BOOMERANG returns

Philip Mauskopf, P. A R Ade, A. Balbi, P. Cabella, G. De Gasperis, P. Natoli, N. Vittorio, J. J. Bock, V. V. Hristov, W. C. Jones, A. E. Lange, J. R. Bond, C. R. Contaldi, J. J. Borrill, A. Boscaleri, B. P. Crill, P. de Bernardis, G. De Troia, A. Iacoangeli, S. MasiA. Melchiorri, F. Nati, F. Piacentini, G. Polenta, S. Ricciardi, A. de Oliveira-Costa, M. Tegmark, G. di Stefano, G. Romeo, K. Ganga, E. Hivon, A. H. Jaffe, J. E. Ruhl, T. S. Kisner, T. Montroy, E. Torbet, C. Mactavish, C. B. Netterfield, E. Pascale, D. Pogosyan, S. Prunet

Research output: Contribution to journalArticle

1 Citation (Scopus)

Abstract

BOOMERANG was one of the first experiments to map large areas of the cosmic microwave background (CMB) with high signal-to-noise during a long duration balloon (LDB) flight in 1998/99. BOOMERANG uses bolometric detectors measuring frequency bands from 90 to 400 GHz, a frequency range that complements the lower frequency range of experiments using HEMT amplifiers such as DASI and WMAP. Here, we discuss the status of the analysis of the B98 data including initial comparison of the B98 data with WMAP and component separation of the B98 maps in order to measure the Sunyaev-Zel'dovich effect. Finally, we describe the second LDB flight of the BOOMERANG telescope in January, 2003 with a receiver designed to map the polarisation of the CMB.

Original languageEnglish (US)
Pages (from-to)733-740
Number of pages8
JournalNew Astronomy Reviews
Volume47
Issue number8-0
DOIs
StatePublished - Nov 2003
Externally publishedYes

Fingerprint

balloon flight
frequency ranges
flight
microwaves
high electron mobility transistors
complement
polarization
receivers
amplifiers
experiment
telescopes
low frequencies
detectors
microwave
detector
analysis
comparison
effect
measuring

Keywords

  • CMB
  • CMB polarisation
  • Component separation
  • Sunyaev-Zel'dovich effect

ASJC Scopus subject areas

  • Astronomy and Astrophysics

Cite this

Mauskopf, P., Ade, P. A. R., Balbi, A., Cabella, P., De Gasperis, G., Natoli, P., ... Prunet, S. (2003). BOOMERANG returns. New Astronomy Reviews, 47(8-0), 733-740. https://doi.org/10.1016/j.newar.2003.07.019

BOOMERANG returns. / Mauskopf, Philip; Ade, P. A R; Balbi, A.; Cabella, P.; De Gasperis, G.; Natoli, P.; Vittorio, N.; Bock, J. J.; Hristov, V. V.; Jones, W. C.; Lange, A. E.; Bond, J. R.; Contaldi, C. R.; Borrill, J. J.; Boscaleri, A.; Crill, B. P.; de Bernardis, P.; De Troia, G.; Iacoangeli, A.; Masi, S.; Melchiorri, A.; Nati, F.; Piacentini, F.; Polenta, G.; Ricciardi, S.; de Oliveira-Costa, A.; Tegmark, M.; di Stefano, G.; Romeo, G.; Ganga, K.; Hivon, E.; Jaffe, A. H.; Ruhl, J. E.; Kisner, T. S.; Montroy, T.; Torbet, E.; Mactavish, C.; Netterfield, C. B.; Pascale, E.; Pogosyan, D.; Prunet, S.

In: New Astronomy Reviews, Vol. 47, No. 8-0, 11.2003, p. 733-740.

Research output: Contribution to journalArticle

Mauskopf, P, Ade, PAR, Balbi, A, Cabella, P, De Gasperis, G, Natoli, P, Vittorio, N, Bock, JJ, Hristov, VV, Jones, WC, Lange, AE, Bond, JR, Contaldi, CR, Borrill, JJ, Boscaleri, A, Crill, BP, de Bernardis, P, De Troia, G, Iacoangeli, A, Masi, S, Melchiorri, A, Nati, F, Piacentini, F, Polenta, G, Ricciardi, S, de Oliveira-Costa, A, Tegmark, M, di Stefano, G, Romeo, G, Ganga, K, Hivon, E, Jaffe, AH, Ruhl, JE, Kisner, TS, Montroy, T, Torbet, E, Mactavish, C, Netterfield, CB, Pascale, E, Pogosyan, D & Prunet, S 2003, 'BOOMERANG returns', New Astronomy Reviews, vol. 47, no. 8-0, pp. 733-740. https://doi.org/10.1016/j.newar.2003.07.019
Mauskopf P, Ade PAR, Balbi A, Cabella P, De Gasperis G, Natoli P et al. BOOMERANG returns. New Astronomy Reviews. 2003 Nov;47(8-0):733-740. https://doi.org/10.1016/j.newar.2003.07.019
Mauskopf, Philip ; Ade, P. A R ; Balbi, A. ; Cabella, P. ; De Gasperis, G. ; Natoli, P. ; Vittorio, N. ; Bock, J. J. ; Hristov, V. V. ; Jones, W. C. ; Lange, A. E. ; Bond, J. R. ; Contaldi, C. R. ; Borrill, J. J. ; Boscaleri, A. ; Crill, B. P. ; de Bernardis, P. ; De Troia, G. ; Iacoangeli, A. ; Masi, S. ; Melchiorri, A. ; Nati, F. ; Piacentini, F. ; Polenta, G. ; Ricciardi, S. ; de Oliveira-Costa, A. ; Tegmark, M. ; di Stefano, G. ; Romeo, G. ; Ganga, K. ; Hivon, E. ; Jaffe, A. H. ; Ruhl, J. E. ; Kisner, T. S. ; Montroy, T. ; Torbet, E. ; Mactavish, C. ; Netterfield, C. B. ; Pascale, E. ; Pogosyan, D. ; Prunet, S. / BOOMERANG returns. In: New Astronomy Reviews. 2003 ; Vol. 47, No. 8-0. pp. 733-740.
@article{405676caf8ec46dea956833328118868,
title = "BOOMERANG returns",
abstract = "BOOMERANG was one of the first experiments to map large areas of the cosmic microwave background (CMB) with high signal-to-noise during a long duration balloon (LDB) flight in 1998/99. BOOMERANG uses bolometric detectors measuring frequency bands from 90 to 400 GHz, a frequency range that complements the lower frequency range of experiments using HEMT amplifiers such as DASI and WMAP. Here, we discuss the status of the analysis of the B98 data including initial comparison of the B98 data with WMAP and component separation of the B98 maps in order to measure the Sunyaev-Zel'dovich effect. Finally, we describe the second LDB flight of the BOOMERANG telescope in January, 2003 with a receiver designed to map the polarisation of the CMB.",
keywords = "CMB, CMB polarisation, Component separation, Sunyaev-Zel'dovich effect",
author = "Philip Mauskopf and Ade, {P. A R} and A. Balbi and P. Cabella and {De Gasperis}, G. and P. Natoli and N. Vittorio and Bock, {J. J.} and Hristov, {V. V.} and Jones, {W. C.} and Lange, {A. E.} and Bond, {J. R.} and Contaldi, {C. R.} and Borrill, {J. J.} and A. Boscaleri and Crill, {B. P.} and {de Bernardis}, P. and {De Troia}, G. and A. Iacoangeli and S. Masi and A. Melchiorri and F. Nati and F. Piacentini and G. Polenta and S. Ricciardi and {de Oliveira-Costa}, A. and M. Tegmark and {di Stefano}, G. and G. Romeo and K. Ganga and E. Hivon and Jaffe, {A. H.} and Ruhl, {J. E.} and Kisner, {T. S.} and T. Montroy and E. Torbet and C. Mactavish and Netterfield, {C. B.} and E. Pascale and D. Pogosyan and S. Prunet",
year = "2003",
month = "11",
doi = "10.1016/j.newar.2003.07.019",
language = "English (US)",
volume = "47",
pages = "733--740",
journal = "New Astronomy Reviews",
issn = "1387-6473",
publisher = "Elsevier",
number = "8-0",

}

TY - JOUR

T1 - BOOMERANG returns

AU - Mauskopf, Philip

AU - Ade, P. A R

AU - Balbi, A.

AU - Cabella, P.

AU - De Gasperis, G.

AU - Natoli, P.

AU - Vittorio, N.

AU - Bock, J. J.

AU - Hristov, V. V.

AU - Jones, W. C.

AU - Lange, A. E.

AU - Bond, J. R.

AU - Contaldi, C. R.

AU - Borrill, J. J.

AU - Boscaleri, A.

AU - Crill, B. P.

AU - de Bernardis, P.

AU - De Troia, G.

AU - Iacoangeli, A.

AU - Masi, S.

AU - Melchiorri, A.

AU - Nati, F.

AU - Piacentini, F.

AU - Polenta, G.

AU - Ricciardi, S.

AU - de Oliveira-Costa, A.

AU - Tegmark, M.

AU - di Stefano, G.

AU - Romeo, G.

AU - Ganga, K.

AU - Hivon, E.

AU - Jaffe, A. H.

AU - Ruhl, J. E.

AU - Kisner, T. S.

AU - Montroy, T.

AU - Torbet, E.

AU - Mactavish, C.

AU - Netterfield, C. B.

AU - Pascale, E.

AU - Pogosyan, D.

AU - Prunet, S.

PY - 2003/11

Y1 - 2003/11

N2 - BOOMERANG was one of the first experiments to map large areas of the cosmic microwave background (CMB) with high signal-to-noise during a long duration balloon (LDB) flight in 1998/99. BOOMERANG uses bolometric detectors measuring frequency bands from 90 to 400 GHz, a frequency range that complements the lower frequency range of experiments using HEMT amplifiers such as DASI and WMAP. Here, we discuss the status of the analysis of the B98 data including initial comparison of the B98 data with WMAP and component separation of the B98 maps in order to measure the Sunyaev-Zel'dovich effect. Finally, we describe the second LDB flight of the BOOMERANG telescope in January, 2003 with a receiver designed to map the polarisation of the CMB.

AB - BOOMERANG was one of the first experiments to map large areas of the cosmic microwave background (CMB) with high signal-to-noise during a long duration balloon (LDB) flight in 1998/99. BOOMERANG uses bolometric detectors measuring frequency bands from 90 to 400 GHz, a frequency range that complements the lower frequency range of experiments using HEMT amplifiers such as DASI and WMAP. Here, we discuss the status of the analysis of the B98 data including initial comparison of the B98 data with WMAP and component separation of the B98 maps in order to measure the Sunyaev-Zel'dovich effect. Finally, we describe the second LDB flight of the BOOMERANG telescope in January, 2003 with a receiver designed to map the polarisation of the CMB.

KW - CMB

KW - CMB polarisation

KW - Component separation

KW - Sunyaev-Zel'dovich effect

UR - http://www.scopus.com/inward/record.url?scp=0242267624&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0242267624&partnerID=8YFLogxK

U2 - 10.1016/j.newar.2003.07.019

DO - 10.1016/j.newar.2003.07.019

M3 - Article

AN - SCOPUS:0242267624

VL - 47

SP - 733

EP - 740

JO - New Astronomy Reviews

JF - New Astronomy Reviews

SN - 1387-6473

IS - 8-0

ER -