Emission Line Galaxies with MOS: from cosmic noon to the reionization era
| When |
Sep 18, 2017 12:00 PM
to
Sep 22, 2017 02:30 PM |
|---|---|
| Where | Kavli Institute for Cosmology, University of Cambridge |
| Contact Name | LOC |
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Emission Line Galaxies with MOS: from cosmic noon to the reionization era
18 - 22 September 2017, Kavli Institute for Cosmology, Cambridge, UK
Registration and Abstract Submission are now closed
Galaxies showing strong emission lines are precious laboratories to study the physical mechanisms driving and regulating star formation through cosmic time, since they can be easily observed from the local universe to the highest redshifts.
With the advent of the last generation of optical and near-infrared Multi Object and Integral Field Spectrographs (MOS, IFS), we have entered in a new golden era for emission line studies. Therefore, it is now possible to draw a detailed picture of the several inter-linked physical processes driving star formation and chemical evolution in galaxies from low to high redshifts as never before. In particular, large and deep MOS surveys appear as powerful tools to trace physical properties of galaxies in space and time with high statistical significance. Exciting enough, the next generation of ground-based and space-borne multifrequency MOS facilities (e.g. VLT-MOONS, JWST-NIRSpec, Subaru-PFS, WEAVE, 4MOST, DESI, E-ELT-MOSAIC) will arrive with the promise of revolutionising the field, providing high multiplexing data of unprecedented sensitivity over large cosmic volumes. This will allow us to trace the physical properties of galaxies in space and time by pushing studies into the rather unexplored low-mass regime, from intermediate redshifts (z~1-2) to the reionization era at z>6, with profound implications in our understanding of galaxy formation and evolution.
This Workshop will be a chance to review and discuss crucial aspects of galaxy formation and evolution at intermediate and high redshifts. We aim at bringing together leading experts in the scientific exploitation of current and future MOS facilities, and more broadly scientists active in the investigation of emission line galaxies, emission line and photoionization modelling, and cosmological/hydrodynamic simulations. Early-career researchers are especially encouraged to participate.
The following key topics will be covered:
- Star Formation throughout Cosmic Time.
- Excitation mechanisms and emission line diagnostics.
- Metallicity, chemical abundances and gradients.
- Galaxy kinematics and dynamics.
- Primordial Universe and reionization.
- Prospects for high redshift studies with upcoming facilities.
Invited Speakers
- Jarle Brinchmann (Sterrewacht Leiden)
- Andrew Bunker (University of Oxford)
- Marco Castellano (Osservatorio Astronomico di Roma)
- Michele Cirasuolo (European Southern Observatory)
- Romeel Davé (University of Western Cape)
- Anna Feltre (Institut d'Astrophysique de Paris)
- Andrea Ferrara (Scuola Normale Superiore di Pisa)
- Lisa Kewley (Australian National University)
- Filippo Mannucci (Osservatorio di Arcetri)
- Ivelina Momcheva (Yale University)
- Thorsten Naab (Max-Planck-Institut für Astrophysik)
- Laura Pentericci (Osservatorio Astronomico di Roma)
- Enrique Pérez Montero (Instituto de Astrofísica de Andalucía)
- Celine Peroux (Laboratoire dʼAstrophysique de Marseille)
- Naveen Reddy (University of California, Riverside)
- Brant Robertson (University of California, Santa Cruz)
- Daniel Schaerer (Observatoire de Genève)
- Alice Shapley (University of California, Los Angeles)
- Daniel Stark (University of Arizona)
- Charles C. Steidel (California Institute of Technology)
- Lidia Tasca (Laboratoire d'Astrophysique de Marseille)
- Arjen van der Wel (Max-Planck-Institut für Astronomie)
- Emily Wisnioski (Max-Planck-Instituts für extraterrestrische Physik)
Sponsors
We gratefully acknowledge funding from the Kavli Foundation and from a grant from the Templeton Foundation held by Prof. Martin Rees.
Organizing Committee
Scientific Organizing Committee
- Ricardo Amorin (co-chair)
- Ricardo Chavez (co-chair)
- Avishai Dekel
- Olivier Le Fevre
- Roberto Maiolino
- Laura Pentericci
- Max Pettini
- Alice Shapley
- Debora Sijacki
- Renske Smit
- Lutz Wisotzki
- Ricardo Amorin
- Sandra Berner
- Ricardo Chavez
- Roberto Maiolino
- Renske Smit
-
Almarie Williams
Scientific Programme
KICC Workshop 2017 – Scientific Programme
Monday, 18 September
12:00 – 13:15 REGISTRATION AND LUNCH
13:15 – 13:30 WELCOME
First Session: Star formation through cosmic time with MOS
Chair: Renske Smit
13:30 – 14:00 Romeel Davé: “Models for the cosmic evolution of star formation in galaxies“ (Invited)
14:00 – 14:30 Ivelina Momcheva: “Wide-field Slitless Spectroscopy from Space: Unique Constraints on Galaxy Evolution from Cosmic Dusk to Dawn” (Invited)
14:30 – 14:50 David Gilbank: “The lowest-mass star-forming galaxies at cosmic high noon”
14:50 – 15:10 Annagrazia Puglisi: “FMOS unveils the optical properties of z~1.6 Herschel dusty starbursts”
15:10 – 15:30 Margherita Talia: “The SFR Cookbook: recipes for spectroscopic estimators at 1<z<3”
15:30 – 16:00 COFFEE BREAK
16:00 – 16:30 Naveen Reddy: “Key Results on the Dust Attenuation, Equivalent Width Distributions, and Ionizing Escape Fractions of High-Redshift Galaxies” (Invited)
16:30 – 16:50 Anita Zanella: “Spatially resolved emission line maps: a crucial ingredient to study giant star-forming clumps at high redshift”
16:50 – 17:20 Laura Pentericci: “VANDELS- a deep spectroscopic survey of the CANDELS fields” (Invited)
17:20 – 17:50 Lidia Tasca: ”Evolutionary pathways of star forming galaxies since z~5” (Invited)
18:00 – 19:00 WELCOME RECEPTION
Tuesday, 19 September
Second Session I: Emission line diagnostics, chemical abundances, and metallicity gradients
Chair: Allison Strom
09:30 – 10:00 Anna Feltre: “Spectral features of different ionizing sources within galaxies” (Invited)
10:00 – 10:20 Alba Vidal-García: “Modeling the ultraviolet emission from young galaxies at high redshift”
10:20 – 10:40 Michaela Hirschmann: “Cosmic evolution of synthetic nebular emission lines of galaxies out to the epoch of re-ionisation”
10:40 – 11:00 Ben Forrest: “A Population of Extreme [OIII]+Hβ Emission Line Galaxies Tracing an Overdensity at z~3.5 in CDF-South”
11:00 – 11:30 COFFEE BREAK
11:30 – 12:00 Daniel Schaerer: “Emission lines in high-z star-forming galaxies” (Invited)
12:00 – 12:20 Olivier Le Fèvre: “CIII emitters with 2< z <3.8 in the VUDS survey: statistics and populations”
12:20 – 12:40 Thomas Fletcher: “The nature of the ionising spectrum in a large sample of faint z∼3 Lyman alpha emitters”
12:40 – 13:00 Michael Maseda: “CIII] Emitters in the MUSE UDF Survey”
13:00 – 14:00 LUNCH
Chair: Ricardo Amorin
14:00 – 14:30 Alice Shapley: “Untangling the new landscape of z~2 emission-line measurements?” (Invited)
14:30 – 14:50 Daniel Masters: “The importance of abundance ratio variations in interpreting high redshift emission line spectra”
14:50 – 15:10 Kim-Vy Tran: “The MOSEL Survey : Emission Line Galaxies at 3 <z <4”
15:10 – 15:30 Stephen Wilkins: “Insights for the Epoch of Reionisation from low-redshift Extreme Emission Line Sources”
15:30 – 16:00 COFFEE BREAK
16:00 – 16:30 Filippo Mannucci: “The cosmic evolution of metallicity and abundance gradients”(Invited)
16:30 – 17:00 Andrea Ferrara: “The Interstellar Medium of High Redshift Galaxies” (Invited)
17:00 – 17:30 OPEN DISCUSSION I (Lead: Rob Kennicutt)
Wednesday, 20 September
Second Session II: Emission line diagnostics, chemical abundances, and metallicity gradients
Chair: Marco Castellano
09:30 – 10:00 Enrique Pérez-Montero: “Secondary chemical abundances in starburst galaxies in different cosmological epochs” (Invited)
10:00 – 10:20 Nimisha Kumari: “Probing Emission Line Galaxies with MUSE”
10:20 – 10:40 Jorge Sanchez Almeida: “Evidence for gas accretion sustaining star-formation in disk galaxies”
10:40 – 11:00 José M. Vílchez: “Metallicity of Emission Line Galaxies Located in Extreme Density Environments”
11:00 – 11:30 COFFEE BREAK
11:30 – 12:00 Allison Strom: “New insights into measuring gas chemistry and ionization in high-z star-forming galaxies with the Keck Baryonic Structure Survey” (Invited)
12:00 – 12:20 Tucker Jones : “Accurate chemical abundance diagnostics for high redshift galaxies”
12:20 – 12:40 Ryan Sanders: “Increasing the accuracy of metallicity measurements over the past 12 Gyr of cosmic history”
12:40 – 13:00 Antonello Calabrò: “Star-forming dwarf galaxies at z <1 in the VUDS survey: new insights on the low-mass end of the mass-metallicity relation”
13:00 – 14:00 LUNCH
Chair: Ricardo Chávez
14:00 – 14:30 Celine Peroux: “Connecting gas and stars: insights from abundances and kinematics” (Invited)
14:30 – 14:50 Mirko Curti: “The KLEVER Survey : Spatially resolved gas excitation properties and metallicity gradients in high redshift galaxies”
Third Session I: Dynamical studies of galaxies
14:50 – 15:10 Alfred Tiley: “Gas Kinematics and Galaxy Dynamics for ∼1000 z=0.6-2 Galaxies from KMOS”
15:10 – 15:30 Vera Patricio: “Sub-kiloparsec MUSE view of z∼1 strongly lensed galaxies”
15:30 – 16:00 COFFEE BREAK
16:00 – 16:30 Arjen van der Wel: “The LEGA-C Survey: Gas and Stellar Kinematics at z~1” (Invited)
16:30 – 16:50 Caroline Straatman: “The kinematics of intermediate redshift galaxies with LEGA-C”
16:50 – 17:10 Roberto Terlevich: “Cosmology with HII galaxies and the universality of the IMF”
19:00 – 22:00 DINNER (Peterhouse)
Thursday, 21 September
Third Session II: Dynamical studies of galaxies
Chair: Anna Feltre
09:50 – 10:20 Hannah Übler : “Kinematics of star-forming galaxies at z~1-2 with KMOS3D”
10:20 – 10:40 Susan Kassin: “The Assembly of Disk Galaxies: From Keck to JWST”
10:40 – 11:00 Owen Turner: “The KMOS Deep Survey (KDS): dynamical measurements of typical star-forming galaxies at z ∼ 3.5”
11:00 – 11:30 COFFEE BREAK
Fourth Session: Early galaxies and reionization
11:30 – 12:00 Jarle Brinchmann: “Spectroscopy from space - the synergy of Euclid with other spectroscopic facilities” (Invited)
12:00 – 12:20 Brian Siana: “Rest-Optical Spectroscopy of Lensed Dwarf Galaxies at 1<z<3: Analogs of Reionization Galaxies”
12:20 – 12:40 Kimihiko Nakajima: “Ly-alpha Emitters with Intense [OIII] Emission: Analogs of Galaxies in the Reionization Era?”
12:40 – 13:00 Jean Michel Gomes: “FADO: Fitting Analysis using Differential evolution Optimization - A novel spectral population synthesis tool for the exploration of galaxy evolution”
13:00 – 14:00 LUNCH
Chair: Stephen Wilkins
14:00 – 14:30 Daniel Stark: “Spectroscopic Properties of Galaxies in the Reionization Era” (Invited)
14:30 – 14:50 Francesca Marchi: “Investigating the connection between LyC and Lyα emission and other indirect indicators”
14:50 – 15:10 David Sobral: “The brightest Lyman-alpha emitters at z∼7 as seen by ALMA, HST and the VLT”
15:10 – 15:30 Jorryt Matthee: “Calibrating Lyman-alpha with Halpha at the peak of cosmic star formation history”
15:30 – 16:00 COFFEE BREAK
16:00 – 16:30 Marco Castellano: “The contribution of faint galaxies to cosmic reionization” (Invited)
16:30 – 16:50 Rebecca Bowler: “Unveiling the nature of the brightest z > 6 galaxies with MOS”
16:50 – 17:20 OPEN DISCUSSION II (Lead: Smit and Wilkins)
Friday, 22 September
Fifth Session: The future
Chair: Arjen van der Wel
09:40 – 10:10 Brant Robertson: “Looking Forward to Looking Backward: Extragalactic Spectroscopy with WFIRST” (Invited)
10:10 – 10:40 Andy Bunker: “Prospects for high redshift studies with JWST and other upcoming facilities” (Invited)
10:40 – 11:00 Chris Willott: “Highly multiplexed information on emission line galaxies via JWST slitless spectroscopy ”
11:00 – 11:30 COFFEE BREAK
11:30 – 11:50 Emma Curtis-Lake: “Constraining the stochasticity of star formation at high redshifts with JWST"
11:50 – 12:10 Francois Hammer: “MOSAIC at the ELT:A Gigantic Step into the Deep Universe”
12:10 – 12:40 Roberto Maiolino: SUMMARY
12:40 – 14:00 LUNCH
Registration and Abstract Submission
The abstract submission and registration are now closed. Accepted speakers will be contacted soon. We expect to publish the workshop programme by the end of May.
Invited Speakers
- Jarle Brinchmann (Sterrewacht Leiden)
- Andrew Bunker (University of Oxford)
- Marco Castellano (Osservatorio Astronomico di Roma)
- Michele Cirasuolo (European Southern Observatory)
- Romeel Davé (University of Western Cape)
- Anna Feltre (Institut d'Astrophysique de Paris)
- Andrea Ferrara (Scuola Normale Superiore di Pisa)
- Lisa Kewley (Australian National University)
- Filippo Mannucci (Osservatorio di Arcetri)
- Ivelina Momcheva (Yale University)
- Thorsten Naab (Max-Planck-Institut für Astrophysik)
- Laura Pentericci (Osservatorio Astronomico di Roma)
- Enrique Pérez Montero (Instituto de Astrofísica de Andalucía)
- Celine Peroux (Laboratoire dʼAstrophysique de Marseille)
- Naveen Reddy (University of California, Riverside)
- Brant Robertson (University of California, Santa Cruz)
- Daniel Schaerer (Observatoire de Genève)
- Alice Shapley (University of California, Los Angeles)
- Daniel Stark (University of Arizona)
- Allison Strom (Caltech/Carnegie Observatories)
- Lidia Tasca (Laboratoire d'Astrophysique de Marseille)
- Hannah Übler (Max-Planck-Institut für extraterrestrische Physik)
- Arjen van der Wel (Max-Planck-Institut für Astronomie)
Participants
Invited Speakers
- Jarle Brinchmann (Sterrewacht Leiden)
- Andrew Bunker (University of Oxford)
- Marco Castellano (Osservatorio Astronomico di Roma)
- Michele Cirasuolo (European Southern Observatory)
- Romeel Davé (University of Western Cape)
- Anna Feltre (Institut d'Astrophysique de Paris)
- Andrea Ferrara (Scuola Normale Superiore di Pisa)
- Lisa Kewley (Australian National University)
- Filippo Mannucci (Osservatorio di Arcetri)
- Ivelina Momcheva (Yale University)
- Thorsten Naab (Max-Planck-Institut für Astrophysik)
- Laura Pentericci (Osservatorio Astronomico di Roma)
- Enrique Pérez Montero (Instituto de Astrofísica de Andalucía)
- Celine Peroux (Laboratoire dʼAstrophysique de Marseille)
- Naveen Reddy (University of California, Riverside)
- Brant Robertson (University of California, Santa Cruz)
- Daniel Schaerer (Observatoire de Genève)
- Alice Shapley (University of California, Los Angeles)
- Daniel Stark (University of Arizona)
- Allison Strom (Caltech/Carnegie Observatories)
- Lidia Tasca (Laboratoire d'Astrophysique de Marseille)
- Hannah Übler (Max-Planck-Institut für extraterrestrische Physik)
- Arjen van der Wel (Max-Planck-Institut für Astronomie)
Contributed Talks
- Rebecca Bowler (University of Oxford)
- Antonello Calabrò (INAF, Osservatorio Astronomico di Roma)
- Mirko Curti (University of Florence)
- Emma Curtis-Lake (Institut d'Astrophysique de Paris)
- Mark Dijkstra (University of Oslo)
- Alyssa Drake (Observatoire de Lyon)
- Thomas Fletcher (University College London)
- Ben Forrest (Texas A&M University)
- David Gilbank (South African Astronomical Observatory)
- Jean Michel Gomes (Instituto de Astrofísica e Ciências do Espaço)
- Francois Hammer (Paris Observatory)
- Michaela Hirschmann (Institute d'Astrophysique de Paris)
- Tucker Jones (UC Davis)
- Susan Kassin (Space Telescope Science Institute)
- Rob Kennicutt (IoA, University of Cambridge)
- Nimisha Kumari (Institute of Astronomy)
- Olivier Le Fèvre (Aix-Marseille Université)
- Roberto Maiolino (Cavendish Lab., University of Cambridge)
- Francesca Marchi (Osservatorio Astronomico di Roma)
- Michael Maseda (Leiden Observatory)
- Daniel Masters (California Institute of Technology)
- Jorryt Matthee (Leiden Observatory)
- Kimihiko Nakajima (European Southern Observatory)
- Vera Patricio (CRAL)
- Annagrazia Puglisi (Università degli Studi di Padova)
- Jorge Sanchez Almeida (Instituto de Astrofisica de Canarias)
- Ryan Sanders (University of California, Los Angeles)
- Brian Siana (UC Riverside)
- David Sobral (Lancaster University)
- Caroline Straatman (Max Plank Institute for Astronomy)
- Margherita Talia (University of Bologna)
- Elena Terlevich (INAOE)
- Roberto Terlevich (INAOE and IoA)
- Alfred Tiley (CEA, Durham University)
- Kim-Vy Tran (Texas A&M University)
- Owen Turner (Royal Observatory Edinburgh)
- Alba Vidal-García (IAP/CNRS-UPMC)
- José M. Vílchez (IAA-CSIC)
- Stephen Wilkins (University of Sussex)
- Chris Willott (NRC Herzberg)
- Anita Zanella (ESO Garching)
Accommodation
Accommodation can be reserved at Murray Edwards College, which is located a short walk from the KICC. The promotional code you can use is KAVLI2017 (case sensitive). The rate is £88.20 per ensuite room per night inclusive of full English breakfast.
Accommodation can also be reserved at Churchill College, similarly at a very short walk from the KICC.
Travel
Contact
Kavli Institute for Cosmology Cambridge
c/o Institute of Astronomy
Madingley Road
Cambridge
CB3 0HA
United Kingdom
Maps
Map of the KICC and IoA within Cambridge
Institute of Astronomy on the scrollable University of Cambridge map
When visiting KICC please enter via the IoA entrance on Madingley Rise where our main reception area is located.
Arriving by Road
The Institute of Astronomy main entrance is situated on Madingley Rise which joins Madingley Road opposite JJ Thompson Avenue. The map of the KICC site shows available parking.
The main car park is the first entrance on the right after leaving Madingley Road and has about 30 parking spaces.
Additional parking is available (out of office hours) further up Madingley Rise. If you follow the main rise up and round where it turns to the right there is a larger gravel car park to the right (with about 50 spaces) and more parking in front of Greenwich House right at the end of Madingley Rise.
Alternatively parking is available at the Park and Ride, which is less than 10 mins walk away from IoA, along Madingley Road, and also nearby street parking is available along Clerk Maxwell Road.
A disabled parking space is available immediately outside the main entrance.
Arriving by Public Transport
A citi 4 (or uni 4) bus is the best route from the city centre to the Institute of Astronomy, though the service is infrequent, especially on the return journey later on in the evening. Ideally leave the bus at the stop at the entrance to JJ Thomson Avenue and cross the road to Madingley Rise.
Timetable information for this route
Arriving by Rail
General information about UK train services is available at the National Rail Enquiries website. In general, trains are quicker but more expensive than coaches.
Stagecoach Cambus runs services between Cambridge rail station and the city centre, or take a taxi from the queue just outside the station.
There are regular train connections to Cambridge from London. Trains depart from King's Cross or Liverpool Street stations in London. The journey time of the faster King's Cross trains (Cambridge Cruiser trains) is about 45 minutes, while the other trains are slower and take around 70 minutes, or longer.
Maps of the London underground are available on the TFL website.
Eurostar
London can be reached from Paris or Brussels by the Eurostar train which uses the channel tunnel. You will arrive at London St Pancras International station. King's Cross station is next to St Pancras, so walk to King's Cross and catch a train from there to Cambridge (timetables).
Arriving by Coach
There are frequent coach connections from the centre of London to Cambridge. These depart from Victoria coach station (near Victoria railway station) and take about 2 hours (more in peak hours). Coach tickets can be bought from the driver. Please note that delays are common because of heavy traffic in and around London.
The Cambridge coach station is close to the city centre and there is an adjacent taxi rank.
Long-distance coach services are run by JetLink and NationalExpress. A combined timetable can be found at the National Express website. Stagecoach Cambus runs services in Cambridge and to/from nearby villages and towns.
The University has compiled further information on local bus travel.
Arriving by Air
London Stansted
This is the closest major airport, about 25 miles (40 minutes by car) from Cambridge. It is well served by airlines flying to European destinations. For flight information contact the BAA Stansted website or contact the airlines directly.
Cambridge is within easy reach by rail, coach or taxi. The railway station is part of the terminal. The services to Cambridge run frequently and take about 30 minutes. The service operates seven days a week, the first train departing at 05:51 (Monday to Sunday). The last direct train to Cambridge departs at 21:18 Monday to Saturday and 22:40 on Sundays.
There is also a good coach service (JetLink lines 757 or 797) which departs at 40 past the hour every 2 hours. The journey takes about 50 minutes. Tickets can be purchased from the coach ticket desk in the arrivals area of the terminal, on the coach or from the National Express web site
London Heathrow
Many airlines fly to London Heathrow. There is a direct coach service to Cambridge (JetLink 797) which operates every 2 hours at 20 minutes to the hour and the journey takes 2 hours 20 minutes. National Express web site. Another coach (JetLink 787) departs at 20 past every 2 hours but the journey takes 20 minutes longer than the 797 service.
A fast train service, the Heathrow Express, connects the airport with London Paddington station. From there use the Underground to connect with rail or coach services listed above to reach Cambridge. The Circle and Hammersmith and City Lines operate between Paddington and Kings Cross.
Underground Trains
We suggest you take the Piccadilly line from Heathrow Airport to Kings Cross. Change to the main line Kings Cross station, from which fast trains depart to Cambridge railway station.
Taxi
Black cabs outside the airport can be three times the price of a pre-booked taxi.
London Gatwick
This airport is located to the south of London.
The Thameslink service (operated by First Capital Connect) from Gatwick Airport to St Pancras is the most efficient way to reach the King's Cross mainline station (which is situated adjacent to St Pancras) and take the fast trains to Cambridge. The Gatwick Airport railway station is accessible from the South Terminal.
Coach
We do not recommend travelling from Gatwick to Cambridge by coach. The journey takes about 4 hours.
Taxi
Black cabs outside the airport can be three times the price of a pre-booked taxi.
Luton
Some budget airlines (e.g. EasyJet) use Luton airport, which is about 35 miles from Cambridge. No intercontinental flights operate from Luton. Contact the Luton Airport web site for a list of operating companies.
There is no efficient train connection from Luton airport to Cambridge, but there is a coach service (JetLink 787) once every two hours, departing just outside the terminal building. It takes about 1.5 hours to reach Cambridge.
Taxi
Black cabs outside the airport can be three times the price of a pre-booked taxi.
London City
The City airport is located very close to the centre of London. It serves major European cities. See the London City Airportweb site for details. There is a shuttle bus from the airport that connects with the London Underground network.
Taxi
Black cabs outside the airport can be three times the price of a pre-booked taxi.
Talks
- Welcome
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- Feltre
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- Momcheva
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- Gilbank
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- Schaerer
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- Forrest
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- Puglisi
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- Talia
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- Fletcher
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- Reddy
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- Masters
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- Uebler
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- Willott
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- Matthee
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- Marchi
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- Maseda
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- Stark
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- Castellano
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- Sobral
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- Calabro
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- Wilkins
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- Jones
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- Curti
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- SanchezAlmeida
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- Sanders
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- Shapley
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- Straatman
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- Strom
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- Tiley
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- VanDerWel
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- Patricio
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- VidalGarcia
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- Peroux
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- Nakajima
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- Discussion2
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- Siana
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- Turner
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- VyTran
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- Dave
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- Zanella
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- Bowler
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- Brinchmann
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- Hirschmann
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- CurtisLake
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- Kumari
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- PerezMontero
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- Bunker
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- Mannucci
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- Vilchez
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- Discussion1
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- Robertson
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- Pentericci
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- LeFevre
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- Kassin
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- Terlevich
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- Ferrara
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- Summary.pdf
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- Hammer
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- Gomes
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