標(biāo)題: Titlebook: Deep Fields; Proceedings of the E Stefano Cristiani,Alvio Renzini,Robert E. Williams Conference proceedings 2001 Springer-Verlag Berlin Hei [打印本頁] 作者: 不友善 時間: 2025-3-21 19:37
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
作者: Perineum 時間: 2025-3-21 23:58
978-3-642-07673-2Springer-Verlag Berlin Heidelberg 2001作者: CHURL 時間: 2025-3-22 03:24
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-作者: 空洞 時間: 2025-3-22 07:06 作者: OPINE 時間: 2025-3-22 09:23
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作者: expunge 時間: 2025-3-22 16:00
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 作者: expunge 時間: 2025-3-22 19:46
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作者: 善于騙人 時間: 2025-3-22 21:22
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作者: 抗生素 時間: 2025-3-23 01:36
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作者: 公共汽車 時間: 2025-3-23 06:38
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作者: 放大 時間: 2025-3-23 12:16 作者: 平常 時間: 2025-3-23 17:42
https://doi.org/10.1007/978-1-4842-4366-4HDFs are prone to selection biases. These biases are extremely severe beyond . such that a meaningful interpretation of generic galaxy evolution is not possible. We can however extract well defined volume-limited samples at . < 1. The data are entirely consistent with passive/null-evolution for elli作者: IOTA 時間: 2025-3-23 20:55 作者: Incompetent 時間: 2025-3-24 01:48
https://doi.org/10.1007/978-1-4842-4366-4mits (Ferguson et al. [11]). This is also the aim of the FORS Deep Field (FDF), which has about 5 times the field-size of the two Hubble Deep Fields together and, in addition, contains a relatively bright quasar of 18.5mag at . = 3.36 at its center. A full exploration of the FDF multicolor data requ作者: BADGE 時間: 2025-3-24 03:32 作者: 捐助 時間: 2025-3-24 07:16
Deep Fields978-3-540-45514-1Series ISSN 1431-2433 Series E-ISSN 1611-6143 作者: sundowning 時間: 2025-3-24 14:01
Stefano Cristiani,Alvio Renzini,Robert E. WilliamsThis is the first survey of deep field astronomy, based on the new instruments of ESO and STSCI作者: CON 時間: 2025-3-24 17:36 作者: beta-cells 時間: 2025-3-24 20:31
Hans Jürgen Ohlbach,Norbert EisingerI give examples of stellar work that is done with data collected in the course of extragalactic surveys, including the Hamburg/ESO objective-prism survey. I list some considerations to be taken into account for future (stellar) surveys.作者: 仇恨 時間: 2025-3-25 02:29 作者: 有花 時間: 2025-3-25 05:02
https://doi.org/10.1007/978-1-4842-4366-4Optical observations of INSs are reviewed and their emission properties discussed in an evolutionary framework.作者: 爆米花 時間: 2025-3-25 10:52
https://doi.org/10.1007/978-1-4842-4366-4We summarise the main results of recent work on the Lyman break galaxy population which takes advantage of newly commissioned instrumentation on the VLT and Keck telescopes to push the detection of these objects to new wavelengths and more sensitive limits.作者: 玩笑 時間: 2025-3-25 13:36
https://doi.org/10.1007/978-1-4842-4366-4We present a status report of the ground-based follow-up observations of the Hubble Deep Field South underway with ESO facilities, in La Silla or Paranal. This includes broad-band and interference filters imaging, as well as spectroscopy, both in the visible and in the IR.作者: 無辜 時間: 2025-3-25 16:05 作者: 建筑師 時間: 2025-3-25 21:13
,Working on Other People’s “Waste”: Stars in Extragalactic Surveys,I give examples of stellar work that is done with data collected in the course of extragalactic surveys, including the Hamburg/ESO objective-prism survey. I list some considerations to be taken into account for future (stellar) surveys.作者: NATAL 時間: 2025-3-26 01:36 作者: 符合規(guī)定 時間: 2025-3-26 06:58
Like Candles on the Moon: Optical Observations of Pulsars,Optical observations of INSs are reviewed and their emission properties discussed in an evolutionary framework.作者: 粗俗人 時間: 2025-3-26 10:04 作者: 柔聲地說 時間: 2025-3-26 12:53 作者: Mitigate 時間: 2025-3-26 18:15
A Progress Report on the Caltech Faint Galaxy Redshift Survey,I review recent progress on determining the SEDs and luminosity functions for galaxies in the large magnitude limited sample in the region of the HDF-North of the Caltech Faint Galaxy Redshift Survey.作者: 心神不寧 時間: 2025-3-26 23:02 作者: manifestation 時間: 2025-3-27 05:03
1431-2433 astronomy, based on the powerful telescopes and instruments developed in recent years. It is organized along topical themes, such as the extragalactic background radiation at different wavelengths, the evolution of galaxies, the history of star formation, the nature of absorbers, the reionization of作者: anaphylaxis 時間: 2025-3-27 07:14 作者: Phagocytes 時間: 2025-3-27 10:36
https://doi.org/10.1007/978-1-4842-4366-4rios. On the other hand, they provide the possibility to find dust obscured starbursts, a fraction of which may trace the formation of proto-ellipticals at . > 2. In this paper, the most recent results on EROs are reviewed and the main implications discussed.作者: reflection 時間: 2025-3-27 15:21 作者: 外形 時間: 2025-3-27 21:25 作者: tackle 時間: 2025-3-27 22:47
Conference proceedings 2001f galaxies. Stellar and substellar objects were not neglected, however, and one session was devoted to nearby bodies such as trans-Neptunian solar system objects, brown dwarfs, and stars with special characteristics.作者: CARE 時間: 2025-3-28 05:10 作者: 種類 時間: 2025-3-28 06:22
Exploring the Formation and Evolution of Massive Ellipticals with Extremely Red Objects,rios. On the other hand, they provide the possibility to find dust obscured starbursts, a fraction of which may trace the formation of proto-ellipticals at . > 2. In this paper, the most recent results on EROs are reviewed and the main implications discussed.作者: outset 時間: 2025-3-28 12:29 作者: 價值在貶值 時間: 2025-3-28 14:52 作者: MIRE 時間: 2025-3-28 21:59
Patterns at Work: Multiple Waves and very late-type dwarfs and subdwarfs. Among the new high proper motion objects, the coolest subdwarf was discovered in follow-up observations with Keck [17]. The APM discoveries have also lead to the finding of a new population of ancient Halo white dwarfs that make up 10% of the Galactic Halo dark matter [6].作者: 音樂學(xué)者 時間: 2025-3-29 01:16
https://doi.org/10.1007/978-1-4842-4366-4 galaxy and Field 2 is in the halo 9 kpc away from the center. The shell in Field 1 can be naturally explained to be the stellar debris of the smaller galaxy accreted by NGC 5128 approximately 160 to 500 Myr ago.作者: 歌曲 時間: 2025-3-29 05:53
https://doi.org/10.1007/978-1-4842-4366-4the theoretical predictions, so that no major challenge for the CDM scenarios emerge from this comparison. However, the discrepancies observed suggest that an improvement in the knowledge and in the treatment or the physical ingredients of the models is still needed.作者: Diuretic 時間: 2025-3-29 09:58 作者: 心胸開闊 時間: 2025-3-29 13:54
https://doi.org/10.1007/978-1-4842-4366-4m 0 < . < 4. If these methods are reliable, as is suggested by a local galaxy calibration, the merger fraction of galaxies scales ., peaks near ., and declines thereafter. I also discuss how this system is likely part of the ultimate physical classification of galaxies.作者: 姑姑在炫耀 時間: 2025-3-29 17:05 作者: Wernickes-area 時間: 2025-3-29 22:16
Deep VLT Imaging of NGC 5128, galaxy and Field 2 is in the halo 9 kpc away from the center. The shell in Field 1 can be naturally explained to be the stellar debris of the smaller galaxy accreted by NGC 5128 approximately 160 to 500 Myr ago.作者: BUOY 時間: 2025-3-30 01:39 作者: 釘牢 時間: 2025-3-30 06:56
First Results from the SPICES Survey, > 1. One of the SPICES fields has been the target of a deep 190 ksec . exposure; we discuss initial results from analysis of that data set. Finally, we briefly discuss a successful campaign to identify high-redshift sources in the SPICES fields.作者: CHAR 時間: 2025-3-30 11:13
Morphological Evolution of Galaxies to ,,m 0 < . < 4. If these methods are reliable, as is suggested by a local galaxy calibration, the merger fraction of galaxies scales ., peaks near ., and declines thereafter. I also discuss how this system is likely part of the ultimate physical classification of galaxies.作者: 受辱 時間: 2025-3-30 15:17
1431-2433 re not neglected, however, and one session was devoted to nearby bodies such as trans-Neptunian solar system objects, brown dwarfs, and stars with special characteristics.978-3-642-07673-2978-3-540-45514-1Series ISSN 1431-2433 Series E-ISSN 1611-6143 作者: 殺死 時間: 2025-3-30 18:30 作者: inferno 時間: 2025-3-31 00:36
https://doi.org/10.1007/978-1-4842-4366-4one place upper limit to the abundance of Ly-. galaxies. From the comparison with Ly-. surveys at . we conclude that bright Ly-. galaxies become such rare beyond . = 5 that a non-evolving population seems virtually excluded.作者: 商業(yè)上 時間: 2025-3-31 04:20 作者: 思考 時間: 2025-3-31 06:15 作者: babble 時間: 2025-3-31 11:13 作者: Orchiectomy 時間: 2025-3-31 16:44 作者: Liberate 時間: 2025-3-31 20:25 作者: slow-wave-sleep 時間: 2025-4-1 01:00 作者: Dorsal 時間: 2025-4-1 03:24 作者: arboretum 時間: 2025-4-1 07:41
Deep in a Star-Forming Region with the VLT: Looking for Sub-Jupiter Mass Objects, larger than they would have if emitting like black bodies. Model predictions of exotic near-infrared colors due to prominent molecular bands have been confirmed by very cool evolved objects discovered in a variety of surveys, implying that such very cool objects are both detectable as well as relat作者: MAZE 時間: 2025-4-1 13:18 作者: motivate 時間: 2025-4-1 17:37
Deep VLT Imaging of NGC 5128,. 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
