Deep Drilling Program. Lynne Jones LSST Performance Scien2st. LSST All Hands Mee6ng August 13-17, 2012

Similar documents
Present and Future Large Optical Transient Surveys. Supernovae Rates and Expectations

An end-to-end simulation framework for the Large Synoptic Survey Telescope Andrew Connolly University of Washington

The Yale/ODI Survey(s)

Tier 1 proposal and runs

The Large Synoptic Survey Telescope

Large Synoptic Survey Telescope

LCO Global Telescope Network: Operations and policies for a time-domain facility. Todd Boroson

THE DARK ENERGY SURVEY: 3 YEARS OF SUPERNOVA

Dark Sky Observing Preview. BSA Troop 4 Pasadena, CA

Phys 100 Astronomy (Dr. Ilias Fernini) Review Questions for Chapter 1

telescopes resolve it into many faint (i.e. distant) stars What does it tell us?

From the Big Bang to Big Data. Ofer Lahav (UCL)

MIDTERM PRACTICE EXAM ANSWERS

LSST Science. Željko Ivezić, LSST Project Scientist University of Washington

The Dark Energy Survey Public Data Release 1

SkyMapper and the Southern Sky Survey

Assignment #12 The Milky Way

SkyMapper and the Southern Sky Survey

The Earth Orbits the Sun Student Question Sheet (Advanced)

Astro 301/ Fall 2006 (50405) Introduction to Astronomy

If there is an edge to the universe, we should be able to see our way out of the woods. Olber s Paradox. This is called Olber s Paradox

What Objects Are Part of the Solar System?

What does the universe look like?

CIBER Measurements of the Mean Intensity of the NIR background

Exploring the Depths of the Universe

Mapping Document. GCSE (9-1) Astronomy. Pearson Edexcel Level 1/Level 2 GCSE (9-1) in Astronomy (1AS0)

Universe Celestial Object Galaxy Solar System

Synergies between and E-ELT

High Redshift Universe

Chapter 23: Dark Matter, Dark Energy & Future of the Universe. Galactic rotation curves

V. Astronomy Section

The Universe and Galaxies. Adapted from:

[FILE] MILKY WAY AT HOME EBOOK

Imaging with SPIRIT Exposure Guide

Outline: Part II. The end of the dark ages. Structure formation. Merging cold dark matter halos. First stars z t Univ Myr.

Introduction to SDSS -instruments, survey strategy, etc

Galaxies. The majority of known galaxies fall into one of three major classes: spirals (78 %), ellipticals (18 %) and irregulars (4 %).

Galaxies and the Universe

2. Very generally, describe how the Milky Way Galaxy formed. (Words or labeled picture)

It is a very human trait to wonder where we are in this universe. Usually, the only hint of the vastness of the universe comes at night.

JINA Observations, Now and in the Near Future

The Science Cases for CSTAR, AST3, and KDUST

Introduction to the Universe. What makes up the Universe?

Griffith Observatory Field Trip Guide

BENCHMARK SC.E.1.2.1

Let s Observe M31 and M45!

Astroimaging From Easy to Less Than Easy. S. Douglas Holland

Summer Messier List Observing Club

The Space Around Us. A quick overview of the solar system. Reid Pierce Lincoln Jr. High Bentonville, Arkansas

Current Status of MIRIS

LSST Cosmology and LSSTxCMB-S4 Synergies. Elisabeth Krause, Stanford

CST Prep- 8 th Grade Astronomy

Chapter 16 Dark Matter, Dark Energy, & The Fate of the Universe

Dark Energy. Cluster counts, weak lensing & Supernovae Ia all in one survey. Survey (DES)

TAKE A LOOK 2. Identify This star is in the last stage of its life cycle. What is that stage?

A. The moon B. The sun C. Jupiter D. Earth A. 1 B. 2 C. 3 D. 4. Sky Science Unit Review Konrad. Here is a selection of PAT style questions.

The Milky Way Galaxy. Some thoughts. How big is it? What does it look like? How did it end up this way? What is it made up of?

Chapter 15 The Milky Way Galaxy. The Milky Way

How do telescopes "see" on Earth and in space?

1. Galaxy (a) the length of a planet s day. 2. Rotational Period (b) dust and gases floating in space

The Milky Way & Galaxies

Outline 8: History of the Universe and Solar System

Plan. Questions? Syllabus; administrative details. Some Definitions. An Idea of Scale

Introduction to the Universe

Class 5 Cosmology Large-Scale Structure of the Universe What do we see? Big Bang Cosmology What model explains what we see?

The Big Bang Theory (page 854)

3. The diagram below shows the Moon at four positions in its orbit around Earth as viewed from above the North Pole.

Contents. Part I Developing Your Skills

Observational Astronomy Astro-25. Professor Meyer-Canales Saddleback College

Understanding Exoplanets and Other Variable Sources. in Sparsely-Sampled Time Domain Surveys. Michael B. Lund. Dissertation

refractors satellite electromagnetic radiation

Astronomy Universe: all of space and everything in it

Strong gravitational lenses in the 2020s

Énergie noire Formation des structures. N. Regnault C. Yèche

Age-redshift relation. The time since the big bang depends on the cosmological parameters.

Station #1 Galaxy Cards. Standard 4a: Students know galaxies are clusters of billions of stars and may have different shapes.

Land Surface Data AssimilaEon: DART and CLM

The Milky Way. Overview: Number of Stars Mass Shape Size Age Sun s location. First ideas about MW structure. Wide-angle photo of the Milky Way

Welcome to Astronomy 402/602

The WFIRST High La/tude Survey. Christopher Hirata, for the SDT November 18, 2014

Figure 69.01a. Formation of Stars

arxiv: v1 [astro-ph.im] 15 Nov 2018

NIRSpec Multi-Object Spectroscopy of Distant Galaxies

Galaxy formation and evolution. Astro 850

Planets in other Star Systems

Wednesday Jan. 22. Syllabus and class notes are at: go to courses, AST301 Introduction to Astronomy Lacy

Test Name: 09.LCW.0352.SCIENCE.GR Q1.S.THEUNIVERSE-SOLARSYSTEMHONORS Test ID: Date: 09/21/2017

JEWELS of the COSMIC DEEP Messier's first guide to the night sky

Supernovae with Euclid

The Evolution of Massive Galaxies at 3 < z < 7 (The Hawaii 20 deg 2 Survey H2O)

An Introduction to Galaxies and Cosmology. Jun 29, 2005 Chap.2.1~2.3

The Kepler Mission. NASA Discovery Mission # 10: Are there other planets, orbiting other stars, with characteristics similar to Earth?

Time Domain Astronomy in the 2020s:

Dark Baryons and their Hidden Places. Physics 554: Nuclear Astrophysics Towfiq Ahmed December 7, 2007

Apache Point Observatory

Microlensing (planet detection): theory and applications

Milky Way Structure. Nucleus Disk Halo Sun is about 30,000 LY from center

Space Test Review. Unit Test on Thursday April 17

Science Benchmark: 06 : 04 Standard 04: Stargazing universe, the light-year, speed of light Grade Benchmark Standard Page

Overview of Gaia-ESO Survey results based on high-resolution spectra of FGK-type stars Rodolfo Smiljanic! (Gaia-ESO WG11 co-coordinator)

Transcription:

Deep Drilling Program Lynne Jones LSST Performance Scien2st LSST All Hands Mee6ng August 13-17, 2012

Overview Topics to cover Super- quick review of DD request OpSim runs produced in response to request Highlight differences between runs: # of DDFs, field locaeons Coadded & single- visit depth in DD fields, Eme between obs Overall WFD completeness Process for going forward InteracEon between DD WG / OpSim / Science Council UpdaEng DD white papers & summarizing results from each set of opsim runs (iteraeve process) Timeline 2

Review of DD program request Large Scale Structure Low exenceon, high galacec laetude, high eclipec laetude, mule- wavelength observaeons ugrizy limit: 28.5 (ugri), 28.0 (z), 27.0 (y) no cadence constraints Weak Lensing ugrizy no cadence constraints limit: 5x main survey Galaxies ugrizy no cadence constraints limit: 28.0 (ugriz), 27.0 (y) Supernova Low exdncdon, high galacdc ladtude, visible to other telescopes with MOS grizy ObservaDons every few days throughout season in all filters Transients and Variable Stars Milky Way and Local Volume Solar System LMC, SMC, IC 4651 (open cluster) gr Dense -me sampling from few minutes to several days South galacdc pole, galacdc andcenter, one of three proposed open clusters ConjuncEon of Neptune and Jupiter Trojan points (in 2022, at RA=19:35, Dec=- 21:38) grizy limit: 29.0 (g), 27.0 (r), 28.9 (i) r limit: 27.0 (r) in each of 8 epochs Varied -me constraints between few minutes to years Tight -me constraints spread over a year 3

Review of DD request ExtragalacDc fields Transients/Variable Stars fields Milky Way fields Solar System fields grizy observa-ons in each sequence, every few nights (weighted toward z) Add u band exposures during dark -me grizy observa-ons in each sequence, every few nights (weighted toward z) Add u band exposures during dark -me g band con-nuous for 1 hour, then 7 more hours of observa-ons spaced over next 3 days; repeat in r then repeat in g and r again 30 nights of izy/izy/izy sequences every night gri sequences spread over 2 years 8 nights of 85 minutes of con-nuous r band observa-ons, spaced at par-cular intervals over one year 5 fields with 265 nights of grizy, and addidonal u band - 1675 hrs 5 fields with 265 nights of grizy, and addidonal u band - 1547 hrs 6 fields - 192 hrs 3 fields - 407 hrs 9 fields - 102 hrs 4

OpSim Runs in response to DD request OpSim runs produced in response to request TVS / Milky Way / Solar System fields not yet included in runs ExtragalacEc fields implemented, including some variaeons.. with full 10 fields, ~1.5x oversubscripeon vs opsim3.61 Run opsim6.24 opsim4.262 opsim8.26 opsim5.211 opsim6.27 opsim6.267 Short Descrip0on No DD fields Updated opsim3.61 (i.e. 6 old strawman DD fields) 4 (sci council) DD fields 4 (sci council) DD fields + 1 more 4 (sci council) DD fields + 6 more (selected by opsim) 4 (sci council) DD fields + 6 more (selected by DD WG) 5

Download links on science wiki - see DD pages hlps://www.lsstcorp.org/sciencewiki/index.php?etle=dd_firstopsim hlps://www.lsstcorp.org/sciencewiki/index.php?etle=deep_drilling_fields 6

Opsim 4.262 (6 DDFs, old obs request) 7

Opsim 8.26 (4 SC DDFs) 8

Opsim 5.211 (4 SC DDFs + 1) 9

Opsim 6.27 (4 SC DDFs + 6 more) 10

Opsim 4.267 (4 SC DDFs + 6 more from DDWG) 11

Opsim 4.262 (6 DDFs, old obs request) 12

Opsim 8.26 (4 SC DDFs) 13

Opsim 5.211 (4 SC DDFs + 1) 14

Opsim 6.27 (4 SC DDFs + 6 more) 15

Opsim 4.267 (4 SC DDFs + 6 more from DDWG) 16

Opsim 4.262 (6 DDFs, old obs request) 17

Opsim 8.26 (4 SC DDFs) 18

Opsim 5.211 (4 SC DDFs + 1) 19

Opsim 6.27 (4 SC DDFs + 6 more) 20

Opsim 4.267 (4 SC DDFs + 6 more from DDWG) 21

Opsim 4.262 (6 DDFs, old obs request) 22

Opsim 8.26 (4 SC DDFs) 23

Opsim 5.211 (4 SC DDFs + 1) 24

Opsim 6.27 (4 SC DDFs + 6 more) 25

Opsim 4.267 (4 SC DDFs + 6 more from DDWG) 26

Effect on WFD - reduced completeness Description No DD 6 old DDFs 4 SC DDFs 4 SC + 1 4 SC + 6 more 4 SC + 6 DD WG Run Name opsim6.24 opsim4.262 opsim8.26 opsim5.211 opsim6.27 opsim4.267 Total Visits* 2,307,343 2,272,508 2,310,444 2,334,341 2,372,537 2,479,519 Average Slew Time 9.59 s 8.51 s 7.51 s 7.10 s 6.62 s 6.36 s 100 <= P 2216 1486 1096 870 693 512 90 <= P 2229 1512 1109 888 698 524 80 <= P 2245 1705 1202 1007 731 558 70 <= P 2280 2182 1900 1847 1436 1330 60 <= P 2286 2240 2168 2213 1768 1665 50 <= P 2291 2283 2263 2255 2023 2040 40 <= P 2293 2290 2289 2279 2135 2253 30 <= P - 2293 2292 2291 2215 2289 20 <= P - - 2293 2293 2264 2290 10 <= P - - - - 2284 2293 0 < P - - - - 2293-27

Opsim 6.24 (no DDFs) 28

Opsim 4.262 (6 DDFs, old obs request) 29

Opsim 8.26 (4 SC DDFs) 30

Opsim 5.211 (4 SC DDFs + 1) 31

Opsim 6.27 (4 SC DDFs + 6 more) 32

Opsim 4.267 (4 SC DDFs + 6 more from DDWG) 33

Effect on WFD + other mini- surveys Compare runs with metrics captured in SSTAR report and other OpSim tools 34

So what s next? Process for going forward InteracEon between DD WG / OpSim / Science Council Update DD white papers & summarizing results from each set of opsim runs EvaluaEng DD runs for DD science - DDWG EvaluaEng DD runs for general science - OpSim General report on each iteraeon, recommendaeons & guide for further development SC can provide feedback if necessary Timeline General rule: delay choices as long as possible (first light) Do we need to pick more fields on an earlier Emescale? Review before end of commissioning period 35

Feedback