Characterizing the satellites of massive galaxies up to z ∼ 2: young populations to build the outskirts of nearby massive galaxies

The accretion of minor satellites is currently proposed as the most likely mechanism to explain the significant size evolution of the massive galaxies during the last ∼10 Gyr. In this paper, we investigate the rest-frame colours and the average stellar ages of satellites found around massive galaxies (M_star ∼ 10^11 M_⊙) since z ∼ 2. We find that the satellites have bluer colours than their central galaxies. When exploring the stellar ages of the galaxies, we find that the satellites have similar ages to the massive galaxies that host them at high redshifts, while at lower redshifts they are, on average, ≳1.5 Gyr younger. If our satellite galaxies create the envelope of nearby massive galaxies, our results would be compatible with the idea that the outskirts of those galaxies are slightly younger, metal-poorer and with lower [α/Fe] abundance ratios than their inner regions.

Testing diagnostics of nuclear activity and star formation in galaxies at z > 1

We present some of the first science data with the new Keck/MOSFIRE instrument to test the effectiveness of different AGN/SF diagnostics at z ~ 1.5. MOSFIRE spectra were obtained in three H-band multi-slit masks in the GOODS-S field, resulting in 2 hr exposures of 36 emission-line galaxies. We compare X-ray data with the traditional emission-line ratio diagnostics and the alternative mass-excitation and color-excitation diagrams, combining new MOSFIRE infrared data with previous HST/WFC3 infrared spectra (from the 3D-HST survey) and multiwavelength photometry. We demonstrate that a high [O III]/Hβ ratio is insufficient as an active galactic nucleus (AGN) indicator at z > 1. For the four X-ray-detected galaxies, the classic diagnostics ([O III]/Hβ versus [N II]/Hα and [S II]/Hα) remain consistent with X-ray AGN/SF classification. The X-ray data also suggest that "composite" galaxies (with intermediate AGN/SF classification) host bona fide AGNs. Nearly ~2/3 of the z ~ 1.5 emission-line galaxies have nuclear activity detected by either X-rays or the classic diagnostics. Compared to the X-ray and line ratio classifications, the mass-excitation method remains effective at z > 1, but we show that the color-excitation method requires a new calibration to successfully identify AGNs at these redshifts.

The evolutionary paths among galaxy types on the red sequence at 0.3 < Z < 1.5

We have studied the main evolutionary paths among the galaxy types residing on the massive end of the Red Sequence and nearby locations on the Green Valley during the last ∼9 Gyr. The morphological and star formation properties of a sample of these galaxies at 0 . 3 < z < 1 .5 with stellar masses M_∗ > 5 × 10^10 M_⊙ have been analysed. We present direct observational evidence for the first time of the existence of two main evolutionary paths among the different red galaxy types since z ∼ 1 .5, which provide some clues on the nature of the processes that have governed the assembly of present-day massive quiescent galaxies. The results are in excellent agreement with the hierarchical evolutionary framework proposed in the Eliche-Moral et al. (2010) model. Data from SHARDS (one of the ESO/GTC Large Programmes approved in 2009A) will complement and improve the present findings, shedding some light into many of the still unsettled questions concerning the migration of galaxies from the Blue Cloud to the Red Sequence at z < 1 .5.

Determinação do contorno pulmonar orientado em sequências temporais de imagens de RM pela transformada de Hough.

O estudo do movimento pulmonar é assunto de grande interesse na área médica. A observação direta do mesmo é inviável, uma vez que o pulmão colapsa quando a caixa torácica é aberta. Dentre os meios de observação indireta, escolheu-se o imageamento por ressonância magnética em respiração livre e sem uso de nenhum gás para melhorar o contraste ou qualquer informação de sincronismo. Esta escolha propõe diversos desafios, como: a superar a alta variação na qualidade das imagens, que é baixa, em geral, e a suscetibilidade a artefatos, entre outras limitações a serem superadas. Imagens de Tomografia Computadorizada apresentam melhor qualidade e menor tempo de aquisição, mas expõem o paciente a níveis consideráveis de radiação ionizante. É apresentada uma metodologia para segmentação do pulmão, produzindo um conjunto de pontos coordenados. Isto é feito através do processamento temporal da sequência de imagens de RM. Este processamento consiste nas seguintes etapas: geração de imagens temporais (2DSTI), transformada de Hough modificada, algoritmo de contornos ativos e geração de silhueta. A partir de um dado ponto, denominado centro de rotação, são geradas diversas imagens temporais com orientações variadas. É proposta uma formulação modificada da transformada de Hough para determinar curvas parametrizadas que sejam síncronas ao movimento diafragmático, chamados movimentos respiratórios. Também são utilizadas máscaras para delimitar o domínio de aplicação da transformada de Hough. São obtidos movimentos respiratórios que são suavizados pelo algoritmo de contornos ativos e, assim, permitem a geração de contornos para cada quadro pertencente a sequência e, portanto, de uma silhueta do pulmão para cada sequência.

Art influences on Mark Z. Danielewski's House of Leaves and Los Angeles's influence on Johnny Truant

"...is a novel that combines literature and art to create a unique postmodern object. It was published just over a decade ago, and in that time numerous scholars and students have written papers and articles on it. Within these articles, the themes are usually about deconstruction, the house as a digital object, the house's lack of homeliness, or characters who claim authorial presence. Danielewski distance himself from that role. The house and its impossible labyrinth are the central feature of the book. A house should provide stability, but this house shifts its rooms and walls at random. A house should protect its occupants, but this one kills people. This house links itself into an infinite amount of information through its use of the internet as an influence and a stylistic device, but it has nothing but an absence in its very foundation, an empty labyrinth with an unseen monster."

Weighted composition operators on the predual and dual Banach spaces of Beurling algebras on Z

Let vv be a weight sequence on ZZ and let ψ,φψ,φ be complex-valued functions on ZZ such that φ(Z)⊂Zφ(Z)⊂Z. In this paper we study the boundedness, compactness and weak compactness of weighted composition operators Cψ,φCψ,φ on predual Banach spaces c0(Z,1/v)c0(Z,1/v) and dual Banach spaces ℓ∞(Z,1/v)ℓ∞(Z,1/v) of Beurling algebras ℓ1(Z,v)ℓ1(Z,v).

On the Analytic Solutions of the Functional Equations w 1 f(a 1 z) + w 2 f(a 2 z) + ... + w n f(a n z) = 0

In this paper, it is showed that, given an integer number n ≥ 2, each zero of an exponential polynomial of the form w1az1+w2az2+⋯+wnazn, with non-null complex numbers w 1,w 2,…,w n and a 1,a 2,…,a n , produces analytic solutions of the functional equation w 1 f(a 1 z) + w 2 f(a 2 z) + ... + w n f(a n z) = 0 on certain domains of C, which represents an extension of some existing results in the literature on this functional equation for the case of positive coefficients a j and w j.

Catalog of type and referred specimens of fossil ostracodes in the Field Museum of Natural History / [by] Matthew H. Nitecki -- and Diana Z. Handler --.

v.17:no.5(1968)

Aleutian islanders; Eskimos of the north Pacific / by George I. Quimby, Curator of Exhibits, Dept. of Anthropology. Drawings by Helen Z. Quimby.

no.35(1944)

Letters from Z.W. Nixon to William Tudor,

Four letters regarding the legal and financial aspects involving the Chanca silver mine and its stakeholders, Tudor, McCall, Maling, and Prevost, and a copy of a letter from Nixon to Prevost. Nixon additionally comments on domestic news, including the renaming of the U.S.S. Susquehanna as the U.S.S. Brandywine by John Quincy Adams in honor of the Marquis de Lafayette. The ship conveyed Lafayette back to France after his tour of the United States. Nixon also mentions Charles Stewart and his court martial.

Talfīq al-akhbār wa-talqīḥ al-āthār fī waqāʻiʻ Qāzān wa-Bulghār wa-mulūk al-Tatār

athar M. M. al-Ramzī.

Tashīl al-majāz ilá fann al-muʻammá wa-al-alghāz

jamʻ Ṭāhir al-Jazāʼirī.

Ṭirāz al-majālis

li-Shihāb al-Dīn Aḥmad ibn Muḥammad al-Khafājī.

Kitāb Bahjat al-asrār wa-maʻdan al-anwār fī baʻḍ manāqib al-quṭb al-Rabbānī wa-al-ghawth al-Ṣamadānī wa-al-baḥr al-zākhir al-nūrānī ṣāḥib al-maqām al-ʻalī Muḥyī al-Dīn Abī Muḥammad ʻAbd al-Qādir al-Jīlī

taʼlīf Nūr al-Dīn Abī al-Ḥasan ʻAlī ibn Yūsuf Abī Faḍl al-Shaṭnūbī. Wa-bi-hāmishihi Kitāb Riyāḍ al-basātīn fī akhbār al-Shaykh ʻAbd al-Qādir al-Jīlī Muḥyī al-Dīn taʼlīf Muḥammad al-Amīn al-Kīlānī al-Tūnisī.

Risālah fī al-ʻamal bi-rubʻ al-dāyirah al-ālah al-maʻrūfah / taʼlīf al-Shaykh al-Imām al-ʻAllāmah ʻIzz al-Dīn ʻAbd al-ʻAzīz ibn Muḥammad al-Wafāʼī al-Muwaqqit bi-Jāmiʻ al-Muʼayyad : manuscript, 1673

Unbound.