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English version - Richard de Grijs
English version - Richard de Grijs

... of this fascinating new phenomenon will be found. Catching another intermittent pulsar in its ON mode is up to chance. Is there another candidate out there ready to reveal its secrets, or will it forever lurk hidden in the dark unknowns of space? Lyne hopes that follow-up measurements of PSR J192 ...
Semester 2016B - Gran Telescopio CANARIAS
Semester 2016B - Gran Telescopio CANARIAS

FOE 2017 Poster Contributions - College of Science | Oregon State
FOE 2017 Poster Contributions - College of Science | Oregon State

... Title: GRBs as redshift estimators via a machine learning approach Abstract: DeWe propose an alternative technique based on the semi-parametric generalized additive model, GAM (Hastie & Tibshirani 1986). GAM allows to represent the relationship as the sum of smooth functions including very few predi ...
ASI 2017 Abstract Book - Astronomical Society of India
ASI 2017 Abstract Book - Astronomical Society of India

... One of the most outstanding challenges in extragalactic astronomy is to identify the astrophysical processes responsible for transforming simple dark matter haloes into the heterogenous population of galaxies inhabiting today's Universe. How did different morphological types form and evolve? Does th ...
Missions
Missions

... All types of light are ‘electromagnetic radiation’. Electromagnetic radiation propagates through space as a wave. Although this wave always travels at the same speed in a vacuum (the famous speed of light, 300 000 kilometres per second), some of its characteristics vary depending on its energy. Ultr ...
Estimating the Cost of Extremely Large Telescopes
Estimating the Cost of Extremely Large Telescopes

... The Keck telescopes provide a recent example of how radical design innovations can "break the cost curve." A comparison with the Mayall 4-m telescope at Kitt Peak National Observatory (KPNO) illustrates the point dramatically. The Mayall telescope was completed in 1973 at a cost of $10.65 million. B ...
The first focused hard X-ray images of the sun with
The first focused hard X-ray images of the sun with

... limited by thermal motions in the spacecraft itself. This results in a point source reconstructed using a certain combination of star trackers to appear to be shifted by an arcminute or two in R.A./decl. coordinates compared to the same point source reconstructed using a different combination of sta ...
Transparencies - Rencontres de Moriond
Transparencies - Rencontres de Moriond

... • The LSST Telescope and Camera • Dark Energy Science • Schedule and Plans ...
The Hubble Space Telescope Optical Systems Failure Report
The Hubble Space Telescope Optical Systems Failure Report

... The rough grinding operation for the Hubble Space Telescope began in December 1978, at the Perkin-Elmer Corporation, in Wilton, Connecticut. The mirror was then transferred to Perkin-Elmer in Danbury, Connecticut, now Hughes Danbury Optical Systems, Inc. (HDOS), where polishing was completed in Apr ...
The Hubble Space Telescope Optical Systems Failure Report
The Hubble Space Telescope Optical Systems Failure Report

... The rough grinding operation for the Hubble Space Telescope began in December 1978, at the Perkin-Elmer Corporation, in Wilton, Connecticut. The mirror was then transferred to Perkin-Elmer in Danbury, Connecticut, now Hughes Danbury Optical Systems, Inc. (HDOS), where polishing was completed in Apr ...
FPU Subunits
FPU Subunits

... no major deviation of grating profile from spec PACS FPU Subunits ...
120 Inch Telescope Aluminizing 2-7-06
120 Inch Telescope Aluminizing 2-7-06

... 37. Raise flange till flush with mirror cell; using screwdriver rotate slotted studs (3) to engage clamps with outer diameter of hole and tighten with 15/16 inch open end wrench. (47-b) ...
Manufacture of a 1.7 m prototype of the GMT primary mirror segments
Manufacture of a 1.7 m prototype of the GMT primary mirror segments

... The aspheric surface was generated to an accuracy of about 15 µm rms by ITT Industries. Loose-abrasive grinding and polishing were performed by the Mirror Lab. We polished the mirror primarily using a 30 cm diameter stressed lap, essentially the same system used to polish the 1.8 m f/1 primary mirro ...
$doc.title

... Remote  access  to  digital  sky  survey  (DSS)  images  is  integrated  into  FACSUM  and  downloaded  images  may   be  displayed  directly  in  DS9  (providing  on  the  fly  finder  charts).      The  JSkyCalc  program  written  b ...
ESA BR-170 - ESA Science
ESA BR-170 - ESA Science

Shearer et al Observations of Fermi Pulsars 2009-10
Shearer et al Observations of Fermi Pulsars 2009-10

The Ages of Astrophotography - Powered by Catchers of the Light
The Ages of Astrophotography - Powered by Catchers of the Light

... “The process of M. Daguerre is much more sensitive to the action of light than those which had been used so far. Never before has natural moonlight produced any perceptible physical effect, even when magnified with the largest lens, or focused by the biggest reflective mirror. The plates prepared by ...
Telescope Web Sites
Telescope Web Sites

Document
Document

... De-spaceing of the HST secondary mirror along the telescope optical axis from (orbit driven) thermal instabilities in the OTA causes variations in the PSF structures which are typically THE dominant source of systmatic errors in coronagraphic PSF subtraction. The thermal time constant of the OTA is ...
Comprehensive search for natural satellites of Vesta by the Dawn
Comprehensive search for natural satellites of Vesta by the Dawn

History of the Telescope
History of the Telescope

... main axes around which it rotates, is elevated against the horizon in such a way, that its angle equals the polar altitude and is pointing at the pole. The second axis, named the declination axis, is mounted on the hour axis exactly vertical (at right angle). If the telescope, mounted in this way, i ...
Lab 6 - College of San Mateo
Lab 6 - College of San Mateo

... 6. Keeping the telescope fixed in position, rotate the prism table platform until light from the slit reflects from the OTHER side of the prism adjoining the apex angle A. As in the previous step, place the image precisely on the intersection of the crosshairs. Read THE SAME window as in the previou ...
1985e - Astrophotography with small telescopes
1985e - Astrophotography with small telescopes

... This weekend had been a tiring but refreshing one at the Riverside Telescope Don at the comet discovery site Maker's Conference at Camp Oakes, near on the morning of the discovery. Big Bear City in southern California. Over 1300 individuals had attended the Memorial Day Weekend gathering, held every ...
ASTRONOMIA SPAIN inglés.qxd
ASTRONOMIA SPAIN inglés.qxd

... These are some of the results we present in ‘Astronomy made in Spain’, a project of the Spanish Astronomical Society (Sociedad Española de Astronomía, SEA) to commemorate the International Year of Astronomy 2009. This book is a collection of conversations with the Spanish astronomers who have publis ...
LARRY MARSCHALL CLEA
LARRY MARSCHALL CLEA

... •Modern digital data and analysis techniques, using, wherever possible, real data. •Modular: each module includes software, student ...
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XMM-Newton



The XMM-Newton, also known as the X-ray Multi-Mirror Mission and the High Throughput X-ray Spectroscopy Mission, is an orbiting X-ray observatory launched by ESA in December 1999 on an Ariane 5 rocket. It is named in honor of Sir Isaac Newton. The telescope was placed in a very eccentric 48 hour elliptical orbit at 40°; at its apogee it is nearly 114,000 kilometres (71,000 mi) from Earth, while the perigee is only 7,000 kilometres (4,300 mi).
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