alx-ai/arxiv_papers · Datasets at Hugging Face

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[20] M.A. Ballester, quant-ph/0507073.
[21] D. Gross, “Finite Phase Space Methods in Quantum Information ”, Diploma
Thesis, Potsdam (2005). Available online at http://gross.qipc.org/diplom.pdf .
[22] S. Colin, J. Corbett, T. Durt and D. Gross, J. Opt. B: Quantum and Semicl.
Optics7, S778 (2005).
[23] C. Godsil and A. Roy, European J. Combin. ,30, 246 (2009). Also available as
quant-ph/0511004.
[24] S.D. Howard, A.R. Calderbank and W. Moran, EURASIP J. Appl. Sig. Pro-
cess.2006, 85865 (2006).
[25] A.J. Scott, J. Phys. A 39, 13507 (2006). Also available as quant-ph/0604049.
[26] T. Durt, quant-ph/0604117 (2006).
[27] S.T. Flammia, J. Phys. A 39, 13483 (2006). Also available as quant-
ph/0605050.
[28] M. Grassl, conference presentation at MAGMA 2006 Confer-
ence(Tehnische Universit¨ at Berlin, 2006). Available online at
http://magma.maths.usyd.edu.au/Magma/2006 .
[29] I.H. Kim, Quant. Inf. Comp. 8, 730 (2007). Also available as quant-
ph/0608024.
[30] D.M. Appleby, Opt. Spect. 103, 416 (2007). Also available as quant-
ph/0611260.
[31] L. Bos and S. Waldron, New Zealand J. Math. 36, 113 (2007).
[32] A. Roy and A.J. Scott, J. Math. Phys. 48, 072110 (2007). Also available as
quant-ph/0703025.55
[33] O. Albouy and M.R. Kibbler, Journal of Russian Laser Research 28, 429
(2007). Also available as arXiv:0704.0511.
[34] D.M. Appleby, H.B. Dang and C.A. Fuchs, arXiv:0707.2071.
[35] M. Khatirinejad, Journal of Algebraic Combinatorics 28, 333 (2008).
[36] B.G. Bodmann, P.G. Casazza, D. Edidin and R. Balan, Information Sci-
ences and Systems, CISS 2008, Proceedings of 42nd Annual Con ference, p. 721
(2008).
[37] M.R. Kibler, J. Phys. A 41, 375302 (2008). Also available as arXiv:0807.2837.
[38] I. Bengtsson and H. Granstr¨ om, Open Sys. Information Dyn. 16, 145 (2009).
Also available as arXiv:0808.2974.
[39] M. Grassl, conference presentation at Seeking SICs: A Workshop on Quantum
Frames and Designs (Perimeter Institute, Waterloo, 2008). Available online at
http://pirsa.org/08100069 .
[40] M. Grassl, Lecture Notes in Computer Science 5393, 89 (2008).
[41] M. Fickus, J. Fourier Anal. Appl. 15, 413 (2009).
[42] D.M. Appleby, Foundations of Probability and Physics-5, V¨ axj¨ o 2008, AI P
Conf. Proc. 1101, 223 (2009). Also available as arXiv:0905.1428.
[43] C.A. Fuchs and R. Schack, arXiv:0906.2187 (2009).
[44] D.M. Appleby, arXiv:0909.5233 (2009).
[45] D.M. Appleby, ˚A. Ericsson and C.A. Fuchs, arXiv:0910.2750 (2009).
[46] A.J. Scott and M. Grassl, arXiv:0910.5784 (2009).
[47] I. Bengtsson and K. ˙Zyczkowski, Geometry of Quantum States (Cambridge
University Press, Cambridge, 2006).
[48] C.A. Fuchs, quant-ph/0205039.
[49] P.O. Boykin, M. Sitharam, P.H. Tiep and P. Wocjan, Quantum Inf. Comput.
7, 371 (2007). Also available as quant-ph/0506089.
[50] N. Mukunda, Arvind, S. Chaturvedi and R. Simon, Phys. Rev. A 65, 012102
(2001). Also available as quant-ph/0107006.
[51] G.R. Goodson and R.A. Horn, Lin. Alg. App. 430, 1025 (2009).
[52] N. Jacobson, Lie Algebras (Dover Publications, New York, 1979).
[53] J.E. Humphreys, Introduction to Lie Algebras and Representation Theory
(Graduate Texts in Mathematics, Springer-Verlag, New York, 197 0).
[54] W. Fulton and J. Harris, Representation Theory (Graduate Texts in Mathe-
matics, Springer-Verlag, New York, 1991).
[55] A.O. Barut and R R¸ aczka, Theory of Group Representations and Applications
(World Scientiﬁc, Singapore, 1986).
[56] W.K. Wootters, Ann. Phys. (N.Y.) 176, 1 (1987).
[57] A. Vourdas, Rep. Prog. Phys. 67, 267 (2004).
arXiv:1001.0005v1 [astro-ph.CO] 30 Dec 2009Astronomy& Astrophysics manuscriptno.akari˙RXJ1716˙v5 c∝circlecopyrtESO 2018
October30,2018
Environmentaldependenceof 8 µmluminosityfunctionsof
galaxiesatz ∼0.8
Comparison between RXJ1716.4 +6708 andthe AKARI NEP deep ﬁeld.⋆,⋆⋆
Tomotsugu Goto1,2,⋆⋆⋆, Yusei Koyama3,T.Wada4,C.Pearson5,6,7,H.Matsuhara4,T.Takagi4, H.Shim8, M.Im8,
M.G.Lee8, H.Inami4,9,10,M.Malkan11, S.Okamura3,T.T.Takeuchi12, S.Serjeant7, T.Kodama2, T.Nakagawa4,
S.Oyabu4,Y.Ohyama13, H.M.Lee8, N.Hwang2, H.Hanami14, K.Imai15,and T.Ishigaki16
1Institute for Astronomy, University of Hawaii,2680 Woodla wnDrive, Honolulu, HI,96822, USA
e-mail:tomo@ifa.hawaii.edu
2National Astronomical Observatory, 2-21-1 Osawa,Mitaka, Tokyo, 181-8588,Japan
3Department of Astronomy, School of Science,The University of Tokyo, Tokyo113-0033, Japan
4Institute of Space and Astronautical Science, JapanAerosp ace Exploration Agency, Sagamihara,Kanagawa 229-8510
5Rutherford Appleton Laboratory, Chilton, Didcot,Oxfords hire OX110QX, UK
6Department of Physics,Universityof Lethbridge, 4401 Univ ersity Drive,Lethbridge, AlbertaT1J 1B1, Canada
7Astrophysics Group, Department of Physics, The OpenUniver sity, MiltonKeynes, MK76AA, UK
8Department of Physics& Astronomy, FPRD,Seoul National Uni versity, Shillim-Dong,Kwanak-Gu, Seoul 151-742, Korea
9Spitzer Science Center,California Institute ofTechnolog y, Pasadena, CA91125
10Department of Astronomical Science,The Graduate Universi tyfor Advanced Studies
11Department of Physicsand Astronomy, UCLA,Los Angeles, CA, 90095-1547 USA
12Institute for Advanced Research, Nagoya University, Furo- cho, Chikusa-ku, Nagoya 464-8601
13Academia Sinica,Institute of Astronomyand Astrophysics, Taiwan
14Physics Section,Facultyof Humanities and SocialSciences , Iwate University, Morioka, 020-8550
15TOMER&D Inc. Kawasaki, Kanagawa 2130012, Japan
16Asahikawa National College of Technology, 2-1-6 2-joShunk ohdai, Asahikawa-shi, Hokkaido 071-8142
Received September 15, 2009; accepted December 16, 2009
ABSTRACT
Aims.Weaim to reveal environmental dependence of infraredlumin osity functions (IR LFs)of galaxies at z ∼0.8 using the AKARI
satellite. AKARI’s wide ﬁeld of view and unique mid-IR ﬁlter s help us to construct restframe 8 µm LFs directly without relying on
SEDmodels.
Methods. We construct restframe 8 µm IR LFs in the cluster region RXJ1716.4 +6708 at z=0.81, and compare them with a blank
ﬁeld using the AKARI North Ecliptic Pole deep ﬁeld data at the same redshift. AKARI’s wide ﬁeld of view (10’ ×10’) is suitable to
investigate wide range of galaxy environments. AKARI’s 15 µm ﬁlter is advantageous here since it directly probes restfr ame 8µm at
z∼0.8, without relyingona large extrapolation based ona SEDﬁ t,which was the largestuncertainty inprevious work.
Results. We have found that cluster IR LFsat restframe 8 µm have a factor of 2.4smaller L∗and a steeper faint-end slope than that
of the ﬁeld. Conﬁrming this trend, we also found that faint-e nd slopes of the cluster LFs becomes ﬂatter and ﬂatter with de creasing
local galaxy density. These changes in LFs cannot be explain ed by a simple infall of ﬁeld galaxy population into a cluster . Physics
that canpreferentiallysuppress IR luminous galaxies inhi gh density regions is requiredtoexplain the observed resul ts.
Keywords. galaxies: evolution, galaxies:interactions, galaxies:s tarburst, galaxies:peculiar, galaxies:formation

[20] M.A. Ballester, quant-ph/0507073.

[21] D. Gross, “Finite Phase Space Methods in Quantum Information ”, Diploma

Thesis, Potsdam (2005). Available online at http://gross.qipc.org/diplom.pdf .

[22] S. Colin, J. Corbett, T. Durt and D. Gross, J. Opt. B: Quantum and Semicl.

Optics7, S778 (2005).

[23] C. Godsil and A. Roy, European J. Combin. ,30, 246 (2009). Also available as

quant-ph/0511004.

[24] S.D. Howard, A.R. Calderbank and W. Moran, EURASIP J. Appl. Sig. Pro-

cess.2006, 85865 (2006).

[25] A.J. Scott, J. Phys. A 39, 13507 (2006). Also available as quant-ph/0604049.

[26] T. Durt, quant-ph/0604117 (2006).

[27] S.T. Flammia, J. Phys. A 39, 13483 (2006). Also available as quant-

ph/0605050.

[28] M. Grassl, conference presentation at MAGMA 2006 Confer-

ence(Tehnische Universit¨ at Berlin, 2006). Available online at

http://magma.maths.usyd.edu.au/Magma/2006 .

[29] I.H. Kim, Quant. Inf. Comp. 8, 730 (2007). Also available as quant-

ph/0608024.

[30] D.M. Appleby, Opt. Spect. 103, 416 (2007). Also available as quant-

ph/0611260.

[31] L. Bos and S. Waldron, New Zealand J. Math. 36, 113 (2007).

[32] A. Roy and A.J. Scott, J. Math. Phys. 48, 072110 (2007). Also available as

quant-ph/0703025.55

[33] O. Albouy and M.R. Kibbler, Journal of Russian Laser Research 28, 429

(2007). Also available as arXiv:0704.0511.

[34] D.M. Appleby, H.B. Dang and C.A. Fuchs, arXiv:0707.2071.

[35] M. Khatirinejad, Journal of Algebraic Combinatorics 28, 333 (2008).

[36] B.G. Bodmann, P.G. Casazza, D. Edidin and R. Balan, Information Sci-

ences and Systems, CISS 2008, Proceedings of 42nd Annual Con ference, p. 721

(2008).

[37] M.R. Kibler, J. Phys. A 41, 375302 (2008). Also available as arXiv:0807.2837.

[38] I. Bengtsson and H. Granstr¨ om, Open Sys. Information Dyn. 16, 145 (2009).

Also available as arXiv:0808.2974.

[39] M. Grassl, conference presentation at Seeking SICs: A Workshop on Quantum

Frames and Designs (Perimeter Institute, Waterloo, 2008). Available online at

http://pirsa.org/08100069 .

[40] M. Grassl, Lecture Notes in Computer Science 5393, 89 (2008).

[41] M. Fickus, J. Fourier Anal. Appl. 15, 413 (2009).

[42] D.M. Appleby, Foundations of Probability and Physics-5, V¨ axj¨ o 2008, AI P

Conf. Proc. 1101, 223 (2009). Also available as arXiv:0905.1428.

[43] C.A. Fuchs and R. Schack, arXiv:0906.2187 (2009).

[44] D.M. Appleby, arXiv:0909.5233 (2009).

[45] D.M. Appleby, ˚A. Ericsson and C.A. Fuchs, arXiv:0910.2750 (2009).

[46] A.J. Scott and M. Grassl, arXiv:0910.5784 (2009).

[47] I. Bengtsson and K. ˙Zyczkowski, Geometry of Quantum States (Cambridge

University Press, Cambridge, 2006).

[48] C.A. Fuchs, quant-ph/0205039.

[49] P.O. Boykin, M. Sitharam, P.H. Tiep and P. Wocjan, Quantum Inf. Comput.

7, 371 (2007). Also available as quant-ph/0506089.

[50] N. Mukunda, Arvind, S. Chaturvedi and R. Simon, Phys. Rev. A 65, 012102

(2001). Also available as quant-ph/0107006.

[51] G.R. Goodson and R.A. Horn, Lin. Alg. App. 430, 1025 (2009).

[52] N. Jacobson, Lie Algebras (Dover Publications, New York, 1979).

[53] J.E. Humphreys, Introduction to Lie Algebras and Representation Theory

(Graduate Texts in Mathematics, Springer-Verlag, New York, 197 0).

[54] W. Fulton and J. Harris, Representation Theory (Graduate Texts in Mathe-

matics, Springer-Verlag, New York, 1991).

[55] A.O. Barut and R R¸ aczka, Theory of Group Representations and Applications

(World Scientiﬁc, Singapore, 1986).

[56] W.K. Wootters, Ann. Phys. (N.Y.) 176, 1 (1987).

[57] A. Vourdas, Rep. Prog. Phys. 67, 267 (2004).

arXiv:1001.0005v1 [astro-ph.CO] 30 Dec 2009Astronomy& Astrophysics manuscriptno.akari˙RXJ1716˙v5 c∝circlecopyrtESO 2018

October30,2018

Environmentaldependenceof 8 µmluminosityfunctionsof

galaxiesatz ∼0.8

Comparison between RXJ1716.4 +6708 andthe AKARI NEP deep ﬁeld.⋆,⋆⋆

Tomotsugu Goto1,2,⋆⋆⋆, Yusei Koyama3,T.Wada4,C.Pearson5,6,7,H.Matsuhara4,T.Takagi4, H.Shim8, M.Im8,

M.G.Lee8, H.Inami4,9,10,M.Malkan11, S.Okamura3,T.T.Takeuchi12, S.Serjeant7, T.Kodama2, T.Nakagawa4,

S.Oyabu4,Y.Ohyama13, H.M.Lee8, N.Hwang2, H.Hanami14, K.Imai15,and T.Ishigaki16

1Institute for Astronomy, University of Hawaii,2680 Woodla wnDrive, Honolulu, HI,96822, USA

e-mail:tomo@ifa.hawaii.edu

2National Astronomical Observatory, 2-21-1 Osawa,Mitaka, Tokyo, 181-8588,Japan

3Department of Astronomy, School of Science,The University of Tokyo, Tokyo113-0033, Japan

4Institute of Space and Astronautical Science, JapanAerosp ace Exploration Agency, Sagamihara,Kanagawa 229-8510

5Rutherford Appleton Laboratory, Chilton, Didcot,Oxfords hire OX110QX, UK

6Department of Physics,Universityof Lethbridge, 4401 Univ ersity Drive,Lethbridge, AlbertaT1J 1B1, Canada

7Astrophysics Group, Department of Physics, The OpenUniver sity, MiltonKeynes, MK76AA, UK

8Department of Physics& Astronomy, FPRD,Seoul National Uni versity, Shillim-Dong,Kwanak-Gu, Seoul 151-742, Korea

9Spitzer Science Center,California Institute ofTechnolog y, Pasadena, CA91125

10Department of Astronomical Science,The Graduate Universi tyfor Advanced Studies

11Department of Physicsand Astronomy, UCLA,Los Angeles, CA, 90095-1547 USA

12Institute for Advanced Research, Nagoya University, Furo- cho, Chikusa-ku, Nagoya 464-8601

13Academia Sinica,Institute of Astronomyand Astrophysics, Taiwan

14Physics Section,Facultyof Humanities and SocialSciences , Iwate University, Morioka, 020-8550

15TOMER&D Inc. Kawasaki, Kanagawa 2130012, Japan

16Asahikawa National College of Technology, 2-1-6 2-joShunk ohdai, Asahikawa-shi, Hokkaido 071-8142

Received September 15, 2009; accepted December 16, 2009

ABSTRACT

Aims.Weaim to reveal environmental dependence of infraredlumin osity functions (IR LFs)of galaxies at z ∼0.8 using the AKARI

satellite. AKARI’s wide ﬁeld of view and unique mid-IR ﬁlter s help us to construct restframe 8 µm LFs directly without relying on

SEDmodels.

Methods. We construct restframe 8 µm IR LFs in the cluster region RXJ1716.4 +6708 at z=0.81, and compare them with a blank

ﬁeld using the AKARI North Ecliptic Pole deep ﬁeld data at the same redshift. AKARI’s wide ﬁeld of view (10’ ×10’) is suitable to

investigate wide range of galaxy environments. AKARI’s 15 µm ﬁlter is advantageous here since it directly probes restfr ame 8µm at

z∼0.8, without relyingona large extrapolation based ona SEDﬁ t,which was the largestuncertainty inprevious work.

Results. We have found that cluster IR LFsat restframe 8 µm have a factor of 2.4smaller L∗and a steeper faint-end slope than that

of the ﬁeld. Conﬁrming this trend, we also found that faint-e nd slopes of the cluster LFs becomes ﬂatter and ﬂatter with de creasing

local galaxy density. These changes in LFs cannot be explain ed by a simple infall of ﬁeld galaxy population into a cluster . Physics

that canpreferentiallysuppress IR luminous galaxies inhi gh density regions is requiredtoexplain the observed resul ts.

Keywords. galaxies: evolution, galaxies:interactions, galaxies:s tarburst, galaxies:peculiar, galaxies:formation