KMap
Dr. David Sand is an observational astronomer with a variety of interests. He spends a lot of his time searching for and understanding the smallest galaxies in the Universe, as they are extremely dark matter dominated and are signposts for structure formation. Dr. Sand is also broadly interested in time domain astronomy, and in particular understanding the progenitors and explosion mechanisms of supernovae. Dr. Sand does some instrument development to further his team's scientific goals.

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Courses
  • SFSEOP
    Seminiar with a Focus on Stellar Evolution from an Observational Perspective

  • SDG
    Structure and Dynamics of Galaxies

  • SFSEOP
    Seminar with a Focus on Stellar Evolution from an Observational Perspective

  • S
    Stars

  • FA
    Fundamentals of Astronomy

Grants
  • Funding agency logo
    The First Early FUV Observations of a Type IIP Supernova

    Principal Investigator (PI)

    2023

    $23.8K
    Active
  • Funding agency logo
    Gas Content of a New Class of Stellar System in the Virgo Cluster

    Principal Investigator (PI)

    2023

    $11.2K
    Active
  • Funding agency logo
    Collaborative Research: Dwarf Galaxies Over Cosmic Time

    Principal Investigator (PI)

    2022

    $271.5K
    Active
  • Funding agency logo
    Bringing Supernova Light-Curve Modeling into the LSST Era

    Principal Investigator (PI)

    2022

    $85.0K
    Active
  • Funding agency logo
    Ultra-Diffuse Galaxy Formation in Groups -- Tidal or Born That Way?

    Principal Investigator (PI)

    2022

    $43.6K
    Active
  • Funding agency logo
    Completing the Picture: The Globular Cluster Systems of Field Ultra-Diffuse Galaxies

    Principal Investigator (PI)

    2022

    $11.0K
    Active
  • Funding agency logo
    WoU-MMA: An Integrated Time Domain System for Discovery and Fast Follow-up of Gravitational Wave Events and Other Transients

    Principal Investigator (PI)

    2021

    $875.4K
    Active
  • Funding agency logo
    Progenitors and Explosions of TESS Supernovae

    Principal Investigator (PI)

    2021

    $70.0K
    Active
  • Funding agency logo
    The NGC253 Satellite Luminosity Function: A Case Study for Low Density Environments

    Principal Investigator (PI)

    2021

    $46.7K
    Active
  • Funding agency logo
    Confirming a Failed Supernova Candidate in M51

    Principal Investigator (PI)

    2021

    $41.6K
    Active
News
  • Mysterious 'blue blobs' reveal a new kind of star system

    2022

  • Ripples in Space: The Little Telescope That Could

    2017

  • In Hunting Supernovae, 'Get Them While They're Young'

    2017

Publications (139)
Recent
  • Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-Faint Dwarf Galaxy in the Constellation Pegasus

    2022

  • Weak Mass Loss from the Red Supergiant Progenitor of the Type II SN 2021yja

    2022

  • Infant-phase reddening by surface Fe-peak elements in a normal type Ia supernova

    2022

  • The DECam Local Volume Exploration Survey Data Release 2

    2022

  • Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae

    2022

  • Hubble Space Telescope Observations of NGC 253 Dwarf Satellites: Three Ultra-faint Dwarf Galaxies

    2022

  • Nebular-phase spectra of Type Ia supernovae from the Las Cumbres Observatory Global Supernova Project

    2022

  • AGC 226178 and NGVS 3543: Two Deceptive Dwarfs toward Virgo

    2022

  • Hubble Space Telescope Imaging of Isolated Local Volume Dwarfs GALFA Dw3 and Dw4

    2022

  • A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers during the Third Gravitational-wave Observing Run

    2022

  • The LBT satellites of Nearby Galaxies Survey (LBT-SONG): the satellite population of NGC 628

    2021

  • The Early Discovery of SN 2017ahn: Signatures of Persistent Interaction in a Fast-declining Type II Supernova

    2021

  • AT 2019qyl in NGC 300: Internal Collisions in the Early Outflow from a Very Fast Nova in a Symbiotic Binary

    2021

  • H\ensuremath{\alpha} Reverberation Mapping of the Intermediate-mass Active Galactic Nucleus in NGC 4395

    2021

  • SN 2017fgc: A Fast-expanding Type Ia Supernova Exploded in Massive Shell Galaxy NGC 474

    2021

  • Introducing the LBT Imaging of Galactic Halos and Tidal Structures (LIGHTS) survey. A preview of the low surface brightness Universe to be unveiled by LSST

    2021

  • SN 2019muj - a well-observed Type Iax supernova that bridges the luminosity gap of the class

    2021

  • The Blue Supergiant Progenitor of the Supernova Imposter AT 2019krl

    2021

  • Satellites around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations versus Simulations

    2021

  • NGC 5128 Globular Cluster Candidates Out to 150 kpc: A Comprehensive Catalog from Gaia and Ground-based Data

    2021

  • Circumstellar Medium Constraints on the Environment of Two Nearby Type Ia Supernovae: SN 2017cbv and SN 2020nlb

    2021

  • An Exceptional Dimming Event for a Massive, Cool Supergiant in M51

    2021

  • Forbidden hugs in pandemic times. II. The luminous red nova variety: AT 2020hat and AT 2020kog

    2021

  • Hubble Space Telescope Imaging of Isolated Local Volume Dwarfs GALFA-Dw3 and Dw4

    2021

  • A Bright Ultraviolet Excess in the Transitional 02es-like Type Ia Supernova 2019yvq

    2021

  • RR Lyrae Stars in the Newly Discovered Ultra-faint Dwarf Galaxy Centaurus I

    2021

  • AT 2020iko: A WZ Sge-type Dwarf Nova Candidate with an Anomalous Precursor Event

    2021

  • Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH

    2021

  • An impostor among us II: Progenitor, environment, and modelling of AT 2016jbu

    2021

  • Eridanus IV: an Ultra-faint Dwarf Galaxy Candidate Discovered in the DECam Local Volume Exploration Survey

    2021

  • Evidence for multiple origins of fast declining Type II supernovae from spectropolarimetry of SN 2013ej and SN 2017ahn

    2021

  • ASASSN-15hy: An Underluminous, Red 03fg-like Type Ia Supernova

    2021

  • Resolved Dwarf Galaxy Searches within 5 Mpc with the Vera Rubin Observatory and Subaru Hyper Suprime-Cam

    2021

  • A population of luminous globular clusters and stripped nuclei with elevated mass to light ratios around NGC 5128

    2021

  • The DECam Local Volume Exploration Survey: Overview and First Data Release

    2021

  • Carnegie Supernova Project: The First Homogeneous Sample of Super-Chandrasekhar-mass/2003fg-like Type Ia Supernovae

    2021

  • AT 2019qyl in NGC 300: Early Outflow Collisions for a Very Fast Nova in a Symbiotic Binary

    2021

  • An impostor among us I: Photometric and spectroscopic evolution of AT 2016jbu

    2021

  • Discovery of an Ultra-faint Stellar System near the Magellanic Clouds with the DECam Local Volume Exploration Survey

    2021

  • Eridanus II: A Fossil from Reionization with an Off-center Star Cluster

    2021

  • Evidence for Ultra-diffuse Galaxy Formation through Tidal Heating of Normal Dwarfs

    2021

  • Supernova 2018cuf: A Type IIP Supernova with a Slow Fall from Plateau

    2020

  • Constraining the Source of the High-velocity Ejecta in Type Ia SN 2019ein

    2020

  • The Elusive Distance Gradient in the Ultrafaint Dwarf Galaxy Hercules: A Combined Hubble Space Telescope and Gaia View

    2020

  • Hubble Space Telescope Imaging of Antlia B: Star Formation History and a New Tip of the Red Giant Branch Distance

    2020

  • Optical and Near-infrared Observations of the Nearby SN Ia 2017cbv

    2020

  • Neutral Hydrogen Observations of Low Surface Brightness Galaxies around M101 and NGC 5485

    2020

  • SN 2014ab: an aspherical Type IIn supernova with low polarization

    2020

  • Robotic reverberation mapping of the broad-line radio galaxy 3C 120

    2020

  • Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run

    2020

  • SN 2019ehk: A Double-peaked Ca-rich Transient with Luminous X-Ray Emission and Shock-ionized Spectral Features

    2020

  • The Satellite Luminosity Function of M101 into the Ultra-faint Dwarf Galaxy Regime

    2020

  • A Mildly Relativistic Outflow from the Energetic, Fast-rising Blue Optical Transient CSS161010 in a Dwarf Galaxy

    2020

  • Two Ultra-faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey

    2020

  • Strong Near-Infrared Carbon Absorption in the Transitional Type Ia SN 2015bp

    2020

  • The luminous red nova variety: AT 2020hat and AT 2020kog

    2020

  • The case for strangulation in low-mass hosts: DDO 113

    2020

  • The electron-capture origin of supernova 2018zd

    2020

  • SN 2013aa and SN 2017cbv: Two Sibling Type Ia Supernovae in the Spiral Galaxy NGC 5643

    2020

  • The Steward Alerts for Science System (SASSy)

    2020

  • The Gravitational Wave Treasure Map: A Tool to Coordinate, Visualize, and Assess the Electromagnetic Follow-Up of Gravitational Wave Events

    2020

  • A Gaia-based Catalog of Candidate Stripped Nuclei and Luminous Globular Clusters in the Halo of Centaurus A

    2020

  • The progenitor of the supernova imposter AT 2019krl: a SN 2008S-like transient from a blue supergiant

    2020

  • The long-lived Type IIn SN 2015da: Infrared echoes and strong interaction within an extended massive shell

    2020

  • SN 2017gmr: An Energetic Type II-P Supernova with Asymmetries

    2019

  • Multi-Messenger Astronomy with Extremely Large Telescopes

    2019

  • K2 Observations of SN 2018oh Reveal a Two-component Rising Light Curve for a Type Ia Supernova

    2019

  • Carnegie Supernova Project-II: The Near-infrared Spectroscopy Program

    2019

  • Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068

    2019

  • Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo\textquoterights Third Observing Run

    2019

  • A new class of flares from accreting supermassive black holes

    2019

  • A Physical Basis for the H-band Blue-edge Velocity and Light-curve Shape Correlation in Context of Type Ia Supernova Explosion Physics

    2019

  • The Type II-P Supernova 2017eaw: From Explosion to the Nebular Phase

    2019

  • The Wide Field Infrared Survey Telescope: 100 Hubbles for the 2020s

    2019

  • Evidence for a Chandrasekhar-mass explosion in the Ca-strong 1991bg-like type Ia supernova 2016hnk

    2019

  • The Young and Nearby Normal Type Ia Supernova 2018gv: UV-Optical Observations and the Earliest Spectropolarimetry

    2019

  • The M101 Satellite Luminosity Function and the Halo─Halo Scatter among Local Volume Hosts

    2019

  • The Lick AGN Monitoring Project 2011: Photometric Light Curves

    2019

  • CCCP and MENeaCS: (updated) weak-lensing masses for 100 galaxy clusters

    2019

  • Signatures of circumstellar interaction in the Type IIL supernova ASASSN-15oz

    2019

  • The aspherical explosion of the Type IIP SN 2017gmr$^{\textdagger}$

    2019

  • WFIRST: Enhancing Transient Science and Multi-Messenger Astronomy

    2019

  • Carnegie Supernova Project-II: Using Near-infrared Spectroscopy to Determine the Location of the Outer $^56$Ni in Type Ia Supernovae

    2019

  • Uncovering the Orbit of the Hercules Dwarf Galaxy

    2019

  • ASTRO2020 White Paper: JWST: Probing the Epoch of Reionization with a Wide Field Time-Domain Survey

    2019

  • Astro2020 Science White Paper: Radio Counterparts of Compact Object Mergers in the Era of Gravitational-Wave Astronomy

    2019

  • Hyper Wide Field Imaging of the Local Group Dwarf Irregular Galaxy IC 1613: An Extended Component of Metal-poor Stars

    2019

  • Tidal Destruction in a Low-mass Galaxy Environment: The Discovery of Tidal Tails around DDO 44

    2019

  • Optical Follow-up of Gravitational-wave Events during the Second Advanced LIGO/VIRGO Observing Run with the DLT40 Survey

    2019

  • Nebular Hensuremath{alpha} Limits for Fast Declining SNe Ia

    2019

  • The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin

    2019

  • The Faint End of the Centaurus A Satellite Luminosity Function

    2019

  • Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the Kepler 2 Observations

    2019

  • Carnegie Supernova Project-II: Near-infrared Spectroscopic Diversity of Type II Supernovae

    2019

  • Signatures of Tidal Disruption in Ultra-faint Dwarf Galaxies: A Combined HST, Gaia, and MMT/Hectochelle Study of Leo V

    2019

  • Nebular Spectroscopy of the \ldquoBlue Bump\rdquo Type Ia Supernova 2017cbv

    2018

  • Continuum Reverberation Mapping of the Accretion Disks in Two Seyfert 1 Galaxies

    2018

  • Target of Opportunity Observations of Gravitational Wave Events with LSST

    2018

  • Bo\ otes III is a Disrupting Dwarf Galaxy Associated with the Styx Stellar Stream

    2018

  • Near-infrared Spectral Evolution of the Type Ia Supernova 2014J in the Nebular Phase: Implications for the Progenitor System

    2018

  • A nearby super-luminous supernova with a long pre-maximum \amp ``plateau'' and strong C II features

    2018

  • Stability of the Broad-line Region Geometry and Dynamics in Arp 151 Over Seven Years

    2018

  • SN 2016coi/ASASSN-16fp: an example of residual helium in a typeIc supernova?

    2018

  • Evidence for Ultra-diffuse Galaxy \ldquoFormation\rdquo through Galaxy Interactions

    2018

  • Red and Reddened: Ultraviolet through Near-Infrared Observations of Type Ia Supernova 2017erp

    2018

  • An Excess of Low-mass X-Ray Binaries in the Outer Halo of NGC 4472

    2018

  • Chandra X-ray constraints on the candidate Ca-rich gap transient SN 2016hnk

    2018

  • A Deeper Look at the New Milky Way Satellites: Sagittarius II, Reticulum II, Phoenix II, and Tucana III

    2018

  • Science with an ngVLA: Compact binary mergers as traced by gravitational waves

    2018

  • The Early Detection and Follow-up of the Highly Obscured Type II Supernova 2016ija/DLT16am

    2018

  • Development of the Arizona Robotic Telescope Network

    2018

  • Reverberation Mapping of Optical Emission Lines in Five Active Galaxies

    2017

  • Constraints on the Progenitor of SN 2016gkg from Its Shock-cooling Light Curve

    2017

  • Discovery of Diffuse Dwarf Galaxy Candidates around M101

    2017

  • 2FGL J0846.0+2820: A New Neutron Star Binary with a Giant Secondary and Variable {$gamma$-Ray Emission}

    2017

  • Light and Color Curve Properties of Type Ia Supernovae: Theory Versus Observations

    2017

  • A gravitational-wave standard siren measurement of the Hubble constant

    2017

  • Multi-messenger Observations of a Binary Neutron Star Merger

    2017

  • SN 2016coi/ASASSN-16fp: An example of residual helium in a type Ic supernova?

    2017

  • Type Ibn Supernovae Show Photometric Homogeneity and Spectral Diversity at Maximum Light

    2017

  • Rise and fall of the dust shell of the classical nova V339 Delphini

    2017

  • Numerically Modeling the First Peak of the Type IIb SN 2016gkg

    2017

  • A First Transients Survey with JWST: the FLARE project

    2017

  • An Empirical Limit on the Kilonova Rate from the DLT40 One Day Cadence Supernova Survey

    2017

  • Host galaxies and relativistic ejecta of compact binary mergers in the ngVLA era

    2017

  • The Faint Globular Cluster in the Dwarf Galaxy Andromeda I

    2017

  • Dynamical evidence for a strong tidal interaction between the Milky Way and its satellite, Leo V

    2017

  • Early Blue Excess from the Type Ia Supernova 2017cbv and Implications for Its Progenitor

    2017

  • Structural and Photometric Properties of the Andromeda Satellite Dwarf Galaxy Lacerta I from Deep Imaging with WIYN PODI

    2017

  • The Progenitor and Early Evolution of the Type IIb SN 2016gkg

    2017

  • Nebular-phase spectra of nearby Type Ia Supernovae

    2017

  • Type Ia Supernovae: Colors, Rates, and Progenitors

    2017

  • Deep Subaru Hyper Suprime-Cam Observations of Milky Way Satellites Columba I and Triangulum II

    2017

  • Hubble Space Telescope Imaging of the Ultra-compact High Velocity Cloud AGC 226067: A Stripped Remnant in the Virgo Cluster

    2017

  • The Discovery of the Electromagnetic Counterpart of GW170817: Kilonova AT 2017gfo/DLT17ck

    2017

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