The Dark Fields Pdf

[Armonia Bunda]

Nopestill getting leeching bolts if i stand anywhere near a different field, even if i'm standing dead center on the ice field. I tried this with other fields like poison from CPC and it also overrides it. Curiously enough GS4 doesn't actualy take priority, which is good since it expands, but this sure as hell messes with my positioning since you want to be inside the target's hitbox for maximum effectiveness, so staying away from the dark field is not an option.

According to the SC rotation, you are not meant to overlap fields on condi Reaper; you have to wait for each field to expire before applying the next. Even with it comes to Chilling Darkness + Deathly Chill combo, you never apply both Nightfall and Well of Darkness as you would lose a lot of potential bleed application due to the 3s ICD of Chilling Darkness. Usually if you're in Shroud while you have a pre-existing field going, you auto attack until it dissipates and then you apply the RS5+RS4 combo.

Still, even if i did my unga bunga rotation wrong this is tbh a new thing, ice field always gave me chilling bolts no matter what was over or under it, is all i'm saying, like not trying to improve my rotation here just pointing out a bug.

Alexander Gardner created dramatic and vivid photographs of battlefields, which included images of the recently dead. These shocking Civil War-era images continue to haunt the national imagination. After the war, Gardner went west, creating unforgettable pictures of western landscape and portraits of American Indians.

Also included in "Dark Fields of the Republic" are Gardner's portraits of President Abraham Lincoln and other leading figures, both military and civilian. His best-known work, the museum's "cracked-plate" photograph of Lincoln, will be on view for this exhibition. The sitting on Feb. 5, 1865, took place mere weeks before Lincoln's assassination in April. The glass plate cracked, and Gardner created only one print before throwing the plate away.

The show also documents the course of American expansion as settlers moved westward after the war and includes landscapes and portraits of American Indians. Gardner's landscapes, with their sense of almost limitless horizons, juxtaposed with his detailed portraits of Indian chiefs and tribal delegations, have a haunting specificity and gravity. The exhibition is curated by David C. Ward, Portrait Gallery senior historian, with guest curator Heather Shannon, former photo archivist at the Smithsonian's National Museum of the American Indian, and research assistance from Sarah Campbell.

"Dark Fields of the Republic: Alexander Gardner Photographs, 1859-1872" is funded by members of the exhibition's leadership committee. The co-chairs for this philanthropic committee are gratefully acknowledged: The Abraham and Virginia Weiss Charitable Trust, Amy and Marc Meadows, in honor of Wendy Wick Reaves; The Stoneridge Fund of Amy and Marc Meadows; The Abraham Lincoln Bicentennial Foundation; Peter and Rhondda Grant; Mr. and Mrs. Robert Uhler; and Kate Kelly and George Schweitzer.

"Those with an interest in the Civil War, and Lincoln, will find the show thoroughly absorbing, but it is far more than a Civil War exhibition. Curator David Ward is sketching a larger picture of America in the late 19th century, a country transformed by war, disillusioned yet ambitious, moving seamlessly from internecine strife to genocidal violence against its native population."

With launch scheduled in 2022, ESA's Euclid mission is making great progress on both the hardware and the science preparations. Once in space, Euclid will survey a significant portion of the sky and image billions of galaxies across the Universe to investigate the past ten billion years of our cosmic history.

The observations will enable scientists to investigate two cosmological phenomena: the evolution of how galaxies cluster together over the past 10 billion years, and the distortion of galaxy images due to the presence of ordinary and dark matter intervening between them and us, an effect called gravitational lensing. These two phenomena address the mission's key science goal: delving into the history of the Universe's expansion and characterising the acceleration of this expansion during the last few billion years, something that is thought to be caused by the mysterious dark energy.

With a cumulative area of 40 square degrees, equivalent to just over 200 times the footprint of the full Moon in the sky, the Euclid Deep Fields span a portion of the celestial sphere that, while much smaller than the mission's wide survey, is still quite remarkable for a deep survey.

"The choice of the Euclid Deep Fields has been a complex process because of many instrumental and scientific constraints, and we are very pleased with this solution that was recently approved by the Euclid scientific community," said Roberto Scaramella from the National Institute for Astrophysics in Italy, Euclid Survey Scientist and lead of the Euclid Consortium Survey Group.

The selection of the fields was presented on 4 June during the annual meeting of the Euclid Consortium, which is led by Yannick Mellier of Institute d'Astrophysique in Paris, France, and comprises 1500 scientists from across Europe, the US and Canada.

One of the three fields, the Euclid Deep Field North, with an area of 10 square degrees, is located very close to the Northern Ecliptic Pole, in the constellation Draco, the dragon. The proximity to the ecliptic pole ensures maximum coverage throughout the year; the exact position was chosen to obtain maximum overlap with one of the deep fields surveyed by NASA's infrared workhorse, the Spitzer Space Telescope.

The other two fields are located in the southern sky. The challenge entailed selecting a region as close as possible to the Southern Ecliptic Pole, which would provide the best coverage, while at the same time avoiding bright sources in that area, which is home to the Large Magellanic Cloud, one of the galactic neighbours of our Milky Way.

The Euclid Deep Field Fornax, also spanning 10 square degrees, is located in the southern constellation Fornax, the furnace. It encompasses the much smaller Chandra Deep Field South, a 0.11 square degree region of the sky that has been extensively surveyed in the past couple of decades with NASA's Chandra and ESA's XMM-Newton X-ray observatories, as well as the NASA/ESA Hubble Space Telescope and major ground-based telescopes.

The third and largest of the fields is the Euclid Deep Field South, covering 20 square degrees in the southern constellation of Horologium, the pendulum clock. This was the most complex of the three to select because of various technical reasons, also taking into account the capabilities of future ground-based wide field telescopes like the Large Synoptic Survey Telescope. This field has not been covered to date by any deep sky survey and so has a huge potential for new, exciting discoveries.

"We are convinced that the Euclid Deep Fields will become a preferred target in future years for multi-wavelength observations by many telescopes on ground and in space, and hopefully will become as useful and renowned as other famous deep fields surveyed in the past," adds Scaramella.

As opposed to the roughly 30 000 single-visit observations that are needed to cover the Euclid wide survey, each targeting a field slightly apart from the other and with only minimal overlap, the satellite will pay multiple visits to the Euclid Deep Fields. Each field deep field is observed at least 40 times to uncover sources up to two magnitudes fainter than in the wide survey.

The Euclid deep survey has a twofold function: while, on one hand, it provides an accurate data set to validate the main cosmological analysis based on the wide survey, on the other, returning to the same portions of the sky numerous times is also essential for stability monitoring and calibration purposes throughout the course of the mission.

The three deep fields provide a window to examine large amounts of galaxies, looking back to the epoch when the first stars and galaxies formed, which occurred in the first billion year of the Universe's history. Due to cosmic expansion, the light emitted by these galaxies is redshifted to the infrared, so they are best detected at infrared wavelengths, which are poorly accessible from the ground due to Earth's atmosphere. Obtaining data comparable to Euclid's deep survey from the ground would require several tens of years of continuous observing time from the best near-infrared facilities.

Together, the relatively large cumulative area of 40 square degrees, the depth of the survey and Euclid's imaging and spectroscopic capabilities in the infrared maximises the chances of discoveries from the deep survey. The survey will detect several hundred thousand galaxies per square degree; in the case of the most distant sources (with redshift greater than six, corresponding to cosmic epochs when the Universe was less than one billion years old) estimates of the detection rate vary between a few tens to at most a few hundreds of sources per square degree, with the uncertainty being so high due to poor statistics from existing observational data. This will change with Euclid, which can survey an area of this size in a much shorter time than would be needed by Hubble or even the future NASA/ESA/CSA James Webb Space Telescope.

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