized radio bursts with periods varying from a few minutes to a few hours. Fewe…

astro-ph.GA2025★ 3 cited

A Bimodal Metallicity Distribution Function in the Ultra-Faint Dwarf Galaxy Reticulum II

Alice M. Luna, Alexander P. Ji, Anirudh Chiti +6

Star formation in ultra-faint dwarf galaxies (UFDs, ) is suppressed by reionization, but may not be completely quenched. The metallicity distribution function (MD…

astro-ph.IM2024

A Precision Cryogenic Positioning Stage for Detector Dithering and Flexure Compensation

Stephen A. Smee, Stephen C. Hope, Randolph P. Hammond +20

This paper presents the design and technical progress of a precision X-Y stage for detector dithering and flexure compensation. The stage is being developed for use in the Magellan…

astro-ph.IM2024

A Novel Freeform Slicer IFU for the Magellan InfraRed Multi-Object Spectrograph (MIRMOS)

Maren Cosens, Nicholas P. Konidaris, Gwen C. Rudie +16

The Magellan InfraRed Multi-Object Spectrograph (MIRMOS) is a planned next generation multi-object and integral field spectrograph for the 6.5m Magellan telescopes at Las Campanas…