Remote Observing with HdA/MPIA's 50cm Telescope

Similar documents
Capturing and Processing Planetary Images. Petros Pissias Eumetsat Astronomy Club 11/06/2015

in the Mediterranean

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

Telescopes come in three basic styles

Capturing and Processing Deep Space Images. Petros Pissias Eumetsat Astronomy Club 15/03/2018

Photographing the Moon and the ISS. By Thierry Legault

ADVANCED CCD PHOTOMETRY AND EXOPLANET TRANSIT PHOTOMETRY. By : Kenny A. Diaz Eguigure

ADAS Guide to choosing the right Telescope. Produced by Members of the Society, Nov 2017

SimpleDreamEQ2. Upgrade kit equatorial mounts Synta EQ2, Celestron CG3. User guide. Micro GoTo system. Micro GoTo system

Astronomical Equipment for

CCD Astrometric Measurements of WDS Using the itelescope Network

College of San Mateo Observatory

CCD Astrometric Measurements of WDS using the itelescope network

Objectives: My objective in last night s test was to visually compare how changing the focal ratio of a telescope impacts the following:

The Telescopes and Activities on Exoplanet Detection in China. ZHOU Xu National Astronomical Observatories

High-resolution échelle at Skalnaté Pleso: future plans and development T. Pribulla

Small Aperture Amateur Observational Capabilities/Tools (Imaging/Photometry/Spectroscopy)

How to buy a telescope for your institution

A CubeSat Mission for Exoplanet Transit Detection and Astroseismology

OBSERVATIONS OF SATELLITES AND ASTEROIDS IN DERENIVKA, UKRIANE. V.Kudak, V.Perig, Y.Motrunych, I.Nojbauer

VIRUS: A giant spectrograph

SPACE DEBRIS OBSERVATION WITH THE NEW EQUIPMENTS ON SAYAN OBSERVATORY

WeatherWatcher ACP. Astronomers Control Panel (V4 or >) Ambient Virtual Weather Station (Pro or Internet editions) ASCOM platform v4.

Model SGS Dual CCD Self-Guiding Spectrograph

Optics and Telescopes

Training the Next Generation in Space Situational Awareness Research

Future Robotic observatory on Mountain Vidojevica: site and equipment specification

CONTENTS. vii. in this web service Cambridge University Press. Preface Acknowledgements. xiii xvi

Foundations of Astronomy 13e Seeds. Chapter 6. Light and Telescopes

Robotic Telescopes to Science and Public Outreach

C2A for Pulsar2 how to control your telescope from C2A

How Light Beams Behave. Light and Telescopes Guiding Questions. Telescopes A refracting telescope uses a lens to concentrate incoming light at a focus

ASTROPHOTOGRAPHY TARGETS Jan-Feb The Sun in Hydrogen Alpha By Theo Ramakers

Columbia University Astronomy Big Dome Telescope Start up/shut Down

The Norfolk State University 24-inch Rapid Response Robotic Telescope at Fan Mountain (Rev. September 12, 2012)

First observations of the second solar spectrum with spatial resolution at the Lunette Jean Rösch

A Rain Sensitive House Window Closes Automatically When Raining

Narrowband Imaging, or How to Image in Downtown Portland. Duncan Kitchin OMSI Astro Imaging Conference 2010

arxiv: v1 [astro-ph.im] 12 Oct 2015

The Kyiv internet telescope project

3/7/2018. Light and Telescope. PHYS 1411 Introduction to Astronomy. Topics for Today s class. What is a Telescopes?

LIBSlab ANALYZERS ANALYZERS

GERMAN TYPE EQUATORIAL MOUNT (FM 51/52 - FM 100/102 - FM150) USER MANUAL

Contents 1 Introduction

Stellar Observations Network Group

Chapter 6 Telescopes: Portals of Discovery. Agenda. How does your eye form an image? Refraction. Example: Refraction at Sunset

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

SOFT 423: Software Requirements

Refraction is the bending of light when it passes from one substance into another. Your eye uses refraction to focus light.

A Stand-alone Station and DSP Method for Deep Sky Objects Astrophotography

Getting Started: Using An Equatorial Telescope Mount: Everything You Need To Know For Astrophotography Or Visual Use By Allan Hall

Astronomy Lab Course. University of Alabama

Everything YOU wanted to know about Teaching High School Astronomy

» The observatory will be located uphill and north of the Reuter Center at the end of UNC Asheville s road-to-nowhere (Nut Hill Road).

RTS2 Remote Telescope System

TEACHING OBSERVATIONAL METHODS IN ASTROPHYSICS: REMOTE OBSERVATIONS FROM THE SCHOOL

Starlight in the university lab: Astrolab

Amateur Astronomer Participation in the TESS Exoplanet Mission

Light and Telescope 3/4/2018. PHYS 1403 Introduction to Astronomy. Guideposts (cont d.) Guidepost. Outline (continued) Outline.

Scientific Capability of the James Webb Space Telescope and the Mid-InfraRed Instrument

Hubble's Law and the Age of the Universe

Chapter 6 Telescopes: Portals of Discovery

Integration and Commissioning of the new UH Hilo Hoku Ke a Observatory Final Report Student: Callie Crowder 12/2/16

Chapter 6 Light and Telescopes

Observation of Light Curves of Space Objects. Hirohisa Kurosaki Japan Aerospace Exploration Agency Toshifumi Yanagisawa.

McMath-Pierce Adaptive Optics Overview. Christoph Keller National Solar Observatory, Tucson

Operating the Celestron 14 Telescope

Research Article Taiwan Automated Telescope Network

More Optical Telescopes

CCD Double-Star Measurements at Altimira Observatory in 2007

arxiv:astro-ph/ v2 6 Dec 2006

Astronomy. Optics and Telescopes

The VLT dealing with the Atmosphere, a Night Operation point of view

Instructional Planning Yearly Update

NASA Infrared Telescope Facility (IRTF) Alan Tokunaga

UNIWERSAŁ observatory dome

The Transneptunian Automated Occultation Survey (TAOS II) Matthew Lehner ASIAA

Light and Telescope 10/24/2018. PHYS 1403 Introduction to Astronomy. Reminder/Announcement. Chapter Outline. Chapter Outline (continued)

Astronomical "color"

Radio observations of the Milky Way from the classroom

PHYS/ASTR 2060 Popular Observational Astronomy(3) Syllabus

Six Things Everyone Should Know About Astronomy (With Activities)

Hubble Science Briefing

NAOYUKI TAMURA Subaru Instrument Astronomer Subaru Telescope, NAOJ

Lab 4: Stellar Spectroscopy

Housing of Robotic Telescopes Remote Hosting

D.A.R.V. (DSLR / CCD Drift Alignment by Robert Vice)

Mees Observatory telescope checklist

PIRATE The Winnower. Jakub Bochinski Open University

Pole searching algorithm for Wide-field all-sky image analyzing monitoring system

Quick Start Guide. The ieq45 GoTo German Equatorial Mount # 8000C

Venus 2012 transit: spectroscopy and high resolution observations proposals

a) Set the declination to trace the winter Sun's path and rising and setting points in

The URAT project August IAU GA Com. 8, Zacharias et al., the URAT project

Universe. Chapter 6. Optics and Telescopes 11/16/2014. By reading this chapter, you will learn. Tenth Edition

1 A photometric probe for Pan-STARRS

GIANO: pre-slit optics & telescope interface

Hyperion Observatory. Building an automatized observatory. Antonio Pérez Seminario de Astrofotografía. 31/10/2009 1

Amateur Astronomer Participation in the TESS Exoplanet Mission

Light and Telescope 10/22/2018. PHYS 1403 Introduction to Astronomy. Reminder/Announcement. Chapter Outline. Chapter Outline (continued)

Transcription:

Remote Observing with HdA/MPIA's 50cm Telescope Carolin Liefke AstroTechTalk May 5th 2017

Remote observing with HdA/MPIa's 50cm telescope The telescope and its instrumentation Remote observing how does it work? Remote vs. robotic telescopes Things to consider: Operations and protective measures Showcase: the ROTAT observatory at OHP Current status of turning the 50cm telescope into a remote observatory and ToDos Future opportunities for users Tour to the telescope

The Telescope Off-the-shelf 20 (51cm) Planewave astrograph, f = 3450mm, f/6.8 Modified Dall-Kirkham optics (elliptical primary, spherical secondary, field correction lens) Integrated motor focus Heavy-duty German equatorial mount 10micron GM4000 QCI Pointing model based GoTo function with (programmable) object database Both stand-alone or computercontrolled operation possible

The main camera Peltier-cooled wide field CCD camera Moravian Instruments G4 16000 Chip size 36x36mm, pixel size 9µ Moderate anti-blooming gate: linearity is ensured until saturation is reached Off-Axis guider with separate imager Photometric filters BVR c (Johnson-Cousins), Hα (8nm band width), O III (9.5nm band width), UV/IR cut

Examples First Light image of camera: M101 Exoplanet transit lightcurve Pluto astrometry at New Horizons arrival

Low- and mid-res spectrograph DADOS Gratings 200 or 900 lines/mm Three integrated slits: 25, 35 and 50 µm Spectral resolution: Δλ/λ up to 700 (200 lines/mm) and Δλ/λ up to 5000 (900 lines/mm) Can be used with eyepiece, DSLR or CCD (ST8-XME available) Guiding unit Magnitude limit: SNR 50 in 20 minute exposures with 25µm slit for m v 8 (200 lines/mm) and m v 6 (900 lines/mm)

Video astronomy (lucky imaging) Monochrome cameras DMK31, DMK41, ASI 120 and ASI 178 available for video imaging of planets, moon surface etc. Focal length multiplication with barlow lenses Single frames to be analyzed, quality-sorted and stacked by amateur software (e.g. Autostakkert, Registax) Additional image processing (sharpening) RGB color image creation with filters

Also available Taking pretty pictures with HdA-owned DSLRs (Canon EOS 450D and 750D) Adaptors to attach DSLRs from several manufacturers Light pollution reduction filters Several eyepieces and filters for visual observations but Typical time interval between observations: 1-2 months, mostly casual

Let s turn the 50cm telescope into a remote observatory!

Remote observing User operates the telescope via network, doing the same or similar steps as if on site. Physical presence at the telescope ideally not required at any time Everything has to be done remotely Telescope and camera control Opening/closing/moving the dome Switching power on and off Opening/closing covers/dust caps (Changing instruments) Requires additional hardware: Computer for controlling mount, focus and camera, dome control system, IP power controllers, motorized covers

Safety measures Protect the telescope against all kinds of damage resulting from technical or human failures Weather monitoring UPS unit for emergency shutdown for all necessary devices Automatic procedures? Cameras to monitor the telescope during operations Software blocker to avoid pointing the telescope towards the Sun Protect people at the telescope from injuries resulting from remote operation

Robotic telescopes Telescope operates automatically, no user interaction required Users specify observation settings (exposure times, filters, etc.) in advance Taking into account contraints (time interval, limits for air mass or moon distance, etc.), the control software optimizes scheduling Very efficient, making the most out of observing time. Examples: Las Cumbres Observatory, ESO Service Mode Overkill for observing conditions like in Heidelberg

Computer hardware Dome PC: Use amateur observatory control software for Windows, based on ASCOM driver platform integrating mount, camera, focus, dome control, guiding To be operated via remote desktop software, ideally Teamviewer ToDo: Replace the current PC with newer hardware; set up network environment Wishlist for the future: easy-to-use web interface

The dome control system In-house development of an angular transmitter based on a microcontroller with photo sensor and a pinhole gear wheel made by the precision mechanics workshop ToDo: Installation; RS232-controlled relay box for opening/closing/rotation; ASCOM software driver that enables dome tracking

Weather station and All-Sky camera Thesis projects at HdA in 2017 Robin Jäger: Setting up and testing an All-Sky camera with 24/7 operation Lars Meier: Setting up an online weather station and evaluate its data

Future use Telescope should be available to all MPIA staff after having an introduction HdA high school student projects (e.g. Heidelberger Life- Science Lab) In commissioning: Echelle spectrograph with Δλ/λ = 10.000/19.000 Remote imaging will be default, but visual observations and usage of other cameras or instruments still possible Booking system required

We want your project Suitable for all kinds of projects where a telescope of that size with Heidelberg s observing conditions is sufficient Lightcurves for variables, exoplanet transits Low- or mid-res spectra Monitoring programs Thesis or Miniforschung projects