CANDELS Meeting
Location: Ballroom at the Student Union
Peter Capak (IPAC/Caltech), Avishai Dekel (Hebrew University), David Elbaz (CEA Saclay), Sandra Faber (UCSC), Harry Ferguson (STScI), Steve Finkelstein (UT Austin), Susan Kassin (STScI), Laura Pentericci (INAF), Alvio Renzini (INAF), Linda Tacconi (MPE)Day 0: Sunday October 21
- 17:30 - 19:30: Check-In/Registration, Old Chapel
- 18:00 - 21:00: Reception, Old Chapel
Day 1: Monday October 22
- 8:00 - 9:30: Check-In/Registration, Student Union Ballroom
- 8:00 - 13:30: Morning Session - CANDELS and Its Evolution; The High Redshift Universe
Chair: Alex Pope
- 8:00 - 8:55 Breakfast (provided)
- 9:00 - 9:05 Welcome: Daniela Calzetti (Chair, UMass Astronomy Department)
- 9:05 - 9:15 Opening Remarks: Bob Williams
- 9:20 - 9:45 The State of CANDELS: Harry Ferguson
- 9:50 - 10:15 The power law model of galaxy evolution: Sandra Faber
- 10:20 - 10:35 The JWST GTO survey of CANDELS: Christina Williams
- 10:40 - 10:55 The Astrodeep project: status and highlights: Adriano Fontana
- 11:00 - 11:15 Coffee Break
- 11:15 - 11:40 Unveiling the high redshift universe: a view from deep optical spectroscopy: Laura Pentericci
- 11:45 - 12:00 Large VLT Spectroscopic Surveys in the CANDELS fields: Nimish Hathi
- 12:05 - 12:20 Are the most massive galaxies in the universe missed by HST?: Tao Wang
- 12:30 - 13:30 Lunch Break (lunch provided)
- 13:30 - 16:40: Afternoon Session - The High Redshift Universe (continued)
Chair: Kate Whitaker
- 13:30 - 13:55 Continuing to push into the Early Universe with CANDELS: Steve Finkelstein
- 14:00 - 14:15 CIGALE SED fitting and the properties of galaxies at redshift 5<z<8: Denis Burgarella
- 14:20 - 14:35 RELICS and a Candidate Spatially Resolved Arc at z~10: Brett Salmon
- 14:40 - 14:55 A very large (20 kpc) galaxy at z=3.72 near a proto-cluster: Kyoung-Soo Lee
- 15:00 - 15:15 Coffee Break
- 15:15 - 16:05 Flash Presentations (9x5; total 45+5 buffer, total 50 min): Isabella Cox, Maximilien Franco, Kertheik Iyer,Sarah Betti, Intae Jung, Meaghann Stoelting, Jed McKinney, Krystal Tyler, Brittany Vanderhoo
- 16:10 - 16:40 End-of-Session Discussion
- 20:00: Public Lecture: Bob Williams
- For more information: Talk: Robert Williams "Probing the Distant Universe with Hubble Space Telescope"
- 8:00 - 13:30: Morning Session: The Assembly of Galaxy Structures
Chair: Adriano Fontana
- 8:00 - 8:55 Breakfast (provided)
- 9:00 - 9:25 Toward a Standard Model of galaxies: Peter Capak
- 9:30 - 9:55 Compaction Driven Black-Hole Growth: Avishai Dekel
- 10:00 - 10:15 High-redshift elongated galaxies in CANDELS as probes of the cosmic web at z~2: Viraj Pandya
- 10:20 - 10:35 Tracking down the evolutionary links between galaxy populations using cosmic calorimetry: Stephen Eales
- 10:40 - 10:55 The Origin and Evolution of the Galaxy Star Formation Rate-Stellar Mass Correlation: Eric Gawiser
- 11:00 - 11:20 Coffee Break
- 11:20 - 11:35 4A2C2S: The ALMA ALPINE CII Survey. Star formation and galaxy assembly at 4<z<6: Paolo Cassata
- 11:40 - 11:55 Demographics of dust attenuation curves in the local universe and in CANDELS: Samir Salim
- 12:00 - 12:15 Which dust attenuation law(s) for dusty star forming galaxies?: Veronique Buat
- 12:20 - 13:30 Lunch Break (lunch provided)
- 13:30 - 18:30: Afternoon Session - The Assembly of Galaxy Structures (continued)
Chair: Itziar Aretxaga
- 13:30 - 13:55 The Early Evolution of Galactic Disks: Gas and Star Formation: Linda Tacconi
- 14:00 - 14:25 An ALMA view on massive galaxy and galaxy cluster formation: David Elbaz
- 14:30 - 14:45 ALMA deep surveys on CANDELS fields: Kotaro Kohno
- 14:50 - 15:05 JWST/NIRSpec Survey in CANDELS: Physical Conditions in Early Galaxies: Susan Kassin
- 15:10 - 15:25 Coffee Break
- 15:25 - 15:40 Gas-rich star forming disks at low z: analogs for high-z disks: Ben Weiner
- 15:45 - 16:00 Structural Properties and NIR Morphologies of Faint SMGs: Yu-Yen Chang
- 16:05 - 16:20 Investigating galaxy evolution with deep learning in CANDELS: Marc Huertas-Company
- 16:25 - 16:40 Galaxy mergers up to z~2.5: the SF properties of galaxies at separation 3-15 kpc: Danilo Marchesini
- 16:45 - 17:00 CANDELS sheds light on the environmental quenching of low-mass galaxies: Yicheng Guo
- 17:05 - 17:20 Latest results from the MOSDEF survey: Bahram Mobasher
- 17:25 - 17:55 Flash presentations (5x5 = 25+5 buffer, total 30 min): Emmaly Aguilar, Mohammad Akhshik, Alexander de la Vega, Abtin Shahidi, Luwenjia Zhou
- 18:00 - 18:30 End-of-Session Discussion
- 8:00 - 14:00: Morning Session: The Assembly of Galaxy Structures
Chair: Mauro Giavalisco
- 8:00 - 8:55 Breakfast (provided)
- 9:00 - 9:25 Galaxy Formation from CGM prospective: Houjun Mo
- 9:30 - 9:45 Galaxy-Black Hole Co-Evolution in Simba: Romeel Dave
- 9:50 - 10:05 Formation of ultra-diffuse galaxies in the field and in galaxy groups: Fangzhou Jiang
- 10:10 - 10:25 On the formation of UDG galaxies: Timothy Carlton
- 10:30 - 11:00 Coffee Break
- 11:00 - 11:25 On the formation of disk and spheroidal quenched galaxies: Sandro Tacchella
- 11:30 - 11:45 Star Formation, Dust, and Galaxy Structure: What does it mean to be average?: Kate Whitaker
- 11:50 - 12:05 The Galaxy-Halo Connection since z=0 to z=10: Aldo Rodriguez-Puebla
- 12:10 - 12:25 Spatially Resolving ISM and AGN with CANDELS/3D-HST/CLEAR/CEERS: Jonathan Trump
- 12:30 - 14:00 Lunch Break (lunch provided)
- 14:00 - 22:30: Afternoon Session - The HALO-Galaxy Connection and the Structural Evolution of Galaxies (continued)
Chair: Mauro Giavalisco
- 14:00 - 14:15 Close Pair Observability Timescales using Semi-Analytic and Semi-Empirical Mock Observations: Kameswara Bharadwaj
- 14:20 - 14:35 Clump Survival and Migration in VDI Galaxies: a Toy Model versus Simulations and Observations: Nir Mandelker
- 14:40 - 14:55 Visual Morphology Classifications and the Properties of Luminous IR Galaxies in CANDELS: Jeyhan Kartaltepe
- 15:00 - 15:15 The structural stellar mass growth of Milky Way-sized galaxies: Vladimir Avila-Reese
- 15:20 - 15:50 Coffee Break
- 15:50 - 16:05 CANDELS: Radial Structure and Evolution of Galaxies over 0.5<z<2.5: Fengshan Liu
- 16:10 - 16:55 Flash Presentations (8x5 = 40+5 buffer total 45 min): Vicente Estrada-Carpenter,Nima Chartab-Soltani, Marziye Jafariyazani, Zhiyuan Ji, Ekta Shah,Tonima Tasnim-Ananna, Weichen Wang, Guang Yang
- 17:00 - 17:30 Final Discussion, Future plans, TolTEC Intro
- 18:00 - 22:30 Conference Dinner, Old Chapel; Meeting Adjourns
Day 2: Tuesday October 23
Day 3: Wednesday October 24
TolTEC Workshop
Location: UMass Amherst, Amherst room, 10th floor of student center
Kristen Coppin (Univ. of Hertfordshire), James Dunlop (IfA Edinburgh), Chris Hayward (Flatiron Institute), Wei-Hao Wang (Academia Sinica), Jack Sayers (Caltech), Nick Scoville (Caltech) For each survey (UDS and LSS), the workshop participants make recommendations to the TolTEC science team for 4 major decisions:- 1. Contiguous or multiple fields
- 2. Biased or blind fields
- 3. Area and depth of survey
- 4. Prioritized list of fields for the survey (include more than can be allocated to account for schedulability and other issue)
Day 1: Thursday October 25
- 8:00 - 9:30: Check-In/Registration, Amherst Room
- 8:00 - 9:00: Breakfast (provided)
- 9:00 - 9:05: Introduction: Alex Pope
- 9:05 - 9:10: Welcome: John McCarthy (UMass Provost)
- 9:10 - 10:25: Science Session
- - Review talk on dusty side of galaxy evolution: Jim Dunlop (25 min)
- - Review talk on dust continuum surveys: Kristen Coppin (25 min)
- - Talk on theory/modeling of submm galaxies: Chris Hayward (25 min)
- 10:25 - 10:30: Welcome: Tricia Serio (CNS Dean)
- 10:30 - 10:45: Coffee
- 10:45 - 12:15: Intro to TolTEC and the Legacy Survey
- - LMT status and projection for next 3 years: David Hughes (15 min)
- - Instrument progress: Grant Wilson (15 min)
- - LSS science goals: Alex Pope (15 min)
- - UDS science goals: Itziar Aretxaga (15 min)
- - Goals for the meeting, procedure for making decisions to define the surveys (see Workshop Goals above; 15 min)
- - Open discussion and Q&A (15 min)
- 12:15 - 13:15: Lunch (provided)
- 13:15 - 14:45: Discussion - Contiguous vs multiple fields, area-depth parameter space, biased vs unbiased, including any relevant predictions or simulations
- Coordinator: Itziar Aretxaga (Casey, Zavala, Kotaro, Negrello, Franco, Dave, Rodríguez) notes: Tazkera Haque
- 14:45 - 15:00: Coffee
- 15:00 - 16:30 Discussion - Fields: existing/upcoming ancillary data and advanced data products in potential ToLTEC fields
- Coordinator: Steve Eales (Buat/Burgarella, Williams, Baker, Kartaltepe, Cruz-Gonzalez, Alberts, Yoon, Sajina, Greve, Jin, Ferguson, Marchesini) notes: Patrick Kamieneski
- 16:30 - 17:00 Summary of fields suggested
- UD Coordinator: Min Yun & Itziar Aretxaga
- LSS Coordinator: Alex Pope & David Hughes
Day 2: Friday October 26
- 8:00 - 9:00 Breakfast (provided)
- 9:00 - 10:15: Science Session
- - Talk on dust continuum as an ISM tracers: Nick Scoville (25 min)
- - Talk on interferometry single-dish synergy: Wei-Hao Wang (25 min)
- - Extragalactic SZ surveys: Jack Sayers (25 min)
- 10:15 - 10:30: Coffee
- 10:30 - 12:00: Discussion - SZ predictions and considerations for ToLTEC
- Coordinator: Sara Simon (DeNigris, Sanchez, Brodwin, Scannapieco, Mo, Lim, Romero) notes: Sarah Betti
- 12:00 - 13:00: Lunch (provided)
- 13:00 - 13:30: Make clear charge to workshop: 4 decisions to make
- 13:30 - 15:00: Breakout session for LSS and UDS to discuss top field choices and come up with recommendations for each of 4 decisions
- 15:00 - 15:30: Coffee
- 15:30 - 17:00: Breakout summaries and discussion
- Coordinator: Min Yun (Skidmore, Bradford, Staguhn) notes: Nat DeNigris
- - Discuss any overlap in field choices between UDS and LSS
- - Discussion of simulations/calculations needed to fully exploit the TolTEC datasets
- - New observations needed or coordinating with upcoming facilities/surveys