Synoptic Surveys: Boutique & Experiments
August 28 and 29
Hameetman Auditorium, Cahill Astrophysics,
Caltech Campus, Pasadena, California
BACKGROUND:
Surveys have many parameters: depth, cadence, choice of filters and
choice of sky pointings. The purpose of this workshop is to
critically examine the value of specialized surveys and then
forecast the future of specialized surveys in coming decade.
"Boutique" surveys are surveys which deliberately make drastic
choices (which could be rooted in financial issues or a deliberate
focus of the PI) in the survey parameters (listed above). The
ASAS (All Sky Automated Survey) and the on-going ASASSN (ASAS SN)
are exemplars of a boutique survey. In the radio, the Owens Valley
Long Wavelength Array (LWA) has a survey speed 50 times larger than
that of LOFAR-LBA. All these projects
are widely considered to be highly cost effective.
"Experiments" are imaging surveys which are focused on a single or
a well defined goal. The CFHT Legacy Survey (CFHTLS) was focused
strongly on Ia supernova cosmology and was considered to be an
extremely successful survey. The Catalina Sky Survey (CSS) is focused
on finding near-earth asteroids (NEOs) and the choice of filter
(white light) and cadence is tuned for NEO discovery. CSS has, over
nearly a decade, dominated the discovery of NEOs.
"Non TDA but Boutique" Well known examples of experiments are
microlensing surveys and searches for planets via occultation.
Non-time domain boutique surveys include Low Surface brightness
surveys, Narrow-band surveys (Halpha, other neublar lines) and
Polarization surveys.
In Projects we list an incomplete
list of Boutiques and Experiments.
See also
Time Domain Resources for additional projects.
MEETING:
There are two purposes for this meeting. First, one purpose of the
meeting is to understand the role and value of smaller surveys once
larger surveys get going. The proponents of large surveys (naturally)
have been known to claim that large etendues make all other surveys
superfluous. It may well be true but it would be good to have a
nuanced and scholarly discussion.
The second purpose of the meeting is to explore new concepts
or usages of time domain surveys. To aid this goal PIs will first
describe the current status and future prospects of their surveys.
We plan to have good discussion and brain storming to explore
novel usages (e.g. comensal surveys, joint surveys).
When this workshop was conceived there was a planned limit of
60 (so we could have lots of discussion) but the
participants
response was much stronger than anticipated. We have
now extended the meeting to two full days (Friday& Saturday) so
that there will be ample time for discussions.
There is no registration fee. However, we do need to know the head
count accurately for finanical planning reasons.
We are providing a nice ``notebook"
and continental breakfasts, one dinner and refreshments.
Please note that the 2015
PTF Summer School precedes this meeting (August 24-27). You
are welcome to attend that meeting (but then do please register
etc). Also consult this workshop's URL for all matters logistics.
SPEAKERS
IMPORTANT NOTE TO SPEAKERS: Please read
THIS
PRESENTATIONS
Can be found
here
OUTPUT OF THE MEETING
The "proceedings" of the meeting is available, in the form
of a "notebook", one week ahead
of the meeting at this
URL
Each participant will
be supplied with his/her own copy of the notebook (with your name
written on the cover!).
No other ``swag" will be provided.
Please bring your own pens, pencils and
erasers.
List of Participants
- [a] R. Adhikari, Caltech
- [a] M. Anderson, Caltech
- [a] T. Barclay, NASA-Ames
- [a] E. Bellm, Caltech
- [a] L. Bildsten, KITP, UC Santa Barbara
- [a] P. Bilgi, Caltech
- [a] T. Boroson, LCOGT
- [a] G. Bower, ASIAA-Hilo
- [a] S. Bradley Cenko, GSFC
- [a] Y. Cao, Caltech
- [a] R. Chari, IPAC
- [a] J. Cohen, Caltech
- [a] P. Copperthwaite, Harvard
- [a] D. Cook, WIRO to Caltech,
- [a] J. Cooke, Swinburne, Australia
- [a] L. D'Addorio, JPL
- [a] D. Duev, JIVE to Caltech
- [a] G. Duggan, Caltech
- [a] H. Flewelling, IfA
- [a] D. Frail, NRAO
- [a] S. Gezari, UMd
- [a] V. Giryanskaya, Caltech
- [a] G. Hallinan, Caltech
- [a] G. Helou, IPAC
- [a] L. Hillenbrand, Caltech
- [a] A. Ho, MPIA to Caltech
- [a] A. Horesh, Weizmann
- [a] A. Howell, LCOGT
- [a] P. Groot, Radboud, NL
- [a] J. Jensen, Caltech
- [a] M. Juric, UW/LSST
- [a] M. Kasliwal, Caltech
- [a] N. Kawai, Tokyo Tech, Japan
- [a] V. Kaspi, McGill University, Canada
- [a] R. Kirshner, Moore Foundation
- [a] N. Konidaris, Caltech
- [a] S. Kulkarni, Caltech
- [a] T. Kupfer, Radboud to Caltech
- [a] N. Law, UNC, Chapel Hill
- [a] J. Lazio, JPL
- [a] R. Lupton, Princeton
- [a] R. Lunnan, Harvard to Caltech
- [a] A. Mahabal, Caltech
- [a] N. Mahesh, UCLA
- [a] T. Matheson, NOAO
- [a] A. Miller, JPL
- [a] C. Mingarelli, Caltech
- [a] E. Murphy, IPAC
- [a] P. Nugent, LBNL
- [a] C. Ngeow, NCU, Taiwan
- [a] T. Pearson, Caltech
- [a] A. Piro, Carnegie
- [a] T. Prince, Caltech, UK
- [a] E. Quataert, UCB
- [a] R. Quimby, SDSU
- [a] V. Ravi, Melbourne to Caltech
- [a] A. Readhead, Caltech
- [a] A. Rest, STScI
- [a] G. Ricker, MIT
- [a] S. Ridgway, NOAO
- [a] J. Schwab, UCB
- [a] B. Sesar, MPIA, Germany
- [a] A. Shafter, SDSU
- [a] M. Shao, JPL
- [a] B. Shappee, Carnegie
- [a] P. Szkody, UW
- [a] P. van Dokkum, Yale
- [a] T. Vestrand, LANL
- [a] R. Walters, Caltech
- [a] S. Weinreb, JPL
- [a] A. Weinstein, Caltech
- [a] L. Yan, Caltech
- [a] A. Janzen, Caltech
a .. confirmed
* .. plan to attend
? .. hoping to come (subject only to logistics)
T .. unclear (misc)
UNABLE TO ATTEND or NO REPLY:
J. Tonry, IfA-Manoa |
K. Stanek, OSU |
C. Stubbs, Harvard |
D. Bhattacharya, IUCAA |
M. van Kerkwijk, UToronto |
M. Bailes |
N. Gehrels |
M. Ouchi |
J. Kollmeier |
A. Gould |
C. Kochanek |
ZTF-CSAC (remaining): Agueros (Columbia), Pinsonneault (OSU) |
List of Projects
The list below is particularly incomplete with respect to exoplanet
projects.
- All-Sky Automated Search for Supernovae (ASAS-SN)
- Catalina Sky Survey (CSS)
- Catalina Real-Time Transient Survey (CRTS)
- Dark Energy Survey (DES)
- Evryscope
- Desert Fireball Network (DFN)
- Gaia Alerts
- Intermediate Palomar Transient Factory (iPTF)
- Kepler-2 (K2)
- KELT-South
- Kilodegree Extremely Little Telescopes (KELT-North)
- Kepler
- La Silla Quest
- Large Synoptic Survey Telescope (LSST)
- MeerLICHT
- Near-Earth Objects via the Wide-field Infrared Survey Explorer (NEOWISE)
- Optical Gravitation Lensing Experiment (OGLE)
- Panoramic Survey Telescope and Rapid Response System (Pan-STARRS)
- Pi of the Sky
- SkyMapper Southern Sky Survey
- Spacewatch
- Transneptunian Automated Occultation Survey (TAOS II)
- TESS
- Zwicky Transient Factory (ZTF)
- Australian SKA Pathfinder (ASKAP)
- BRIght Target Explorer (BRITE)
- Exploring the X-ray Transient and variable Sky (EXTraS)
- Fermi Gamma-Ray Space Telescope
- Gaia
- LOFAR
- Laser Interferometer Gravitational-wave Observatory (LIGO)
- LOFAR Transient Key Project
- Square Kilometer Array (SKA
- Swift X-Ray Obsrevatory
- ThunderKAT
- VLA Low Band Ionospheric and Transient Experiment (VLITE)
- LWA
Automated Planet Finder (APF)
Deep Lens Survey (DLS)
Near-Earth Asteroid Tracking (NEAT)
Palomar-Quest Sky Survey (PQ)
Sentinel Mission (B612)
Sloan Digital Sky Survey (SDSS)
Missing: WASP et al, KMT Network,