SMA OBSERVER CENTER
 

Current A-ranked Projects

A-ranked projects with tracks in the queue or complete
Project IDP.I.TracksTitle (hover for abstract)
2025B-A001 Hau-Yu Baobab Liu4 Resolving the compact, dusty, inter-arm molecular clouds in M31
2025B-A002 Kuiyun Huang1 Electro-magnetic wave candidate of IceCube Neutrino event
2025B-A004 Tomoki Matsuoka2 A Target of Opportunity Observation of a Type IIn Supernova Revealing Unknown Mass Loss Activity of Massive Stars (copied from 2025A-A001)
2025B-S006 Joel Kastner2 Building an Understanding of the Intrinsic Structures of Planetary Nebulae: SMA CO Mapping of NGC 6072
2025B-S008 Sean Andrews23 A Microwave Continuum Survey of Taurus Protoplanetary Disks
2025B-S009 Anna Ho2 Millimeter-wavelength Monitoring of a Galactic Nova
2025B-S015 Joseph Michail18 Lights, Camera, Action! Filming Horizon-Scale Jet-Launching in M87 with Multi-Epoch VLBI
2025B-S018 Ioannis Myserlis2 SMAPOL: SMA Monitoring of AGNs with POLarization
2025B-S021 Jakob den Brok3 *COM*pleting SMA observations to study the drastic variation of alpha_CO in M101
2025B-S036 Lennart Boehm1 Magnetic fields driving or resisting OB cluster formation
2025B-S038 Joseph Michail1 DDT: AY191 Spectroscopic and Polarimetric Imaging of the Protobinary Source HOPS 361

B-ranked tracks with successful observations:
Project IDP.I.TracksTitle (hover for abstract)
2025B-S004 Luke Keyte1 The Quest for the Missing Sulfur: OCS in the Oph-IRS 48 Dust Trap
2025B-S010 Chi Yan Law3 Unveiling the magnetized path of massive star formation
2025B-S011 Beatrice Kulterer4 Chemistry of Low-Mass Protostars in Irradiated Environments
2025B-S012 Yun-A Jo1 Detecting Molecular Gas and High-Velocity Outflows in the Early Post-AGB Binary IRAS 07253-2001
2025B-S013 Jakob den Brok8 Resolved CO excitation across the Milky-Way Analog Galaxy IC342
2025B-S014 Chi Yan Law2 Polarized Light from Massive Protoclusters (POLIMAP): Zooming into dense clumps in infrared dark clouds
2025B-S016 Jakob den Brok6 Expanding the SMA Molecular Line Survey of Starburst Galaxy Centers
2025B-S018 Ioannis Myserlis7 SMAPOL: SMA Monitoring of AGNs with POLarization
2025B-S020 Zoe Parker8 Finding and characterising extreme debris disks: a pilot study
2025B-S022 Michael McCollough5 SMA Observations during a Multi-Wavelength VLBA Campaign of Cygnus X-3
2025B-S023 Maria S. Kirsanova1 Mapping the Beginning of the Water Ice Evaporation Phase in a Massive Protostar with the SMA
2025B-S024 Shu Liu1 O18O emission in SNR IC443 B region with the SMA (copied from 2023A-S001)
2025B-S028 Aaron Hughes2 CII Observations of Extremely Luminous and High-Redshift DSFGs
2025B-S031 Carl Ingebretsen2 Detecting Millimeter Emission from Planet-hosting Debris Disks.

Current or completed Large Scale Programs spanning ALL semesters:
Project IDP.I.TracksTitle (hover for abstract)
2012B-S097 Qizhou Zhang3 Star Formation in the Central Molecular Zone
2013A-S079 Michael Dunham3 (p)MASSES: (pilot) Mass Assembly of Stellar Systems and their Evolution with the SMA
2013B-S091 Eric Keto61 CMZ
2014A-S093 Michael Dunham55 MASSES: Mass Assembly of Stellar Systems and their Evolution with the SMA
2017A-S060 Garrett "Karto" Keating50 The Millimeter-wave Intensity Mapping Experiment (mmIME)
2017B-S075 Jan Forbrich100 SMA Survey of Resolved Dust and Simultaneous CO Observations of GMCs in M31
2019A-A022 Shih-Ping Lai2 Mosaic Polarization Observations towards Star-forming Cores
2022B-S046 Edo Berger44 POETS: Pursuit of Extragalactic Transients with the SMA
2022B-S047 Karin Oberg72 SMA-SPEC: the SMA Survey of Protoplanetary disks to Explore their Chemistry
2023A-A012 Seamus Clarke33 B-fields, gravity and turbulence across multiple scales - How does the relative importance of gravity, turbulence and magnetic fields impact high-mass star and cluster formation?
2024A-A008 Bovornpratch Vijarnwannaluk6 A SMA Investigation of the Evolution of ISM Density in AGN Host Galaxies
2024B-S057 Eric Koch32 1e4 Msol at 5-sigma per beam. Our GMC catalog will include clouds likely hosting massive star formation and matching the mass of the nearby Perseus molecular cloud. This is an order of magnitude higher physical resolution and mass sensitivity than the landmark PHANGS-ALMA program. Our survey will cover the inner 25 kpc of the disk, which existing single dish mapping shows is CO-bright. It will resolve H2 in >1000 molecular clouds at all evolutionary stages, producing the definitive M31 CO map and cloud catalog. When combined with 4" 21-cm HI and 2" radio continuum VLA maps from the Local Group L-band Survey, this dataset will enable a broad range of ISM and star formation science. This proposal outlines 2 key science areas enabled by connecting the HI, 12CO(2-1) and 13CO(2-1) on resolved scales with existing HST-identified clusters with measured masses and ages: (i) we will leverage matched HI and H2 tracers to test H2 formation models; and (ii) we will test how clouds are kinematically connected to their surrounding HI envelopes and benchmark the timescales on which clusters destroy and drift from their natal clouds. Though we focus on specific science cases, this legacy data has broad applications to ISM and star formation studies. For technical development aspects, we will provide the tools to enable OTF mapping from proposal preparation through imaging, including an online mosaicking time and planning calculator, OTF observing script generator and online tools, enhanced COMPASS capability for OTF data reduction, SMA archive support for OTF-mode observations, and GPU-enabled imaging for large OTF (and pointed) mosaics. ">A complete CO(2-1) Map of M31 with SMA OTF mapping