Populations behind the source-subtracted cosmic infrared background anisotropies

Alexander Kashlinsky; R. G. Arendt; M. Ashby; F. Atrio-Barandela; V. Bromm; N. Cappelluti; S. Clesse; A. Comastri; G. Fazio; S. Driver; A. Ferrara; A. Finoguenov; J. Garcia-Bellido; D. Fixsen; G. Hasinger; K. Helgason; R. J. Hill; R. Jansen; J. Kruk; J. Mather; P. Natarajan; N. Odegard; M. Ricotti; M. Sahlen; E. Switzer; R. Windhorst; E. Wollack; Bin Yue

Populations behind the source-subtracted cosmic infrared background anisotropies

Alexander Kashlinsky, R. G. Arendt, M. Ashby, F. Atrio-Barandela, V. Bromm, N. Cappelluti, S. Clesse, A. Comastri, G. Fazio, S. Driver, A. Ferrara, A. Finoguenov, J. Garcia-Bellido, D. Fixsen, G. Hasinger, K. Helgason, R. J. Hill, R. Jansen, J. Kruk, J. MatherP. Natarajan, N. Odegard, M. Ricotti, M. Sahlen, E. Switzer, R. Windhorst, E. Wollack, Bin Yue

Research output: Contribution to journal › Article › peer-review

Abstract

Source-subtracted CIB fluctuations cannot be explained by known galaxy populations and appear highly coherent with unresolved CXB from significantly abundant accreting BHs. Characterizing the CIB with high accuracy, and constraining the nature of the new populations would produce critically important cosmological information in the next decade.

Original language	English
Pages (from-to)	37
Journal	American Astronomical Society. Bulletin
Volume	51
Issue number	3
Publication status	Published - 31 May 2019
Event	Decadal Survey on Astronomy and Astrophysics : Division on Engineering and Physical Sciences - , United States Duration: 8 Oct 2019 → … https://sites.nationalacademies.org/DEPS/astro2020/

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Kashlinsky, A., Arendt, R. G., Ashby, M., Atrio-Barandela, F., Bromm, V., Cappelluti, N., Clesse, S., Comastri, A., Fazio, G., Driver, S., Ferrara, A., Finoguenov, A., Garcia-Bellido, J., Fixsen, D., Hasinger, G., Helgason, K., Hill, R. J., Jansen, R., Kruk, J., ... Yue, B. (2019). Populations behind the source-subtracted cosmic infrared background anisotropies. American Astronomical Society. Bulletin, 51(3), 37. http://adsabs.harvard.edu/abs/2019BAAS...51c..37K

@article{a01dfd627f534b5bb3a31dd4b7fdbe26,

title = "Populations behind the source-subtracted cosmic infrared background anisotropies",

abstract = "Source-subtracted CIB fluctuations cannot be explained by known galaxy populations and appear highly coherent with unresolved CXB from significantly abundant accreting BHs. Characterizing the CIB with high accuracy, and constraining the nature of the new populations would produce critically important cosmological information in the next decade.",

author = "Alexander Kashlinsky and Arendt, {R. G.} and M. Ashby and F. Atrio-Barandela and V. Bromm and N. Cappelluti and S. Clesse and A. Comastri and G. Fazio and S. Driver and A. Ferrara and A. Finoguenov and J. Garcia-Bellido and D. Fixsen and G. Hasinger and K. Helgason and Hill, {R. J.} and R. Jansen and J. Kruk and J. Mather and P. Natarajan and N. Odegard and M. Ricotti and M. Sahlen and E. Switzer and R. Windhorst and E. Wollack and Bin Yue",

year = "2019",

month = may,

day = "31",

language = "English",

volume = "51",

pages = "37",

journal = "American Astronomical Society. Bulletin",

issn = "0002-7537",

publisher = "American astronomical society",

number = "3",

note = "Decadal Survey on Astronomy and Astrophysics : Division on Engineering and Physical Sciences, Astro2020 ; Conference date: 08-10-2019",

url = "https://sites.nationalacademies.org/DEPS/astro2020/",

}

Kashlinsky, A, Arendt, RG, Ashby, M, Atrio-Barandela, F, Bromm, V, Cappelluti, N, Clesse, S, Comastri, A, Fazio, G, Driver, S, Ferrara, A, Finoguenov, A, Garcia-Bellido, J, Fixsen, D, Hasinger, G, Helgason, K, Hill, RJ, Jansen, R, Kruk, J, Mather, J, Natarajan, P, Odegard, N, Ricotti, M, Sahlen, M, Switzer, E, Windhorst, R, Wollack, E & Yue, B 2019, 'Populations behind the source-subtracted cosmic infrared background anisotropies', American Astronomical Society. Bulletin, vol. 51, no. 3, pp. 37. <http://adsabs.harvard.edu/abs/2019BAAS...51c..37K>

TY - JOUR

T1 - Populations behind the source-subtracted cosmic infrared background anisotropies

AU - Kashlinsky, Alexander

AU - Arendt, R. G.

AU - Ashby, M.

AU - Atrio-Barandela, F.

AU - Bromm, V.

AU - Cappelluti, N.

AU - Clesse, S.

AU - Comastri, A.

AU - Fazio, G.

AU - Driver, S.

AU - Ferrara, A.

AU - Finoguenov, A.

AU - Garcia-Bellido, J.

AU - Fixsen, D.

AU - Hasinger, G.

AU - Helgason, K.

AU - Hill, R. J.

AU - Jansen, R.

AU - Kruk, J.

AU - Mather, J.

AU - Natarajan, P.

AU - Odegard, N.

AU - Ricotti, M.

AU - Sahlen, M.

AU - Switzer, E.

AU - Windhorst, R.

AU - Wollack, E.

AU - Yue, Bin

PY - 2019/5/31

Y1 - 2019/5/31

N2 - Source-subtracted CIB fluctuations cannot be explained by known galaxy populations and appear highly coherent with unresolved CXB from significantly abundant accreting BHs. Characterizing the CIB with high accuracy, and constraining the nature of the new populations would produce critically important cosmological information in the next decade.

AB - Source-subtracted CIB fluctuations cannot be explained by known galaxy populations and appear highly coherent with unresolved CXB from significantly abundant accreting BHs. Characterizing the CIB with high accuracy, and constraining the nature of the new populations would produce critically important cosmological information in the next decade.

M3 - Article

SN - 0002-7537

VL - 51

SP - 37

JO - American Astronomical Society. Bulletin

JF - American Astronomical Society. Bulletin

IS - 3

T2 - Decadal Survey on Astronomy and Astrophysics

Y2 - 8 October 2019

ER -

Populations behind the source-subtracted cosmic infrared background anisotropies

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