Discussions about the observing strategy for the HDF-S focussed primarily on the questions: . What filters/gratings to use for each instrument ? What exposure time to use for each filter/grating ? ... Different areas of the Version 1 output image correspond to variable amounts of exposure time, due to the relatively large pointing shifts necessitated by the multi-instrument observing strategy. ... WFPC-2 Filters, exposure times and limiting AB magnitudes for Version 1 images . Filter . ...

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• HST Observer Monthly
• STIS Instrument Handbook
• Emission Line Observations of Galaxy Nuclei

M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

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• Low Surface Brightness Galaxy Gallery
• Astro-2 and the UIT Experiment

... Observing . Observing details . ... Mike Keith has code to parse these schedules to produce a list of pulsar-specific Parkes observing. ... Please identify which observing sessions you can support and then click on "add new" on Mike's pulsar-specific schedule to add your name to the roster. ... Familiarise yourself with the current remote observing documentation listed below. ... The PPTA dashboard allows anyone to view the log from the current or any previous observing session: . ... PPTA log . ...

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• Evolutionary Paths in Galaxy Morphology
• PPTA Wiki | Main / Observing
• A new twist to polar rings

... Science Users Information > Science and Technical Meetings > Conferences 2016 > Discs in Galaxies . ... Observing Facilities . ... Observing with ESO Telescopes . ... The aim of this Joint international conference is to explore the importance of stellar and gaseous discs in a variety of galaxies from high redshift to the Milky Way in the context of exciting new observations and numerical simulations. ... What are the prospects for observing and interpreting metal gradients in high redshift galaxies?...

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• ESO - Studying the Cosmological Evolution of Galaxy Clusters with (Sub-)mm
• ESO - VIMOS Science Verification Programs at Melipal/UT3
• ESO - Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies

Proposal Identification No.: ... Proposal Type: General Category: Sub-Category: Observation Category: Time Requested this semester: Hours Next Semester: Hours already used for this pro ject: Additional Hours required to complete pro ject: Minimum Useful Time : Expected Data Storage: Prop osal Title: ABSTRACT: Commensal Astronomy Spectroscopy Galactic 0 ( commensal observing only) 0 ( commensal observing only) 1030 650 1h less than 100 GB ... For these observations night-time is required. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/DarlingtagA1902tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/DarlingtagA1902tp.ps
• http://www.naic.edu/vscience/schedule/2014Spring/BradfordtagA2850.pdf

... A radio galaxy is a galaxy that emits an unusually big amount of energy at radio wavelengths. ... Inside of each galaxy with an active nucleus (radio galaxies are among them) there must be a system of a "central machine" responsible for the colossal amount of the emitted energy from radio to gamma ranges. ... Sometimes a radio source in an active galaxy may flare again if the needed conditions appear (a new portion of matter would fall into the furnace of the "central machine"). ...

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• Galaxy sector, archive 2012
• Galaxy sector, archive 2014
• Measurement of the dark halo shape in polar ring galaxies

... Galaxy Evolution home . ... Regulating the ISM and star formation . Cosmological evolution of star-forming galaxies . ... Local Information . ... In order to investigate the cosmological evolution of star-forming galaxies it is essential that we understand the physics which controls the evolution and regulation of star formation in the ISM. ... We use a combined observational and numerical approach to study interacting and merging galaxies in the local Universe. ...

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• Galaxy Evolution: Cosmological evolution of star formation
• Galaxy Evolution: EVN Deadline
• Galaxy Evolution: The origin and evoltuion of radio sources

... Meade Instruments Corporation . ... Refracting telescopes (Meade Models NG-60, NGC-60, DS-2070AT, ETX-70AT, LXD55-AR5, LX55-AR6 ) and mirror-lens telescopes ( ETX-90AT, 105AT, 125AT, LXD55-SC8, 8LX90, LX200 GPS Series ) are generally more versatile in a wide array of land and astronomical applications. ... The intermediate-level observer, or the non-casual telescope user who wishes to purchase one telescope for a lifetime, should consider a Meade Model LXD55 series, 8LX90, or LX200GPS. ... Meade 4M ...

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• ETX-80 Hard Carry Case
• Meade Series 4000 Broadband Nebular Filters
• ETX90 Observer

... The commissioning of the FORS2 multi-mode astronomical instrument at KUEYEN , the second FOcal Reducer/low dispersion Spectrograph at the ESO Very Large Telescope, was successfully finished today. ... FORS2 is now ready to be handed over to the astronomers on April 1, 2000. ... Additional information about the VLT Data Flow System is available in ESO PR 10/99 . ... ESO Press Photo 05a/00 . Preview; JPEG: 400 x 452; 52k] . ... This is the caption to ESO PR Photos 05a-c/00 . ...

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• K-band Arcetri Obscured Supernova Search - What is the KAOSS Projrect?
• Lunar Occultation Group at AAO
• Tracing Dust in Spiral Galaxies

... In this paper we present the results of detailed B, V, R, I, and H study of the isolated nearby blue compact dwarf (BCD) galaxy NGC6789. Judging from the literature the observed galaxy has not been resolved into stars up to now. ... The distance of the galaxy, estimated from the tip of the red giant branch (TRGB) is 2.1 Mpc which places NGC6789 close to the Local Group. ... Key words: nearby galaxies: dwarf galaxies (NGC 6789): distance moduli: star content . ... Distance. ...

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• Polar-Ring Galaxies

Next: Transparency of the Stochastic Up: Model of the Galaxy Previous: Frequency distribution of galactic . ... The parameters of the model resulted from a numerical fitting of various data, such as the observed distribution of the young star population and neutral hydrogen, the density of population II stars in the vicinity of the Sun, the galactic rotation curve and the dynamics and distribution of globular clusters   and dwarf irregular satellites of the Galaxy. ...

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• Gamma-Ray Bursts

... Data Analysis SAS News What is SAS? ... Calibration & Background Calibration Background Analysis . SOC Info XMM-Newton Contact Details How to get to ESAC ESA Research Fellowships ESAC Trainee Projects ESA Young Graduate Trainees . ... Other Links Project Related Links Research Projects Other X-ray Missions Space Weather Links . The Science Operations and Data Systems Division of ESA's Research and Scientific Support Department develops and runs astronomy projects in space. ...

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• XMM-Newton Trainee Project 2004
• Instrument Details Record
• Detailed Description

ATMoB "Galaxy Observing Award " Guidelines Purpose: To promote observing among the membership of the Amateur Telescope Makers of Boston through participation in the Galaxy Observing Awards program. ... Examples of elliptical galaxies: M49, M59, M60, M87, NGC 4125. Limiting Magnitude Assessment: Spirals: A spiral galaxy consists of a flattened disk, with stars forming a (usually two-armed) spiral structure, and a central concentration of stars known as the bulge. ...

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• Amateur Telescope Makers of Boston ATMoB Observing Awards Program
• Amateur Telescope Makers of Boston

... 145Slee,Roy Savage We present detailed radio and optical parameters for the stronger radio sources in 58 Abell cluster fields observed with the Very Large Array (VLA) using scaled arrays at 1.5 and 4.9 GHz. ... The cluster fields were distributed over 24 h of RA and between declinations +35 deg and -30 deg. ... Optical identifications Cluster Source Radio Centroid Optical Position EF Ang. ...

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• The Hamburg/SAO Survey for Emission-Line Galaxies
• Results and Discussion
• Observations and Reduction

... The SMS program is a critical endeavor to investigate whether the predictions of standard cold dark matter cosmology are consistent with the observed matter distribution in the Milky Way halo. It is the deepest, most extended search for optically elusive dwarf satellite galaxies and tidal streams to date, covering the entire Southern hemisphere. ... However only a few dwarf satellites have been found around the Milky Way to date - 22 dwarfs compared to 500-10,000 predicted by theory (Klypin et al. ...

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• GSAOI Disk Galaxies Science Page
• Philip Lah's Research
• Dougal Mackey - CV

... Here some data observed on the 6m telescope with IFP installed in the OLD focal reducer are presented. ... Mkn 3: velocity field . ... NGC 5252: [OIII] image . ... NGC 5252 was observed 23 Feb. 1998 in the [OIII]5007 emission line with CCD TK1024 as detector. ... We observed the ionized gas velocity fields of the spiral galaxies with two purpose. ... Restored velocity field of NGC 157 in the reference frame rotating with the pattern speed overlaid on the Ha image of the galaxy . ... NGC 4100 . ...

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• GRB follow-up team
• These galaxies were observed (Project: vortex)
• SCORPIO: Direct images

Astronotes Armagh Planetarium's Stellar Blog! ... Our Galaxy . ... Other Galaxies . ... Space Flight . ... When Galaxies Collide (Image credit: ALMA (ESO/NAOJ/NRAO). Visible light image: the NASA/ESA Hubble Space Telescope) . In the southern sky constellation of Corvus (the Crow), we see the Antennae Galaxies (alias NGC 4038 and 4039). ... Your email address will not be published. ... Here you will find the latest news and views from the fascinating worlds of astronomy and space exploration. ...

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• Telescope nights at Armagh Planetarium | Astronotes
• observing | Astronotes - Part 4
• Supernova in the Cigar Galaxy | Astronotes

. This artist's impression shows a galaxy located between an observer on Earth and a background quasar that acts as a beacon. The light that travels from the quasar is intercepted by the foreground galaxy on its sightline, carrying out the galaxy's signature all the way to the observer. The sketch shows a side-on view of the system. The inset shows a face-on view of it, the same view captured (albeit with less detail) by the images taken with the SINFONI instrument on ESO's Very Large Telescope. ESO

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• ESA chooses instruments for its Jupiter ICy moons Explorer | Astronomy.com
• Sagittarius in detail | Astronomy.com
• First detailed look at a normal galaxy in the early universe | Astronomy.com

ARCSAT ID NUMBER: AS06 DESCRIPTIVE TITLE: Stromgren Photometry of Galactic Peripherys and Streams PI: Dmitry Bizyaev OBSERVER(S): Dmitry Bizyaev UNCERTIFIED/UNTRAINED OBSERVERS: N/A COLLABORATORS: CONTACT INFORMATION: dmbiz@apo.nmsu.edu TIME REQUESTED: 1 week in the dark time between April 17 and July 3, 2016 INSTRUMENT: SurveyCam FILTERS : Stromgren uvby, 2 square COMMENTS: remote observations BRIEF SCIENCE JUSTIFICATION: Last decade numerous faint ... 2014). ... 2014, ApJ, 787, 24 ...

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• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_jan2016/AS06.html
• http://www.apo.nmsu.edu/Telescopes/ARCSAT/ObsSchedules/arcsat_may2015/AS06.html
• Instruments

... Previous: Substepping and its Application to HST Imaging . ... This is a preliminary report on an application of the co-addition technique based upon the Richardson-Lucy algorithm. The combination of high signal-to-noise ground-based images obtained with the ESO NTT using SUSI with high angular resolution HST FOC f/96 images gives new insights on the properties of galaxy cores and their potential time variability. Cores of galaxies are one of the main thrusts of present extragalactic research. ...

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• A Distributed System for ``Phase II'' Proposal Preparation
• Asteroseismology-Observing for a SONG
• ETCs and Observations Simulation at the VLT