31
31
Oct 6, 2009
10/09
by
NASA/JPL-Caltech/H. Dole (IAS)
image
eye 31
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Coaxing out a signal: this graphic demonstrates how the 24 micron images (shown in blue) of over 20,000 faint galaxies were added up to create a detectable signal at longer wavelengths. In each individual observation, the galaxy is barely visible at 24 microns and invisible at longer wavelengths. When the observations are combined, however, the longer-wavelength images emerge.
Source: http://sscws1.ipac.caltech.edu/Imagegallery/image.php?image_name=sig06-009
52
52
Sep 19, 2013
09/13
by
G. Lagache; H. Dole; J. -L. Puget
texts
eye 52
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To characterise the cosmological evolution of the sources contributing to the infrared extragalactic background, we have developped a phenomenological model that constrains in a simple way the galaxy luminosity function evolution with the redshift, and fits all the existing source counts and redshift distributions, Cosmic Infrared Background intensity and fluctuations observations, from the mid-infrared to the submillimetre range. The model is based on template spectra of starburst and normal...
Source: http://arxiv.org/abs/astro-ph/0209115v1
50
50
Sep 18, 2013
09/13
by
G. Lagache; H. Dole; J. -L. Puget
texts
eye 50
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The discovery of the Cosmic Infrared Background (CIB) in 1996, together with recent cosmological surveys from the mid-infrared to the millimeter have revolutionized our view of star formation at high redshifts. It has become clear, in the last decade, that a population of galaxies that radiate most of their power in the far-infrared (the so-called ``infrared galaxies'') contributes an important part of the whole galaxy build-up in the Universe. Since 1996, detailed (and often painful)...
Source: http://arxiv.org/abs/astro-ph/0509556v1
Performer: Renato Zanelli Writer: Nathan H. Dole; Vincenzo Di Chiara Baritone with orchestra; In Italian. Digitized at 78 revolutions per minute. Four stylii were used to transfer this record. They are 3.8mil truncated conical, 2.3mil truncated conical, 2.8mil truncated conical, 3.3mil truncated conical. The preferred versions suggested by an audio engineer at George Blood, L.P. have been copied to have the more friendly filenames. Matrix number: 64834 Catalog number: 64834
( 1 reviews )
Topics: 78rpm, Popular Music
Source: 78
45
45
Sep 23, 2013
09/13
by
J. Patris; M. Dennefeld; G. Lagache; H. Dole
texts
eye 45
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We present optical spectroscopy of the brightest 170 microns sources in the FIRBACK South Marano (FSM) field. The survey is 90% complete at the 4 sigma level. The spectra are compared with those of a reference sample of faint IRAS (60 microns selected) sources observed in the same conditions . The galaxies in both samples are characterized by a predominance of emission-line spectra and moderate IR luminosities (10E10.5 < L_IR < 10E12 L_Sun). The fraction of AGN's is low (about 15%) and...
Source: http://arxiv.org/abs/astro-ph/0312598v1
Performer: Renato Zanelli Writer: Nathan H. Dole; Vincenzo Di Chiara Baritone with orchestra; In Italian. Digitized at 78 revolutions per minute. Four stylii were used to transfer this record. They are 3.8 mil truncated eliptical, 2.3 mil truncated conical, 2.8 mil truncated conical, 3.3 mil truncated eliptical. The preferred versions suggested by an audio engineer at George Blood, L.P. have been copied to have the more friendly filenames. Matrix number: 64834 Catalog number: 64834
( 1 reviews )
Topics: 78rpm, Popular Music, acoustic
Source: 78
68
68
Sep 17, 2013
09/13
by
M. Béthermin; H. Dole; M. Cousin; N. Bavouzet
texts
eye 68
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comment 0
BLAST (Balloon-borne Large-Aperture Submillimeter Telescope) performed the first deep and wide extragalactic survey at 250, 350 and 500 um. The extragalactic number counts at these wavelengths are important constraints for modeling the infrared galaxies evolution. [...] We use three methods to identify the submillimeter sources. 1) Blind extraction. [...] The photometry is computed with a new simple and quick PSF fitting routine (FASTPHOT). [...] 2) Extraction with prior. [...] 3) A stacking...
Source: http://arxiv.org/abs/1003.0833v4
78 RPMs and Cylinder Recordings
52
52
Jan 23, 2021
01/21
by
John McCormack and Fritz Kreisler; Moszkowski; Nathan H. Dole
audio
eye 52
favorite 1
comment 1
Performer: John McCormack and Fritz Kreisler Writer: Moszkowski; Nathan H. Dole Tenor and Violin with orchestra; (English word by). Digitized at 78 revolutions per minute. Four stylii were used to transfer this record. They are 3.8mil truncated conical, 2.3mil truncated conical, 2.8mil truncated conical, 3.3mil truncated conical. The preferred versions suggested by an audio engineer at George Blood, L.P. have been copied to have the more friendly filenames. Matrix number: 87230 Catalog number:...
( 1 reviews )
Topics: 78rpm, Popular Music
Source: 78
40
40
Sep 18, 2013
09/13
by
D. Elbaz; E. Le Floc'h; H. Dole; D. Marcillac
texts
eye 40
favorite 0
comment 0
We present ISOCAM 15 micron and MIPS 24 micron photometry of a sample of 16 distant Luminous Infrared Galaxies (LIRGs) characterized by a median luminosity L(IR) 2x10^11 Lsol and redshift z = 0.7 (distributed from z = 0.1 to 1.2). While some sources display 24/15 micron flux ratios also consistent with a featureless continuum dominating their mid-infrared (MIR) spectral energy distributions (SEDs), the presence of prominent emission features such as the Polycyclic Aromatic Hydrocarbons is...
Source: http://arxiv.org/abs/astro-ph/0502569v1
78 RPMs and Cylinder Recordings
112
112
Nov 28, 2019
11/19
by
John McCormack and Fritz Kreisler; Moskowski; Nathan H. Dole
audio
eye 112
favorite 0
comment 1
Performer: John McCormack and Fritz Kreisler Writer: Moskowski; Nathan H. Dole Tenor and Violin with Orchestra. Digitized at 78 revolutions per minute. Four stylii were used to transfer this record. They are 3.5mil truncated eliptical, 2.3mil truncated conical, 2.8mil truncated conical, 3.3mil truncated conical. These were recorded flat and then also equalized with Turnover: 500.0. The preferred versions suggested by an audio engineer at George Blood, L.P. have been copied to have the more...
( 1 reviews )
Topics: 78rpm, Classical
Source: 78
78 RPMs and Cylinder Recordings
100
100
Feb 18, 2018
02/18
by
John McCormack and Fritz Kreisler; Moszkowski; Nathan H. Dole
audio
eye 100
favorite 0
comment 1
Performer: John McCormack and Fritz Kreisler Writer: Moszkowski; Nathan H. Dole Tenor and Violin with orchestra; English words. Digitized at 78 revolutions per minute. Four stylii were used to transfer this record. They are 3.8 mil truncated conical, 2.3 mil truncated conical, 2.8 mil truncated conical, 3.3 mil truncated conical. The preferred versions suggested by an audio engineer at George Blood, L.P. have been copied to have the more friendly filenames. Matrix number: 87547 Catalog number:...
( 1 reviews )
Topics: 78rpm, Popular Music
Source: 78
78 RPMs and Cylinder Recordings
115
115
Feb 23, 2018
02/18
by
Moszkowski; John McCormack and Fritz Kriesler; Nathan H. Dole
audio
eye 115
favorite 0
comment 1
Writer: Moszkowski; Nathan H. Dole Performer: John McCormack and Fritz Kriesler Tenor with Violin obbligato and orchestra. Digitized at 78 revolutions per minute. Four stylii were used to transfer this record. They are 3.8 mil truncated conical, 2.3 mil truncated conical, 2.8 mil truncated conical, 3.3 mil truncated conical. The preferred versions suggested by an audio engineer at George Blood, L.P. have been copied to have the more friendly filenames. Matrix number: 87230 Catalog number: 87230
( 1 reviews )
Topics: 78rpm, Popular Music
Source: 78
78
78
Sep 23, 2013
09/13
by
N. Fernandez-Conde; G. Lagache; J. -L. Puget; H. Dole
texts
eye 78
favorite 0
comment 0
The coming Planck and Herschel missions will survey the sky at unprecedented angular scales and sensitivities. Simulations are needed for better interpretating the results of the surveys and for testing new methods of, e.g., source extraction and component separation. We present new simulations of the infrared and submillimeter cosmic background, including the correlation between infrared galaxies. The simulations were used to quantify the source-detection thresholds for Herschel/SPIRE and...
Source: http://arxiv.org/abs/0801.4299v1
55
55
Jul 20, 2013
07/13
by
K. I. Caputi; H. Dole; G. Lagache; J. -L. Puget
texts
eye 55
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We present the results of our most recent works on Spitzer/MIPS 24 micron galaxies. Through a multiwavelength analysis, we study different properties (redshifts, luminosities, stellar masses) characterising the sources which produce the bulk of the mid-IR background. From a comparative study with the total population of Ks-selected galaxies, we determine that 24 micron sources account for an important fraction of the most massive galaxies present at different redshifts. On the other hand, we...
Source: http://arxiv.org/abs/astro-ph/0604236v1
52
52
Sep 22, 2013
09/13
by
N. Fernandez-Conde; G. Lagache; J-L. Puget; H. Dole
texts
eye 52
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comment 0
Herschel and Planck are surveying the sky at unprecedented angular scales and sensitivities over large areas. But both experiments are limited by source confusion in the submillimeter. The high confusion noise in particular restricts the study of the clustering properties of the sources that dominate the cosmic infrared background. At these wavelengths, it is more appropriate to consider the statistics of the unresolved component. In particular, high clustering will contribute in excess of...
Source: http://arxiv.org/abs/1004.0123v1
63
63
Sep 22, 2013
09/13
by
A. Sajina; D. Scott; M. Dennefeld; H. Dole; M. Lacy; G. Lagache
texts
eye 63
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Galaxies selected at 170um by the ISO FIRBACK survey represent the brightest \~10% of the Cosmic Infrared Background. Examining their nature in detail is therefore crucial for constraining models of galaxy evolution. Here we combine Spitzer archival data with previous near-IR, far-IR, and sub-mm observations of a representative sample of 22 FIRBACK galaxies spanning three orders of magnitude in infrared luminosity. We fit a flexible, multi-component, empirical SED model of star-forming galaxies...
Source: http://arxiv.org/abs/astro-ph/0603614v1
64
64
Sep 22, 2013
09/13
by
S. K. Sirothia; M . Dennefeld; D. J. Saikia; H. Dole; F. Ricquebourg; J. Roland
texts
eye 64
favorite 0
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We present observations of the European Large-Area {\it ISO} Survey-North 1 (ELAIS-N1) at 325 MHz using the Giant Metrewave Radio Telescope (GMRT), with the ultimate objective of identifying active galactic nuclei and starburst galaxies and examining their evolution with cosmic epoch. After combining the data from two different days we have achieved a median rms noise of $\approx40 \mu$Jy beam$^{-1}$, which is the lowest that has been achieved at this frequency. We detect 1286 sources with a...
Source: http://arxiv.org/abs/0812.0813v1
49
49
Sep 21, 2013
09/13
by
N. Bavouzet; H. Dole; E. Le Floc'h; K. I. Caputi; G. Lagache; C. S. Kochanek
texts
eye 49
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We present the observed correlations between rest-frame 8, 24, 70 and 160 um monochromatic luminosities and measured total infrared luminosities L_IR of galaxies detected by Spitzer. Our sample consists of 372 star-forming galaxies with individual detections and flux measurements at 8, 24, 70 and 160 um. We have spectroscopic redshifts for 93% of these sources, and accurate photometric redshifts for the remainder. We also used a stacking analysis to measure the IR fluxes of fainter sources at...
Source: http://arxiv.org/abs/0712.0965v1
57
57
Sep 20, 2013
09/13
by
A. Sajina; C. Borys; S. Chapman; H. Dole; M. Halpern; G. Lagache; J. -L. Puget; D. Scott
texts
eye 57
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We present results from JCMT sub-mm observations of sources selected from the {\sl ISO} FIRBACK (Far-IR BACKground) survey, along with UKIRT near-IR imaging of a sub-sample. This gives valuable insight into the brightest $\sim$10% of galaxies which contribute to the Cosmic Infrared Background (CIB). We estimate the photometric redshifts and luminosities of these sources by fitting their Spectral Energy Distributions (SEDs). The data appear to show a bimodal galaxy distribution, with normal...
Source: http://arxiv.org/abs/astro-ph/0301427v3
54
54
Sep 18, 2013
09/13
by
M. Dennefeld; G. Lagache; S. Mei; P. Ciliegi; H. Dole; R. G. Mann; E. L. Taylor; M. Vaccari
texts
eye 54
favorite 0
comment 0
We present a detailed study of the brighter ($> 4\sigma$ detections) sources in the 170$\mu$m FIRBACK northern N1 ISO survey, with the help of complementary data in the optical, radio, and mid-IR domain. For 82% of them, an optical galaxy counterpart is identified, either as the unique source of the IR emission, or as part of a multiple identification. With less than 15% of AGNs, these sources are essentially local, moderate starbursters with a dominating cold dust component. and represent a...
Source: http://arxiv.org/abs/astro-ph/0504344v1
44
44
Sep 18, 2013
09/13
by
G. Lagache; N. Bavouzet; N. Fernandez-Conde; N. Ponthieu; T. Rodet; H. Dole; M. -A. Miville-Deschenes; J. -L. Puget
texts
eye 44
favorite 0
comment 0
We report the detection of correlated anisotropies in the Cosmic Far-Infrared Background at 160 microns. We measure the power spectrum in the Spitzer/SWIRE Lockman Hole field. It reveals unambiguously a strong excess above cirrus and Poisson contributions, at spatial scales between 5 and 30 arcminutes, interpreted as the signature of infrared galaxy clustering. Using our model of infrared galaxy evolution we derive a linear bias b=1.74 \pm 0.16. It is a factor 2 higher than the bias measured...
Source: http://arxiv.org/abs/0707.2443v1
77
77
Sep 19, 2013
09/13
by
K. I. Caputi; G. Lagache; Lin Yan; H. Dole; N. Bavouzet; E. Le Floc'h; P. I. Choi; G. Helou; N. Reddy
texts
eye 77
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We present the rest-frame 8 micron luminosity function (LF) at redshifts z=1 and ~2, computed from Spitzer 24 micron-selected galaxies in the GOODS fields over an area of 291 sq. arcmin. Using classification criteria based on X-ray data and IRAC colours, we identify the AGN in our sample. The rest-frame 8 micron LF for star-forming galaxies at redshifts z=1 and ~2 have the same shape as at z~0, but with a strong positive luminosity evolution. The number density of star-forming galaxies with...
Source: http://arxiv.org/abs/astro-ph/0701283v1
43
43
Sep 23, 2013
09/13
by
E. Le Floc'h; C. Papovich; H. Dole; E. Egami; P. Perez-Gonzalez; G. Rieke; M. Rieke; E. Bell; the Spitzer/MIPS GTO team
texts
eye 43
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Using deep observations of the Chandra Deep Field South obtained with MIPS at 24mic, we present our preliminary estimates on the evolution of the infrared (IR) luminosity density of the Universe from z=0 to z~1. We find that a pure density evolution of the IR luminosity function is clearly excluded by the data. The characteristic luminosity L_IR* evolves at least by (1+z)^3.5 with lookback time, but our monochromatic approach does not allow us to break the degeneracy between a pure evolution in...
Source: http://arxiv.org/abs/astro-ph/0411623v1
54
54
Jul 20, 2013
07/13
by
K. I. Caputi; H. Dole; G. Lagache; R. J. McLure; J. S. Dunlop; J. -L. Puget; E. Le Floc'h; P. G. Perez-Gonzalez
texts
eye 54
favorite 0
comment 0
We investigate the role of the luminous infrared galaxy (LIRG) and ultra-luminous infrared galaxy (ULIRG) phases in the evolution of Ks-selected galaxies and, in particular, Extremely Red Galaxies (ERGs). With this aim, we compare the properties of a sample of 2905 Ks 1x10^{11} Msun assembled at redshift z=0.5. A minimum of 65% of the galaxies with M>2.5x10^{11} Msun at z~2-3 are ULIRGs at those redshifts. 60% of the ULIRGs in our sample have the characteristic colours of ERGs. Conversely,...
Source: http://arxiv.org/abs/astro-ph/0604232v1
5
5.0
Jun 30, 2018
06/18
by
R. Canameras; N. P. H. Nesvadba; R. Kneissl; M. Limousin; R. Gavazzi; D. Scott; H. Dole; B. Frye; S. Koenig; E. Le Floc'h; I. Oteo
texts
eye 5
favorite 0
comment 0
We study the properties of the foreground galaxy of the Ruby, the brightest gravitationally lensed high-redshift galaxy on the sub-millimeter sky as probed by the Planck satellite, and part of our sample of Planck's Dusty GEMS. The Ruby consists of an Einstein ring of 1.4" diameter at z = 3.005 observed with ALMA at 0.1" resolution, centered on a faint, red, massive lensing galaxy seen with HST/WFC3, which itself has an exceptionally high redshift, z = 1.525 $\pm$ 0.001, as confirmed...
Topics: Astrophysics of Galaxies, Astrophysics
Source: http://arxiv.org/abs/1703.02984
5
5.0
Jun 28, 2018
06/18
by
I. Flores-Cacho; D. Pierini; G. Soucail; L. Montier; H. Dole; E. Pointecouteau; R. Pello; E. Le Floch; N. Nesvadba; G. Lagache; D. Guery; R. Canameras
texts
eye 5
favorite 0
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(abridged) We report the discovery of PHz G95.5-61.6, a complex structure detected in emission in the Planck all-sky survey that corresponds to two over-densities of high-redshift galaxies. This is the first source from the Planck catalogue of high-z candidates that has been completely characterised with follow-up observations from the optical to the sub-millimetre domain. Herschel/SPIRE observations at 250, 350 and 500 microns reveal the existence of five sources producing a 500 microns...
Topics: Astrophysics, Cosmology and Nongalactic Astrophysics, Astrophysics of Galaxies
Source: http://arxiv.org/abs/1510.01585
44
44
Sep 18, 2013
09/13
by
A. Beelen; A. Omont; N. Bavouzet; A. Kovacs; G. Lagache; C. de Breuck; A. Weiss; K. M. Menten; J. W. Colbert; H. Dole; G. Siringo; E. Kreysa
texts
eye 44
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comment 0
We present observations aimed at exploring both the nature of Lya emitting nebulae (Lya blobs) at z=2.38 and the way they trace large scale structure (LSS), by exploring their proximity to maximum starbursts through submillimeter emission. Our most important objectives are to make a census of associated submillimeter galaxies (SMGs), check their properties, and look for a possible overdensity in the protocluster J2142-4426 at z=2.38. We used the newly commissioned Large APEX Bolometer Camera...
Source: http://arxiv.org/abs/0803.1615v2
52
52
Sep 23, 2013
09/13
by
K. I. Caputi; H. Dole; G. Lagache; R. J. McLure; J. -L. Puget; G. H. Rieke; J. S. Dunlop; E. Le Floc'h; C. Papovich; P. G. Perez-Gonzalez
texts
eye 52
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comment 0
We present deep Ks 83 microJy (the 80% completeness limit of the Spitzer/GTO 24 micron catalog). 36% of our galaxies have spectroscopic redshifts (mostly at z 1.5. We determine the existence of a bump in the redshift distribution at z~1.9, indicating the presence of a significant population of galaxies with PAH emission at these redshifts. Massive (M>10^11 Msun) star-forming galaxies at redshifts 2500 Msun/yr), and some of them are able to construct a mass of 10^10-10^11 Msun in a single...
Source: http://arxiv.org/abs/astro-ph/0510070v1
47
47
Sep 19, 2013
09/13
by
M. Jauzac; H. Dole; E. Le Floc'h; H. Aussel; K. Caputi; O. Ilbert; M. Salvato; N. Bavouzet; A. Beelen; M. Béthermin; J. -P. Kneib; G. Lagache; J. -L. Puget
texts
eye 47
favorite 0
comment 0
The Cosmic Far-Infrared Background (CIB) at wavelengths around 160 {\mu}m corresponds to the peak intensity of the whole Extragalactic Background Light, which is being measured with increasing accuracy. However, the build up of the CIB emission as a function of redshift, is still not well known. Our goal is to measure the CIB history at 70 {\mu}m and 160 {\mu}m at different redshifts, and provide constraints for infrared galaxy evolution models. We use complete deep Spitzer 24 {\mu}m catalogs...
Source: http://arxiv.org/abs/1009.0419v1
58
58
Sep 19, 2013
09/13
by
J. L. Puget; G. Lagache; D. L Clements; W. T. Reach; H. Aussel; F. R Bouchet; C. Cesarsky; F. X. Désert; H. Dole; D. Elbaz; A. Franceschini; B. Guiderdoni; A. F. M Moorwood
texts
eye 58
favorite 0
comment 0
FIRBACK is a deep survey conducted with the ISOPHOT instrument aboard the Infrared Space Observatory (ISO) at an effective wavelength of 175 $\mu$m. We present here results we have obtained on the first field, the so-called Marano1 which covers around 0.25 square degree. We find that the source density for objects with a flux above 200 mJy exceeds the counts expected for sources found in the IRAS deep surveys with a similar flux by about an order of magnitude. Such an excess was expected on the...
Source: http://arxiv.org/abs/astro-ph/9812039v1
53
53
Sep 22, 2013
09/13
by
E. Egami; G. H. Rieke; J. R. Rigby; C. Papovich; J. -P. Kneib; G. P. Smith; E. Le Floc'h; K. A. Misselt; P. G. Perez-Gonzalez; J. -S. Huang; H. Dole; D. T. Frayer
texts
eye 53
favorite 0
comment 0
We are currently undertaking a Spitzer GTO program to image ~30 massive lensing clusters at moderate redshift with both IRAC and MIPS. By taking advantage of the gravitatinoal lensing power of these clusters, we will study the population of faint galaxies that are below the nominal Spitzer detection limits. Here, we present a few examples of our science programs.
Source: http://arxiv.org/abs/astro-ph/0603657v1
49
49
Sep 23, 2013
09/13
by
E. Egami; J. -P. Kneib; G. H. Rieke; R. S. Ellis; J. Richard; J. Rigby; C. Papovich; D. Stark; M. R. Santos; J. -S. Huang; H. Dole; E. Le Floc'h; P. G. Perez-Gonzalez
texts
eye 49
favorite 0
comment 0
We report the detection of a z~7 galaxy strongly lensed by the massive galaxy cluster Abell 2218 (z=0.175) at 3.6 and 4.5 um using the Spitzer Observatory and at 1.1 um using the Hubble Space Telescope. The new data indicate a refined photometric redshift in the range of 6.6-6.8 depending on the presence of Ly-alpha emission. The spectral energy distribution is consistent with having a significant Balmer break, suggesting that the galaxy is in the poststarburst stage with an age of at least ~50...
Source: http://arxiv.org/abs/astro-ph/0411117v2
26
26
Jun 27, 2018
06/18
by
R. Leiton; D. Elbaz; K. Okumura; H. S. Hwang; G. Magdis; B. Magnelli; I. Valtchanov; M. Dickinson; M. Béthermin; C. Schreiber; V. Charmandaris; H. Dole; S. Juneau; D. Le Borgne; M. Pannella; A. Pope; P. Popesso
texts
eye 26
favorite 0
comment 0
We propose a new method of pushing $Herschel$ to its faintest detection limits using universal trends in the redshift evolution of the far infrared over 24$\mu$m colours in the well-sampled GOODS-North field. An extension to other fields with less multi-wavelength information is presented. This method is applied here to raise the contribution of individually detected $Herschel$ sources to the cosmic infrared background (CIRB) by a factor 5 close to its peak at 250$\mu$m and more than 3 in the...
Topics: Astrophysics of Galaxies, Astrophysics
Source: http://arxiv.org/abs/1503.05779
44
44
Jul 20, 2013
07/13
by
G. Lagache; H. Dole; J. -L. Puget; P. G. Perez-Gonzalez; E. Le Floc'h; G. H. Rieke; C. Papovich; E. Egami; A. Alonso-Herrero; C. W. Engelbracht; K. D. Gordon; K. A. Misselt; J. E. Morrision
texts
eye 44
favorite 0
comment 0
We present an updated phenomenological galaxy evolution model to fit the Spitzer 24, 70 and 160 microns number counts as well as all the previous mid and far infrared observations. Only a minor change of the co-moving luminosity density distribution in the previous model (Lagache, Dole, Puget 2003), combined with a slight modification of the starburst template spectra mainly between 12 and 30 microns, are required to fit all the data available. We show that the peak in the MIPS 24 micron counts...
Source: http://arxiv.org/abs/astro-ph/0406016v1
University of Illinois 78rpm Collection
1,146
1.1K
Jul 18, 2020
07/20
by
J. Fauré; The Westminister Singers; Palestrina; Oliver Holden; Henry Smart; Nathan H. Dole; The Westminster Singers; George Elvey; Charles Wesley; F. E. Weatherly; Edward Perronet; Arthur Sullivan; Jules Granier; Münster; JOHN SEAGLE; Charles Gounod; Stephen Adams
audio
eye 1,146
favorite 0
comment 1
Performer: JOHN SEAGLE; The Westminster Singers; The Westminister Singers Writer: Charles Wesley; Münster; Stephen Adams; F. E. Weatherly; Oliver Holden; Edward Perronet; Henry Smart; Charles Gounod; Palestrina; Jules Granier; Nathan H. Dole; Arthur Sullivan; George Elvey; J. Fauré Baritone with Chorus and Organ; Baritone with Organ. Digitized at 78 revolutions per minute. Four stylii were used to transfer these records. They are 3.5mil truncated eliptical, 2.3mil truncated conical, 2.8mil...
( 1 reviews )
Topics: Sacred, 78rpm
Source: 78
58
58
Sep 20, 2013
09/13
by
E. Le Floc'h; C. Papovich; H. Dole; E. Bell; G. Lagache; G. Rieke; E. Egami; P. Perez-Gonzalez; A. Alonso-Herrero; M. Rieke; M. Blaylock; C. Engelbracht; K. Gordon; D. Hines; K. Misselt; J. Morrison; J. Mould
texts
eye 58
favorite 0
comment 0
We analyze a sample of ~2600 MIPS/Spitzer 24mic sources brighter than ~80muJy and located in the Chandra Deep Field South to characterize the evolution of the comoving infrared (IR) energy density of the Universe up to z~1. Using published ancillary optical data we first obtain a nearly complete redshift determination for the 24mic objects associated with R
Source: http://arxiv.org/abs/astro-ph/0506462v1
67
67
Sep 18, 2013
09/13
by
David L. Clements; J-L Puget; G. Lagache; H. Dole; P. Cox; R. Gispert; W. T. Reach; C. Cesarsky; D. Elbaz; H. Aussel; F. Bouchet; B. Guiderdoni; A. Omont; F-X. Desert; A. Franceschini; A. Moorwood; D. Lemke
texts
eye 67
favorite 0
comment 0
The FIRBACK project is a collaboration of eight institutes aimed at using long wavelength surveys with ISO to uncover the nature of the Cosmic Far-Infrared Background. We have surveyed nearly 4 sq. deg. in three regions in the northern and southern hemispheres with the ISOPHOT instrument on ISO, using the 175 micron filter. As reported by Puget et al. (1998) and Reach et al. (these proceedings), the first 0.25 sq. deg. region studied in this programme contains many more 175 micron sources than...
Source: http://arxiv.org/abs/astro-ph/9809054v1
16
16
Jun 28, 2018
06/18
by
B. Bertincourt; G. Lagache; B. Schulz; L. Conversi; K. Dassas; P. G. Martin; L. Maurin; A. Abergel; A. Beelen; J-P. Bernard; B. P. Crill; H. Dole; S. Eales; J. E. Gudmundsson; E. Lellouch; R. Moreno; O. Perdereau
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We compare the absolute gain photometric calibration of the Planck/HFI and Herschel/SPIRE instruments on diffuse emission. The absolute calibration of HFI and SPIRE each relies on planet flux measurements and comparison with theoretical far-infrared emission models of planetary atmospheres. We measure the photometric cross calibration between the instruments at two overlapping bands, 545 GHz / 500 $\mu$m and 857 GHz / 350 $\mu$m. The SPIRE maps used have been processed in the Herschel...
Topics: Instrumentation and Methods for Astrophysics, Astrophysics, Cosmology and Nongalactic Astrophysics,...
Source: http://arxiv.org/abs/1509.01784
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49
Sep 22, 2013
09/13
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A. Kovács; A. Omont; A. Beelen; C. Lonsdale; M. Polletta; N. Fiolet; T. R. Greve; C. Borys; P. Cox; C. De Breuck; H. Dole; C. D. Dowell; D. Farrah; G. Lagache; K. M. Menten; T. A. Bell; F. Owen
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eye 49
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We present SHARC-2 350 micron data on 20 luminous z ~ 2 starbursts with S(1.2mm) > 2 mJy from the Spitzer-selected samples of Lonsdale et al. and Fiolet et al. All the sources were detected, with S(350um) > 25 mJy for 18 of them. With the data, we determine precise dust temperatures and luminosities for these galaxies using both single-temperature fits and models with power-law mass--temperature distributions. We derive appropriate formulae to use when optical depths are non-negligible....
Source: http://arxiv.org/abs/1004.0819v2
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42
Sep 23, 2013
09/13
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A. Alonso-Herrero; P. G. Perez-Gonzalez; D. M. Alexander; G. H. Rieke; D. Rigopoulou; E. Le Floc'h; P. Barmby; C. Papovich; J. R. Rigby; F. E. Bauer; W. N. Brandt; E. Egami; S. P. Willner; H. Dole; J. -S. Huang
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eye 42
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We investigate the nature of a sample of 92 Spitzer/MIPS 24 micron selected galaxies in the CDFS, showing power law-like emission in the Spitzer/IRAC 3.6-8 micron bands. The main goal is to determine whether the galaxies not detected in X-rays (47% of the sample) are part of the hypothetical population of obscured AGN not detected even in deep X-ray surveys. The majority of the IR power-law galaxies are ULIRGs at z>1, and those with LIRG-like IR luminosities are usually detected in X-rays....
Source: http://arxiv.org/abs/astro-ph/0511507v1
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46
Sep 22, 2013
09/13
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E. Egami; K. A. Misselt; G. H. Rieke; M. W. Wise; G. Neugebauer; J. -P. Kneib; E. Le Floc'h; G. P. Smith; M. Blaylock; H. Dole; D. T. Frayer; J. -S. Huang; O. Krause; C. Papovich; P. G. Perez-Gonzalez; J. R. Rigby
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eye 46
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We have studied the infrared properties of the brightest cluster galaxies (BCGs) located in the cores of X-ray-luminous clusters at 0.15 < z < 0.35. The majority of the BCGs are not particularly infrared-luminous compared with other massive early-type galaxies, suggesting that the cluster environment has little influence on the infrared luminosities of the BCGs. The exceptions, however, are the BCGs in the three X-ray-brightest clusters in the sample, A1835, Z3146, and A2390. These BCGs...
Source: http://arxiv.org/abs/astro-ph/0603656v1
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36
Sep 20, 2013
09/13
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E. L. Taylor; R. G. Mann; A. N. Efstathiou; T. S. R. Babbedge; M. Rowan-Robinson; G. Lagache; A. Lawrence; S. Mei; M. Vaccari; Ph. Heraudeau; S. J. Oliver; M. Dennefeld; I. Perez-Fournon; S. Serjeant; E. Gonzalez-Solares; J. -L. Puget; H. Dole; C. Lari
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eye 36
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We report on a search for the optical counterparts of 175 um - selected sources from the Far-Infrared Background (FIRBACK) survey in the European Large Area ISO Survey (ELAIS) N2 field. Applying a likelihood ratio technique to optical catalogues from the Isaac Newton Telescope - Wide Field Survey (INT--WFS), we found optical identifications for 33 out of 55 FIRBACK sources in this field. These were then reassessed in the light of associations with the ELAIS final catalogue for the the N2 field,...
Source: http://arxiv.org/abs/astro-ph/0506273v1
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90
Jul 20, 2013
07/13
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J. -S. Huang; P. Barmby; G. G. Fazio; S. P. Willner; G. Wilson; D. Rigopoulou; A. Alonso-Herrero; H. Dole; E. Egami; E. Le Floc'h; C. Papovich; P. G. Perez-Gonzalez; J. Rigby; C. W. Engelbracht; K. Gordon; D. Hines; M. Rieke; G. H. Rieke; K Meisenheimer; S. Miyzaki
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eye 90
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IRAC imaging of a 4'7x4'7 area in the Lockman Hole detected over 400 galaxies in the IRAC 3.6 micron and 4.5 micron bands, 120 in the 5.8 micron, and 80 in the 8 micron bandin 30 minutes of observing time. Color-color diagrams suggest that about half of these galaxies are at redshifts 0.61.3). We also detect IRAC counterparts for 6 of the 7 SCUBA sources and all 9 XMM sources in this area. The detection of the counterparts of the SCUBA sources and galaxies at z>1.3 demonstrates the ability...
Source: http://arxiv.org/abs/astro-ph/0406006v2
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60
Sep 18, 2013
09/13
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G. Lagache; J-L. Puget; A. Abergel; F. R. Bouchet; F. Boulanger; P. Ciliegi; D. L. Clements; C. J. Cesarsky; F. X. Désert; H. Dole; D. Elbaz; A. Franceschini; R. Gispert; B. Guiderdoni; L. M. Haffner; M. Harwit; R. Laureijs; D. Lemke; A. F. M. Moorwood; S. Oliver; W. T. Reach; R. J. Reynolds; M. Rowan-Robinson; M. Stickel; S. L. Tufte
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eye 60
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A Cosmic Far-InfraRed Background (CFIRB) has long been predicted that would traces the intial phases of galaxy formation. It has been first detected by Puget et al.(1996) using COBE data and has been later confirmed by several recent studies (Fixsen et al. 1998, Hauser et al. 1998, Lagache et al. 1999). We will present a new determination of the CFIRB that uses for the first time, in addition to COBE data, two independent gas tracers: the HI survey of Leiden/Dwingeloo (hartmann, 1998) and the...
Source: http://arxiv.org/abs/astro-ph/0002284v1
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56
Jul 20, 2013
07/13
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Casey Papovich; H. Dole; E. Egami; E. Le Floc'h; P. G. Perez-Gonzalez; A. Alonso-Herrero; L. Bai; C. A. Beichman; M. Blaylock; C. W. Engelbracht; K. D. Gordon; D. C. Hines; K. A. Misselt; J. E. Morrison; J. Mould; J. Muzerolle; G. Neugebauer; P. L. Richards; G. H. Rieke; M. J. Rieke; J. R. Rigby; K. Y. L. Su; E. T. Young
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eye 56
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Galaxy source counts in the infrared provide strong constraints on the evolution of the bolometric energy output from distant galaxy populations. We present the results from deep 24 micron imaging from Spitzer surveys, which include approximately 50,000 sources to an 80% completeness of 60 uJy. The 24 micron counts rapidly rise at near-Euclidean rates down to 5 mJy, increase with a super-Euclidean rate between 0.4 - 4 mJy, and converge below 0.3 mJy. The 24 micron counts exceed expectations...
Source: http://arxiv.org/abs/astro-ph/0406035v1
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64
Sep 20, 2013
09/13
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G. Wilson; J. -S. Huang; P. G. Perez-Gonzalez; E. Egami; R. J. Ivison; J. R. Rigby; A. Alonso-Herrero; P. Barmby; H. Dole; G. G. Fazio; E. Le Floc'h; C. Papovich; D. Rigopoulou; L. Bai; C. W. Engelbracht; D. Frayer; K. D. Gordon; D. C. Hines; K. A. Misselt; S. Miyazaki; J. E. Morrison; G. H. Rieke; M. J. Rieke; J. Surace
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eye 64
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We investigate Extremely Red Objects (EROs) using near- and mid-infrared observations in five passbands (3.6 to 24 micron) obtained from the Spitzer Space Telescope, and deep ground-based R and K imaging. The great sensitivity of the IRAC camera allows us to detect 64 EROs in only 12 minutes of IRAC exposure time, by means of an R-[3.6] color cut (analogous to the traditional red R-K cut). A pure infrared K-[3.6] red cut detects a somewhat different population and may be more effective at...
Source: http://arxiv.org/abs/astro-ph/0405612v1
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95
Jul 20, 2013
07/13
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H. Dole; E. Le Floc'h; P. G. Perez-Gonzalez; C. Papovich; E. Egami; G. Lagache; A. Alonso-Herrero; C. W. Engelbracht; K. D. Gordon; D. C. Hines; O. Krause; K. A. Misselt; J. E. Morrison; G. H. Rieke; M. J. Rieke; J. R. Rigby; E. T. Young; L. Bai; M. Blaylock; G. Neugebauer; C. A. Beichman; D. T. Frayer; J. R. Mould; P. L. Richards
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eye 95
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We derive galaxy source counts at 70 and 160 microns using the Multiband Imaging Photometer for Spitzer (MIPS) to map the Chandra Deep Field South (CDFS) and other fields. At 70 microns, our observations extend upwards about 2 orders of magnitude in flux density from a threshold of 15 mJy, and at 160 microns they extend about an order of magnitude upward from 50 mJy. The counts are consistent with previous observations on the bright end. Significant evolution is detected at the faint end of the...
Source: http://arxiv.org/abs/astro-ph/0406021v2
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89
Sep 24, 2013
09/13
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M. Rowan-Robinson; T. Babbedge; J. Surace; D. Shupe; F. Fang; C. Lonsdale; E. E. Smith; M. Polletta; B. Siana; E. Gonzalez-Solares; C. Xu; F. Owen; P. Davoodi; H. Dole; D. Dominghue; A. Efstathiou; D. Farrah; M. Fox; A. Franceschini; D. Frayer; E. Hatzimaoglou; F. Masci; G. Morrison; K. Nandra; S. Oliver; N. Onyett; D. Padgett; I. Perez-Fournon; S. Serjeant; G. Stacey; M. Vaccari
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eye 89
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We discuss optical associations, spectral energy distributions and photometric redshifts for SWIRE sources in the ELAIS-N1 area and the Lockman Validation Field. The band-merged IRAC (3.6, 4.5, 5.8 and 8.0 mu) and MIPS (24, 70, 160 mu) data have been associated with optical UgriZ data from the INT Wide Field Survey in ELAIS-N1, and with our own optical Ugri data in Lockman-VF. The spectral energy distributions of selected ELAIS sources in N1 detected by SWIRE, most with spectroscopic redshifts,...
Source: http://arxiv.org/abs/astro-ph/0412184v2
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55
Jul 20, 2013
07/13
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S. Serjeant; A. M. J. Mortier; R. J. Ivison; E. Egami; G. H. Rieke; S. P. Willner; D. Rigopoulou; A. Alonso-Herrero; P. Barmby; L. Bei; H. Dole; C. W. Engelbracht; G. G. Fazio; E. Le Floc'h; K. D. Gordon; T. R. Greve; D. C. Hines; J. -S. Huang; K. A. Misselt; S. Miyazaki; J. E. Morrison; C. Papovich; P. G. Perez-Gonzalez; M. J. Rieke; J. Rigby; G. Wilson
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eye 55
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We present sub-millimeter statistical detections of galaxies discovered in the 5'x5' Spitzer Early Release Observations (to 4-15 microJy 5 sigma at 3.6-8 microns, 170 microJy at 24 microns) through a stacking analysis of our reanalysed SCUBA 8mJy survey maps, and a Spitzer identification of a new sub-millimeter point source in the 8mJy survey region. For sources detected at 5.8 or 8 microns (154 and 111 sources respectively), we detect positive skews in the sub-millimeter flux distributions at...
Source: http://arxiv.org/abs/astro-ph/0406028v1
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51
Jul 20, 2013
07/13
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E. Egami; H. Dole; J. -S. Huang; P. Perez-Gonzalez; E. Le Floc'h; C. Papovich; P. Barmby; R. J. Ivison; S. Serjeant; A. Mortier; D. T. Frayer; D. Rigopoulou; G. Lagache; G. H. Rieke; S. P. Willner; A. Alonso-Herrero; L. Bai; C. W. Engelbracht; G. G. Fazio; K. D. Gordon; D. C. Hines; K. A. Misselt; S. Miyazaki; J. E. Morrison; M. J. Rieke; J. R. Rigby; G. Wilson
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eye 51
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We present Spitzer IRAC (3.6, 4.5, 5.8, 8.0 um) and MIPS (24 um) observations of the SCUBA submillimeter sources and uJy VLA radio sources in a 5'x5' area in the Lockman Hole East region. Out of the ~40 SCUBA/VLA sources in the field, Spitzer counterparts were detected for nearly all except for the few low-weight SCUBA detections. We show that the majority (80-90%) of the detected sources are cold (i.e., starburst-like) infrared-luminous galaxies (L_{IR} > 10^{11} Lsun) at redshift 0.5
Source: http://arxiv.org/abs/astro-ph/0406359v1
