• Study Resource
  • Explore
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
the Colours of rainbow the Brook
the Colours of rainbow the Brook

... through woods and valleys. The brook narrates the story of its musical journey along these places. Imagery of sight and sound are blended in the poem by employing exquisite words and expressions. Summary:“The brook” has been written by “Alfred Tennyson”. The poem traces the life of a brook or small ...
2 Justification and benefits in joining TMT
2 Justification and benefits in joining TMT

... questions with the next generation extremely large class telescopes such as the Thirty Meter Telescope (TMT). The Chinese participation in the TMT will place China in the forefront of astronomy for many decades to come; it can be a transformational experience for Chinese astronomy in terms of scienc ...
The size and shape of the Milky Way disc and halo from M
The size and shape of the Milky Way disc and halo from M

... we will include them in this paper. Brown dwarfs are believed to be among the most numerous luminous objects in our Milky Way. Studying them can thus tell us a lot about the structure of the Milky Way. Brown dwarfs resemble high-redshift galaxies in both colour and angular size. For example, redshif ...
Star Clusters in Mergers
Star Clusters in Mergers

... their distance), hence only slightly fainter. Statistics not different physics. ...
GMRT search for 150 MHz radio emission from the transiting
GMRT search for 150 MHz radio emission from the transiting

... flagged at various stages. The data for the antennas with relatively large errors in antenna-based gain solutions were examined and flagged over the corresponding time ranges. Some baselines were flagged, in view of large closure errors found on the bandpass calibrator. Channel- and time-based flagg ...
powerpoint - High Energy Physics at Wayne State
powerpoint - High Energy Physics at Wayne State

... Astronomy is a Time Machine When we observe a star that is 100 light-years distant, then the light took 100 years to reach us. We are seeing it as it was 100 years ago. The nearest galaxy is about a million light-years from Earth. We see it as it was 1 million years ago. The most distant objects ob ...
SOFIA`s Invisible Universe - Deutsches SOFIA Institut
SOFIA`s Invisible Universe - Deutsches SOFIA Institut

... A Lockheed C141 Starlifter cargo jet aircraft was modified to carry a 91.5 cm (36 inch) telescope mounted inside an opening in front of the wing. Because of the much larger telescope diameter then the Learjet observatory, a better and deeper view into the universe was possible (NASA photography arch ...
First young loose association in the northern hemisphere?
First young loose association in the northern hemisphere?

... !!Most stars detected by the ROSAT mission are younger than 1 Gyr (e.g. Motch et al. 1997). !!Taking account this property, Guillout et al. (1999) cross-correlated the ROSAT All-Sky Survey (RASS) with the Tycho catalogue creating the largest ("14 000 active stars) and most comprehensive set of late- ...
Microsatellite Star Tracker Baffles
Microsatellite Star Tracker Baffles

... It may also occur that several individual pixels may satused to orient the sensor. Simulated sun illumination was urate randomly (specifically for images with longer exproduced by a 75 W Xenon arc-lamp. The light source posure times) so it may be useful to spatially smooth the was coupled to an inte ...
The local spiral structure of the Milky Way
The local spiral structure of the Milky Way

... line in Fig. 2 suggests, these sources trace what appears to be a high-inclination spur bridging the Local Arm to the Sagittarius Arm near l ≈ 50°. Additional evidence for this spur is provided by large-scale molecular emission from CO, as shown in the l-V diagram in Fig. 3. Assuming circular motion ...
3. The MONS Telescope requirements
3. The MONS Telescope requirements

... We assume that the ACS power spectrum is flat at frequencies below 10 mHz, which should be the case if the control loop is operating correctly. We then assume that the ACS power spectrum falls off as frequency squared (i.e., as 1/f in amplitude), as seems likely. The spectrum can then level out at f ...
Black-Body SNR Formulation of Astronomical Camera
Black-Body SNR Formulation of Astronomical Camera

... decreases the optical performance because of an increase of the aberations. It follows that it is not possible to build an optimal camera that can be used for all situations and therefore, it is common practice to build camera systems considering the requirements of the capturing purpose. This, howe ...
Night Photography
Night Photography

... Can be used to blend one raw image processed differently (once for shadows, once for highlights) I use TuFuse and/or TuFuse Pro for Exposure blending: ...
Stars, Galaxies, Superuniverses and the Urantia Book, by Frederick
Stars, Galaxies, Superuniverses and the Urantia Book, by Frederick

... "Your world, Urantia, is one of many similar inhabited planets which comprise the local universe of Nebadon. This universe, together with similar creations, makes up the superuniverse of Orvonton, from whose capital, Uversa, our commission hails. Orvonton is one of the seven evolutionary superuniver ...
July - Rose City Astronomers
July - Rose City Astronomers

... for binoculars that has been created for this purpose by the This same chart can also be used that very evening for making real time observations with binoculars and small telescopes. I AAVSO: will also bring a few charts of a dimmer star for those that http://www.aavso.org/ want to use their larger ...
Strongly Interacting Supernovae - The National Centre for Radio
Strongly Interacting Supernovae - The National Centre for Radio

Observational Studies of Interacting Galaxies and the Development
Observational Studies of Interacting Galaxies and the Development

... are not all formed via merging processes, unless the merging timescale is much longer than the expected value. Spectroscopically, the kinematic properties of close pair galaxies were studied to understand how star formation were quenched at z ∼ 0.5. I discovered that the number of red-red pairs are ...
IRAM Annual Report 2012
IRAM Annual Report 2012

Disks around low-mass stars in extreme environments
Disks around low-mass stars in extreme environments

... large enough to sample the top of the IMF close enough to study low-mass stars 1'' = 420 AU = 0.002 pc ...
The Next Great Exoplanet Hunt Please share
The Next Great Exoplanet Hunt Please share

Superbubble Activity in Star-Forming Galaxies M. S. Oey
Superbubble Activity in Star-Forming Galaxies M. S. Oey

... emission has been detected within many objects, which is qualitatively consistent with the adiabatic evolution model. Two classes of X-ray emission have been identified: objects with X-ray luminosity Lx in excess of the model’s prediction (Chu & Mac Low 1990; Wang & Helfand 1991), and objects that r ...
ESOP August 2013
ESOP August 2013

... Observatory, where he still makes most of his observations • Most observations are recorded in the infrared, allowing higher S/N and even some daytime observations • Observations are concentrated on times when the Moon traverses the Galactic center region, an area of obvious high interest; a hundred ...
Detection of the Stochastic Background of nHz Gravitational Radiation from Massive Black
Detection of the Stochastic Background of nHz Gravitational Radiation from Massive Black

... pulsars, and to 500,000 km in the slowest and rotates rigidly with star. The radio beam (yellow) is driven by a voltage generated by the spinning field in conducting medium -- analogous to the spinning conductor in a fixed field common to most electric generators. ...
Type Ia Supernovae as distance indicators
Type Ia Supernovae as distance indicators

... –Type Ib: Strong He • Essentially no H or Si ...
SGS - SBIG
SGS - SBIG

< 1 ... 19 20 21 22 23 24 25 26 27 ... 141 >

Hubble Deep Field



The Hubble Deep Field (HDF) is an image of a small region in the constellation Ursa Major, constructed from a series of observations by the Hubble Space Telescope. It covers an area 2.5 arcminutes across, about one 24-millionth of the whole sky, which is equivalent in angular size to a 65 mm tennis ball at a distance of 100 metres. The image was assembled from 342 separate exposures taken with the Space Telescope's Wide Field and Planetary Camera 2 over ten consecutive days between December 18 and December 28, 1995.The field is so small that only a few foreground stars in the Milky Way lie within it; thus, almost all of the 3,000 objects in the image are galaxies, some of which are among the youngest and most distant known. By revealing such large numbers of very young galaxies, the HDF has become a landmark image in the study of the early universe, with the associated scientific paper having received over 900 citations by the end of 2014.Three years after the HDF observations were taken, a region in the south celestial hemisphere was imaged in a similar way and named the Hubble Deep Field South. The similarities between the two regions strengthened the belief that the universe is uniform over large scales and that the Earth occupies a typical region in the Universe (the cosmological principle). A wider but shallower survey was also made as part of the Great Observatories Origins Deep Survey. In 2004 a deeper image, known as the Hubble Ultra-Deep Field (HUDF), was constructed from a few months of light exposure. The HUDF image was at the time the most sensitive astronomical image ever made at visible wavelengths, and it remained so until the Hubble Extreme Deep Field (XDF) was released in 2012.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report