IRAS maps of galactic emission and the zodiacal bands

Rowan‐Robinson, M.; Hughes, Joanne; Jones, Mark; Leech, K.; Vedi, K.; Walker, D. W.

doi:10.1093/mnras/249.4.729

Cited by 60 publications

(47 citation statements)

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“…Finally, we agree with the Teplitz et al (2011) measurements performed with the infrared spectrograph (IRS) onboard the Spitzer space telescope. We compare our counts to Hacking & Houck (1987), Lonsdale et al (1990), Rowan-Robinson et al (1990), Saunders et al (1990), Gregorich et al (1995), and Bertin et al (1997) at 60 μm from IRAS data. There are disagreements between the different observations and some error bars may be underestimated, but our model globally agrees with the cloud of points.…”

Section: Comparison Between the Model And The Observed Counts Not Usementioning

confidence: 99%

Modeling the evolution of infrared galaxies: a parametric backward evolution model

Béthermin

Dole

Lagache

et al. 2011

A&A

148

312

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Aims. We attempt to model the infrared galaxy evolution in as simple a way as possible and reproduce statistical properties such as the number counts between 15 μm and 1.1 mm, the luminosity functions, and the redshift distributions. We then use the fitted model to interpret observations from Spitzer, AKARI, BLAST, LABOCA, AzTEC, SPT, and Herschel, and make predictions for Planck and future experiments such as CCAT or SPICA. Methods. This model uses an evolution in density and luminosity of the luminosity function parametrized by broken power-laws with two breaks at redshift ∼0.9 and 2, and contains the two populations of the Lagache model: normal and starburst galaxies. We also take into account the effect of the strong lensing of high-redshift sub-millimeter galaxies. This effect is significant in the sub-mm and mm range near 50 mJy. It has 13 free parameters and eight additional calibration parameters. We fit the parameters to the IRAS, Spitzer, Herschel, and AzTEC measurements with a Monte Carlo Markov chain. Results. The model adjusted to deep counts at key wavelengths reproduces the counts from mid-infrared to millimeter wavelengths, as well as the mid-infrared luminosity functions. We discuss the contribution to both the cosmic infrared background (CIB) and the infrared luminosity density of the different populations. We also estimate the effect of the lensing on the number counts, and discuss the discovery by the South Pole Telescope (SPT) of a very bright population lying at high redshift. We predict the contribution of the lensed sources to the Planck number counts, the confusion level for future missions using a P(D) formalism, and the Universe opacity to TeV photons caused by the CIB. Material of the model (software, tables and predictions) is available online .

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Section: Comparison Between the Model And The Observed Counts Not Usementioning

confidence: 99%

Modeling the evolution of infrared galaxies: a parametric backward evolution model

Béthermin

Dole

Lagache

et al. 2011

A&A

148

312

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“…The shown fit to the Zodiacal light includes thermal emission from asteroidal, cometary and interstellar dust in the solar system [211]. Most observations of the Zodiacal light beyond ∼ 10 µm are carried out beyond the atmosphere, from rockets [154] and from instruments on the satellites IRAS [12,212,213], COBE [78,197,104], IRTS [153] and ISO [197]. A compilation of all observations of the sky brightness until 1997 was prepared by Christoph Leinert and other members of Commission 21 Light of the Night Sky of the International Astronomical Union [125].…”

Section: Astronomical Observations Of Zodiacal Light and Cometsmentioning

confidence: 99%

Dust in the planetary system: Dust interactions in space plasmas of the solar system

Mann¹,

Meyer‐Vernet²,

Czechowski³

2014

Physics Reports

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Cosmic dust particles are small solid objects observed in the solar planetary system and in many astronomical objects like the surrounding of stars, the interstellar and even the intergalactic medium. In the solar system the dust is best observed and most often found within the region of the orbits of terrestrial planets where the dust interactions and dynamics are observed directly from spacecraft. Dust is observed in space near Earth and also enters the atmosphere of the Earth where it takes part in physical and chemical processes. Hence space offers a laboratory to study dust plasma interactions and dust dynamics. A recent example is the observation of nanodust of sizes smaller than 10 nm. We outline the theoretical considerations on which our knowledge of dust electric charges in space plasmas are founded. We discuss the dynamics of the dust particles and show how the small charged particles are accelerated by the solar wind that carries a magnetic field. Finally, as examples for the space observation of cosmic dust interactions, we describe the first detection of fast nanodust in the solar wind near Earth orbit and the first bi-static observations of PMSE, the radar echoes that are observed in the Earth ionosphere in the presence of charged dust.

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“…Examples for such, to varying degrees physical or simply parameterising models are to be found, e.g. in Röser & Staude (1978), Murdock & Price (1985), Deul & Wolstencroft (1988), Rowan-Robinson et al (1990), Reach Table 16. Zodiacal light brightness observed from the Earth (in S10 ) at 500 nm.…”

Section: Heliocentric Dependencementioning

confidence: 99%

The 1997 reference of diffuse night sky brightness

Leinert

Bowyer

Haikala

et al. 1998

Astron. Astrophys. Suppl. Ser.

447

436

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Abstract. In the following we present material in tabular and graphical form, with the aim to allow the nonspecialist to obtain a realistic estimate of the diffuse night sky brightness over a wide range of wavelengths from the far UV longward of Lyα to the far-infrared. At the same time the data are to provide a reference for cases in which background brightness has to be discussed, including the planning for space observations and the issue of protection of observatory sites. We try to give a critical presentation of the status at the beginning of 1997.

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IRAS maps of galactic emission and the zodiacal bands

Cited by 60 publications

References 0 publications

Modeling the evolution of infrared galaxies: a parametric backward evolution model

Modeling the evolution of infrared galaxies: a parametric backward evolution model

Dust in the planetary system: Dust interactions in space plasmas of the solar system

The 1997 reference of diffuse night sky brightness

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