The Right to Privacy

Warren, S. Hazzledine; Brandeis, Louis D.

doi:10.7312/gold91730-002

Cited by 26 publications

(19 citation statements)

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“…Cirasuolo et al (2007) have measured the evolution of the K ‐band galaxy luminosity function to z ≃ 2. The coolest known brown dwarf (classified T8.5) has been found by Warren et al (2007c; spectrum shown in Warren et al 2006). Lodieu et al (2007) have found 129 new brown dwarfs, a significant fraction of the total known, including a dozen below 20 Jupiter masses.…”

Section: Survey Progressmentioning

confidence: 99%

The UKIRT Infrared Deep Sky Survey (UKIDSS)

Lawrence

Warren

Almaini

et al. 2007

Monthly Notices of the Royal Astronomical Society

2,285

2,106

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Final published version including significant revisions. Twenty four pages, fourteen figures. Original version April 2006; final version published in MNRAS August 2007We describe the goals, design, implementation, and initial progress of the UKIRT Infrared Deep Sky Survey (UKIDSS), a seven year sky survey which began in May 2005, using the UKIRT Wide Field Camera. It is a portfolio of five survey components covering various combinations of the filter set ZYJHK and H_2. The Large Area Survey, the Galactic Clusters Survey, and the Galactic Plane Survey cover approximately 7000 square degrees to a depth of K~18; the Deep Extragalactic Survey covers 35 square degrees to K~21, and the Ultra Deep Survey covers 0.77 square degrees to K~23. Summed together UKIDSS is 12 times larger in effective volume than the 2MASS survey. The prime aim of UKIDSS is to provide a long term astronomical legacy database; the design is however driven by a series of specific goals -- for example to find the nearest and faintest sub-stellar objects; to discover Population II brown dwarfs, if they exist; to determine the substellar mass function; to break the z=7 quasar barrier; to determine the epoch of re-ionisation; to measure the growth of structure from z=3 to the present day; to determine the epoch of spheroid formation; and to map the Milky Way through the dust, to several kpc. The survey data are being uniformly processed, and released in stages through the WFCAM Science Archive (WSA : http://surveys.roe.ac.uk/wsa). Before the formal survey began, UKIRT and the UKIDSS consortium collaborated in obtaining and analysing a series of small science verification (SV) projects to complete the commissioning of the camera. We show some results from these SV projects in order to demonstrate the likely power of the eventual complete survey. Finally, using the data from the First Data Release we assess how well UKIDSS is meeting its design targets so far

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Section: Survey Progressmentioning

confidence: 99%

The UKIRT Infrared Deep Sky Survey (UKIDSS)

Lawrence

Warren

Almaini

et al. 2007

Monthly Notices of the Royal Astronomical Society

2,285

2,106

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“…Press & Schechter () or Sheth, Mo & Tormen (), and/or the analytical fits of numerical simulations (e.g. Warren et al ). In this scenario, an M ≃ 10 13 M ⊙ halo is becoming ‘typical’ on an ∼10 Mpc scale (the typical linear size of a large galaxy cluster) at redshifts below z ∼ 5, which is compatible with the collapsing redshift of our HDHM model (see below).…”

Section: Input Physics Of the Nb‐tsph Model Galaxiesmentioning

confidence: 99%

Formation and evolution of early-type galaxies – III. Dependence of the star formation history on the total mass and initial overdensity

Merlin

Chiosi

Piovan

et al. 2012

Monthly Notices of the Royal Astronomical Society

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We investigate the influence of the initial overdensities and masses of proto‐galaxies on their subsequent evolution (the star formation history in particular) to understand whether these key parameters are sufficient to account for the varied properties of the galactic populations. By means of fully hydrodynamical N‐body simulations performed with the code EvoL, we produce 12 self‐similar models of early‐type galaxies of different initial masses and overdensities, and follow their evolution from the early epochs (detachment from the linear regime and Hubble flow at z ≥ 20) down to the stage when mass assembly is complete, i.e. z ≤ 1 (in some cases the models are calculated up to z = 0). The simulations include radiative cooling, star formation, stellar energy feedback, re‐ionizing photo‐heating background and chemical enrichment of the interstellar medium; we do not consider the possible presence of active nuclei. We find a strong correlation between the initial properties of the proto‐haloes and their subsequent star formation histories. Massive (Mtot ≃ 1013 M⊙) haloes experience a single, intense burst of star formation (with rates ≥103 M⊙ yr−1) at early epochs, consistently with observations, with less pronounced dependence on the initial overdensity; intermediate‐mass (Mtot ≃ 1011 M⊙) haloes have histories that strongly depend on their initial overdensity, whereas low‐mass haloes (Mtot ≃ 109 M⊙) always have erratic, bursting like star‐forming histories, due to the ‘galactic breathing’ phenomenon. The model galaxies have morphological, structural and chemical properties resembling those of real galaxies, even though some disagreement still occurs, likely a consequence of some numerical choices. We conclude that total mass and initial overdensity drive the star formation histories of early‐type galaxies. The model galaxies belong to the so‐called quasi‐monolithic (or early hierarchical) scenario in the sense that the aggregation of lumps of dark and baryonic matter is completed very early on in their history. In this picture, nature seems to play the dominant role, whereas nurture has a secondary importance.

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“…They argued that the law should protect not only the confidential relationships between people, but also prevent disclosure of information to the wider public [7]. One of their reasons for this conclusion was that the law of confidence did not provide enough protection in a world where technological advances allowed a photographer to take a picture and publish it without the subject's knowledge or consent [8]. The law should not only protect close relationships, but also protect people ''as against the world'' [9].…”

Section: Legal Considerationsmentioning

confidence: 93%

Balancing between two goods: Health Insurance Portability and Accountability Act and ethical compliancy considerations for privacy-sensitive materials in health sciences archival and historical special collections

Wiener¹,

Gilliland²

2011

J Med Libr Assoc

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With thoughtful planning, it is possible to balance the integrity of and access to the historical record of sensitive documents, while supporting the privacy protections of HIPAA and professional ethical standards. Although it is theorized that collection development policies of institutions have changed due to HIPAA legislation, additional research is suggested to see how various legal interpretations have affected the integrity of the historical record in actuality.

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The Right to Privacy

Cited by 26 publications

References 0 publications

The UKIRT Infrared Deep Sky Survey (UKIDSS)

The UKIRT Infrared Deep Sky Survey (UKIDSS)

Formation and evolution of early-type galaxies – III. Dependence of the star formation history on the total mass and initial overdensity

Balancing between two goods: Health Insurance Portability and Accountability Act and ethical compliancy considerations for privacy-sensitive materials in health sciences archival and historical special collections

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