You Can Make Stellar Images Brighter . Articles | ... A few months ago I wrote an article titled "You Can?t Make Them Brighter". So why am I now writing that you can make them brighter. ... The image of a focused star is actually a small disk called the Airy disk, named after the 19 th century scientist Sir George Airy. ... For a given aperture, a smaller Airy disk means that the light is focused to a smaller disk and is therefore brighter. ... www.astronomy.net . About Astronomy Net | ...

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• New Model: How Do The Sun And Moon Appear To Move Across The Sky - an Astronomy
• You Can't Make Stellar Images Brighter - an Astronomy Net Article
• The Astronomy Shop - Posters - by Astronomy Net

... SEARCH ASP SITE: Match ALL words Match ANY word . ... ASP Conference Series . ... Accidental Astrophysics: The Devil's In the Magnitudes, Part II . ... The star second to the Sun in brilliance is Sirius. ... Recall the magnitude system, passed down to us through a hundred generations of sky watchers, as a means of quantifying stellar brightness ("Accidental Astrophysics," May/June, p. 9). ... Yes, it is a magnitude difference, but that difference is due to the distance between us and the star. ...

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• ASP: Monster Comet Promises Big Show
• ASP: Star Science in the Autumn Sky
• ASP: An Ancient Universe - The Age of the Expanding Universe

... One of the Case galaxies appeared to be a distant and bright AGN. This is CG 273 ( = 09 h 39 m 05 s .8, = +35 36'42", m CG =18 mag). Only one prominent emission line is seen in the wavelength range 3600 - 5500 ?. ... We identify it with the Mg II doublet 2798 ?, the corresponding redshift is 0.670. With the Hubble constant 75 km s -1 Mpc -1 and q 0 =0.5 its absolute blue magnitude M B = -25 mag, which places CG 273 to the class of quasars. ... 1/10/1998 ...

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• CMOS tutorial-conclusion
• First Catalog Sources Not in the Second Catalog
• Some statistical trends and distributions

April 26, 2013 ============== Support for Apogee's preflash option is being added to help remove the latent bulk image artifact that is present in images on Kodak sensors when they have been exposed to a bright infrared source. The effectiveness of this hardware feature is being assessed. ... The support will appear in test variants after version 4.1 and should not be used for critical photometry until we have the camera performance in this mode fully analyzed. ...

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• Shared Skies Photo Gallery

To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...

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• astro-ph

. Album : Фотоальбом Сергея Аюкова :: Travels to distant places and countries :: 1997/08 Japan (Kyoto, Nara) :: 17/08 Kyoto streets. Maruyama park . Up . << Prev . Dreaming about things on display. After checking, they appeared to be not that tasty compared to how they look. Next >> . Created with the tool album generator from David's MarginalHacks on Wed Jun 5 20:38:34 2013 .

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• COMPLEX DATA ANALYSIS

SPECTRAL FEATURES OF THE AVALANCHE DEPOSITS IN LUNAR CRATER REINER. ... Crater Reiner. ... 5 Immature soils (coded in green, box 3) occupy most areas of the inner wall slopes of the crater. ... Distribution of the immature soils shown in Fig. 5 correlates with distribution of the bright materials on the wall slope of the crater as it is seen in Fig. ... The presence of very immature soils on the inner wall slopes and on the central peak of the crater Reiner suggests recent intensive slope processes. ...

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• http://selena.sai.msu.ru/Pug/Publications/ms34/MS058.pdf
• http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf
• Бережной А.А.

... Telescopes · Binoculars · Microscopes . Meade Ultra-High Transmission coatings (UHTC ) Group . ... Meade Standard Coatings: The optical surfaces of all Meade telescopes include high-grade optical coatings fully consistent in quality with the precision of the optical surfaces themselves. ... These specialized, and extremely advantageous, coatings are offered here as the Meade Ultra-High Transmission Coatings (UHTC) group, a coatings group available optionally on many Meade telescope models. ...

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• Meade Series 4000 Broadband Nebular Filters
• Meade Instruments Corporation - Pictor Manual Part 2
• Meade Instruments Corporation - Pictor Manual Parts 19 and 20

... Submitted by Joseph Kristl on 01/22/2007 11:11:43 . ... 16:54:59 local 1/100 sec, f/5.6, ISO 400, fl = 400 mm . While Venus appeared somewhat brighter, it was much higher and thus in a considerably darker sky (and not through thin clouds). My impression at the time was that the comet was brighter than Venus (using calibrated eyeballs.. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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• Mars pictures from Stellafane by Paul Valleli

... One striking feature is a small source of almost pure H 2 line emission, which is located near one of the compact sources in Orion reported by O'Dell and collaborators (HST-18 = 203-504). ... H-H objects, Proplyds, Orion Bar, H 2 . ... We obtained a series of images across the bright rim of the Orion Bar near the peaks of mm-wave molecular line emission with NICMOS cameras 1-3 (NIC1, NIC2, NIC3) in several filters on 1998 February 18. ... The suggestion of an H-H object does not seem compelling. ...

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• The Formation and Evolution of LMC Rich Star Clusters: NGC 1818
• HST/NICMOS Observations of the Interacting System Arp 299
• Some Experiments with the Restoration of NICMOS Camera 2 Images of OMC-1

... F. A. Primini, and H. E. Payne, eds. Pro jective Transform Techniques to Reconstruct the 3-D Structure and the Temp oral Evolution of Solar Polar Plumes A. Llebaria, A. Thernisien, P. Lamy Laboratoire d'Astronomie Spatiale (CNRS) Marseil le Abstract. ... For each pole, the plumes seem to diverge from a virtual point located on the polar axis not far from the solar surface. ... What are polar plumes? ... Plume images (left) and correlative picks in the dual plane(right). ... Inaccurate exposure times...

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• Projective Transform Techniques to Reconstruct the 3-D Structure and the
• Refining the Guide Star Catalog: Plate Evaluations
• Titan Image Processing

... Circumstellar disc of beta Pictoris: constraints on grain properties from polarization. To appear in the Astronomy & Astrophysics . abs , src , ps ] . ... Dust influx to Titan from Hyperion . ... abs ] . ... Characteristics of bulges and disks in interacting galaxies . ... Dust grains around Herbig Ae/Be stars: porous, cometary-like grains? ... To appear in the Astronomy & Astrophysics Supplement . ... Finally, Links may lead you to more options (e.g. via the LANL preprint system). ...

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• Optical properties of cosmic dust analogs
• Database of Optical Properties -- Level: subsubpage

... MASTER Net is 56 square degrees per 1 exposition . ... 06 Dec 2015: GRB 151205B: MASTER-NET early optical observations GCN18665 . ... 18 Nov 2015: GRB 151118A: MASTER-NET optical observations GCN18613 . ... 12 Nov 2015: GRB 151112A: MASTER-NET optical limit GCN18591 . ... 07 Nov 2015: GRB 151107A: MASTER-NET optical observations GCN18565 . ... 31 Oct 2015: Five OTs detected by Global Robotic MASTER Net ATel8232 . ... 02 Oct 2015: GRB 151001B: MASTER-NET early optical observations GCN18380 . ...

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July 19, 1998 . ... An example of the EUV large-scale chain revealed by the modified TRACE EUV images. The TRACE EUV (171 A) image of July 19, 1998 with a number of complicated chains and threads. In particular, an "8"-like structure appear to be present at the central area of the disc restricted by points 1-2-3-4. Some fragments of this structure consist of the two parallel threads. ... Back to the page of the TRACE chains . Back to the parent page . Last update: 9 August 1998 . ...

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• http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/desc.htm
• http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/960522.htm
• http://www.izmiran.rssi.ru/~ichertok/CHAINS/ANNOUNC/980407.htm

The Experiment: To find the first galaxies . Understand basic properties of star formation/galaxies ? guess how a young galaxy, or protogalaxy would appear . ... New stars very blue: will appear redder at large distances (redshift). Dust protects gas from radiation. Dust is heated and is luminous at infrared wavelengths. ... Gas in close to a group of galaxies (cluster) may become very hot and emit X-rays. Previous slide . Next slide . Back to first slide . ...

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• Measurements of anisotropies in the Cosmic Microwave Background Radiation on
• Bojan Nikolic -- 90 GHz Continuum Observations of Messier 66
• G315.4-2.3

THE OPTICAL COUNTERPART TO IGR J11435-6109 Є Є Jose M. Torrejon and I. Negueruela Departamento de FЄ isica, IngenierЄ de Sistemas y TeorЄ de la Senal , Universidad de Alicante, E-03080 Alicante, Spain ia ia ~ jmt@dfists.ua.es ABSTRACT We present photometry and spectroscopy of the possible optical counterparts to the INTEGRAL source IGR J11435-6109. We show that the object within the ROSAT error circle is an M type star and is not related with the INTEGRAL source. ... Key words: X-ray binaries. ...

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• http://hea.iki.rssi.ru/integral06/papers/D06_Forman01-07Mar07_05:08:00.pdf
• http://hea.iki.rssi.ru/integral06/papers/I06_Castro-Tirado01-16May07_19:00:26.pdf

... Since moonshine is really reflected sunlight, the full Moon is on the average slightly brighter in mid-winter, when Earth is closest to the Sun. In addition, the distance of the full Moon also varies, due to the ellipticity ("eccentricity") of the Moon's orbit. On 22 December, 1999, the two effects combined to produce the brightest full Moon of the century. ... This year will be the first full moon to occur on the winter solstice, Dec. 22nd, commonly called the first day of winter. ...

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• Solar Energetic Particles
• The Many Colors of Sunlight
• The Celestial Sphere--lesson plan #1a

... The function is accessible, if the file with the image is open, and Ю identification of a star field is made. ... a) Load a first image by the command " Open ", and others by the command " Open +". b) Make an identification of the field. c) Open the menu " File ", select " Next " or press . ... It is necessary tree or more images. a) Load the first image by the command " Open" , and others by the command " Open + ". b) Open the menu " Marking ", select "Detect moving objects" or press - . ...

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Next: Ejectors in Massive Binary Previous: Artificial Galaxy: Full Matrix . The first version of the Scenario Machine was aimed especially at the simulation of massive binary star evolution. ... First, there is a large class of intermediate mass binaries (say, consisting initially of 8 + 5 solar masses) that can also produce NS and thus lead to the formation of a bright X-ray source. ... Next: Ejectors in Massive Binary Previous: Artificial Galaxy: Full Matrix Mike E. Prokhorov . ...

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• Physicists on the Money
• Brightness constraint
• The Radiopulsar PSRB1259-63?- a Probe in the Stellar Wind Plasma

... The Russian TESIS/ CORONAS-PHOTON Solar Observatory, which has been working in orbit since January 30th, 2009, has photographed one of the most important events in the build up to the upcoming solar cycle - the formation of our star's new southern belt of activity. The first magnetic fields of the new cycle in the southern hemisphere appeared on the Sun's surface on May 23-24th. ... The belt of activity is one of the primary concepts, characterizing the solar cycle. ...

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• Project's diary
• Solar activity hits a new low
• This year's largest group of sunspots passes across the solar disk