papers

Publications (13)

astro-ph.IM2019

The Maunakea Spectroscopic Explorer

Jennifer Marshall, James Bullock, Adam Burgasser +23

The Maunakea Spectroscopic Explorer is a next-generation massively multiplexed spectroscopic facility currently under development in Hawaii. It is completely dedicated to large-sca…

astro-ph.GA2022

Discovery of a new Local Group Dwarf Galaxy Candidate in UNIONS: Boötes V

Simon E. T. Smith, Jaclyn Jensen, Joel Roediger +12

We present the discovery of Boötes V, a new ultra-faint dwarf galaxy candidate. This satellite is detected as a resolved overdensity of stars during an ongoing search for new Loca…

astro-ph.GA2018

The APOGEE-2 Survey of the Orion Star Forming Complex: I. Target Selection and Validation with early observations

J'Neil Cottle, Kevin R. Covey, Genaro Suárez +26

The Orion Star Forming Complex (OSFC) is a central target for the APOGEE-2 Young Cluster Survey. Existing membership catalogs span limited portions of the OSFC, reflecting the diff…

astro-ph.GA2025

Deep in the Fields of the Andromeda Halo: Discovery of the Pegasus VII dwarf galaxy in UNIONS

Simon E. T. Smith, Alan W. McConnachie, Stephen Gwyn +8

We present the newly discovered dwarf galaxy Pegasus VII (Peg VII), a member of the M31 sub-group which has been uncovered in the photometric catalogs from the Ultraviolet Nea…

astro-ph.CO2022

The Pantheon+ Analysis: The Full Dataset and Light-Curve Release

Dan Scolnic, Dillon Brout, Anthony Carr +27

Here we present 1701 light curves of 1550 spectroscopically confirmed Type Ia supernovae (SNe Ia) that will be used to infer cosmological parameters as part of the Pantheon+ SN ana…

astro-ph.GA2018

The Profile of the Galactic Halo from Pan-STARRS1 3 RR Lyrae

Nina Hernitschek, Judith G. Cohen, Hans-Walter Rix +11

We characterize the spatial density of the Pan-STARRS1 (PS1) sample of RR Lyrae stars, to study the properties of the old Galactic stellar halo as traced by RRab stars. This sample…

astro-ph.GA2023

The discovery of the faintest known Milky Way satellite using UNIONS

Simon E. T. Smith, William Cerny, Christian R. Hayes +14

We present the discovery of Ursa Major III/UNIONS 1, the least luminous known satellite of the Milky Way, which is estimated to have an absolute V-band magnitude of $+2.2^{+0.4}_{-…

astro-ph.EP2015

Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - preliminary results

Peter Vereš, Robert Jedicke, Alan Fitzsimmons +14

We present the results of a Monte Carlo technique to calculate the absolute magnitudes (H) and slope parameters (G) of about 240000 asteroids observed by the Pan-STARRS1 telescope…

astro-ph.CO2011

The First High Redshift Quasar from Pan-STARRS

Eric Morganson, Gisella De Rosa, Roberto Decarli +13

We present the discovery of the first high redshift (z > 5.7) quasar from the Panoramic Survey Telescope and Rapid Response System 1 (Pan-STARRS1 or PS1). This quasar was initially…

astro-ph.HE2020

The lowest of the low: discovery of SN 2019gsc and the nature of faint Iax supernovae

Shubham Srivastav, Stephen J. Smartt, Giorgos Leloudas +15

We present the discovery and optical follow-up of the faintest supernova-like transient known. The event (SN 2019gsc) was discovered in a star-forming host at 53\,Mpc by ATLAS. A d…

astro-ph.GA2019

The Sloan Digital Sky Survey Reverberation Mapping Project: Sample Characterization

Yue Shen, Patrick B. Hall, Keith Horne +24

We present a detailed characterization of the 849 broad-line quasars from the Sloan Digital Sky Survey Reverberation Mapping (SDSS-RM) project. Our quasar sample covers a redshift…

astro-ph.CO2022

The Pantheon+ Analysis: Cosmological Constraints

Dillon Brout, Dan Scolnic, Brodie Popovic +43

We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves of 1550 distinct Type Ia supernovae (SNe Ia) ranging in redshift from t…

astro-ph.GA2018

A Color-locus Method for Mapping Using Ensembles of Stars

Albert Lee, Gregory M. Green, Edward F. Schlafly +11

We present a simple but effective technique for measuring angular variation in across the sky. We divide stars from the Pan-STARRS1 catalog into Healpix pixels and determine…