Titlebook: Deep Fields; Proceedings of the E Stefano Cristiani,Alvio Renzini,Robert E. Williams Conference proceedings 2001 Springer-Verlag Berlin Hei

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書目名稱Deep Fields影響因子(影響力)




書目名稱Deep Fields影響因子(影響力)學(xué)科排名




書目名稱Deep Fields網(wǎng)絡(luò)公開度




書目名稱Deep Fields網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Deep Fields被引頻次




書目名稱Deep Fields被引頻次學(xué)科排名




書目名稱Deep Fields年度引用




書目名稱Deep Fields年度引用學(xué)科排名




書目名稱Deep Fields讀者反饋




書目名稱Deep Fields讀者反饋學(xué)科排名

Perineum

978-3-642-07673-2Springer-Verlag Berlin Heidelberg 2001

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Interactive Graphics Using Mouse Eventsh-Kuiper Belt is explored by search projects to find its members and to classify the orbits. The early searches for Transneptunian Objects (TNOs) were all limited in detection range to below about 50 AU. Nevertheless, the results of these searches have proven the prediction that the inner Edgeworth-

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OPINE

Patterns at Work: Multiple Waves survey is to extend existing proper motion catalogues to fainter magnitudes and to detect new nearby low-luminosity objects. With more than 3000 square degrees covered so far, the list of detected objects with proper motions between 0.3 and 3.0 arcsec/yr and 10 < . < 20 exceeds 800 (50% of which ar

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https://doi.org/10.1007/978-1-4842-4366-4. Mpc) giant elliptical galaxy NGC 5128. This galaxy, also known as a bright radio source Centaurus A, displays a rich system of shells, optical filaments, radio lobes, as well as a radio and X-ray jet from an active nucleus. These all make it a classical example of a merger of an elliptical galaxy

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https://doi.org/10.1007/978-1-4842-4366-4yman-continuum radiation that escapes from galaxies at redshifts .. The combined UV-IR photometry for HDF galaxies is also used to investigate whether low-mass starburst galaxies dominate the field-galaxy population at redshift .. The relative lack of objects with the colors of faded bursts suggests

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https://doi.org/10.1007/978-1-4842-4366-4, and the corresponding predictions of the latest version of CDM hierarchical model of galaxy formation. In the photometric redshift distribution of . < 21 samples only 5% of the galaxies are found at ., as predicted by hierarchical scenarios where massive objects are the result of merging processes

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https://doi.org/10.1007/978-1-4842-4366-4gh redshift. Here we briefly review their history, and illustrate one application, using . NICMOS imaging of the Hubble Deep Field North to examine the rest-frame optical luminosities and colors of galaxies at 2 < . < 3, and to constrain their stellar masses. The rest-frame .-band luminosity density

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https://doi.org/10.1007/978-1-4842-4366-4 Galactic latitude fields with deep .. imaging reaching depths of . mag (AB) in the optical and . mag (AB) in the near-infrared. To date we have 626 spectroscopic redshifts for infrared-selected SPICES sources with .. < 20 (Vega). The project is poised to address galaxy formation and evolution to re