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Arcminute Cosmology Bolometer Array Receiver

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The ACBAR 145 GHz measurements were the most precise high multipole measurements of the CMB at the time.
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Reichardt, C. L.; et al. (2009). "High resolution CMB power spectrum from the complete ACBAR data set".
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This article about a specific observatory, telescope or astronomical instrument is a
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Measure the anisotropy of the Cosmic microwave background
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Location of Arcminute Cosmology Bolometer Array Receiver
733: 680: 483: 427: 389: 380: 324: 182:was an experiment to measure the anisotropy of the 106: 84: 74: 32: 24: 753: 700: 284: 8: 20:Arcminute Cosmology Bolometer Array Receiver 19: 300:Cosmic microwave background radiation (CMB) 760: 746: 707: 693: 386: 291: 277: 269: 127: 97: 66: 18: 784:Astronomical experiments in the Antarctic 231: 779:Cosmic microwave background experiments 199:Cosmic microwave background experiments 89:cosmic microwave background experiment 7: 718: 716: 661: 659: 732:. You can help Knowledge (XXG) by 679:. You can help Knowledge (XXG) by 14: 720: 663: 147: 140: 794:Astronomical observatory stubs 1: 506:Arcminute Microkelvin Imager 250:10.1088/0004-637X/694/2/1200 581:Mobile Anisotropy Telescope 541:Cosmic Anisotropy Telescope 501:Atacama Cosmology Telescope 186:. It was active 2000-2008. 184:Cosmic microwave background 80:145 GHz (2.07 mm) 810: 715: 658: 311:Discovery of CMB radiation 363: 316:Timeline of CMB astronomy 306: 219:The Astrophysical Journal 166: 135: 789:Physical cosmology stubs 546:Cosmic Background Imager 352:Sunyaev–Zeldovich effect 204:Observational cosmology 675:-related article is a 28:Antarctic Treaty area 626:South Pole Telescope 370:image (2018) of the 85:Telescope style 526:BICEP (1,2,3,Array) 242:2009ApJ...694.1200R 50: /  21: 673:physical cosmology 621:Simons Observatory 357:Thomson scattering 347:Sachs–Wolfe effect 741: 740: 688: 687: 653: 652: 649: 648: 337:Diffusion damping 177: 176: 801: 762: 755: 748: 724: 717: 709: 702: 695: 667: 660: 641:Very Small Array 387: 293: 286: 279: 270: 253: 235: 226:(2): 1200–1219. 170:edit on Wikidata 151: 150: 144: 131: 126: 123: 121: 119: 117: 115: 113: 102: 101: 70: 65: 64: 62: 61: 60: 55: 54:89.9917°S 44.5°W 51: 48: 47: 46: 43: 22: 809: 808: 804: 803: 802: 800: 799: 798: 769: 768: 767: 766: 714: 713: 656: 654: 645: 479: 423: 376: 375: 361: 332:Cosmic variance 320: 302: 297: 260: 215: 212: 210:Further reading 195: 173: 162: 161: 160: 159: 158: 154: 153: 152: 110: 96: 93:radio telescope 91: 59:-89.9917; -44.5 58: 56: 52: 49: 44: 41: 39: 37: 36: 17: 12: 11: 5: 807: 805: 797: 796: 791: 786: 781: 771: 770: 765: 764: 757: 750: 742: 739: 738: 725: 712: 711: 704: 697: 689: 686: 685: 668: 651: 650: 647: 646: 644: 643: 638: 633: 628: 623: 618: 613: 608: 603: 598: 593: 588: 583: 578: 573: 568: 563: 558: 553: 548: 543: 538: 533: 528: 523: 518: 513: 508: 503: 498: 493: 487: 485: 481: 480: 478: 477: 472: 467: 462: 457: 452: 447: 442: 437: 431: 429: 425: 424: 422: 421: 416: 411: 404: 399: 393: 391: 384: 378: 377: 365: 364: 362: 360: 359: 354: 349: 344: 339: 334: 328: 326: 322: 321: 319: 318: 313: 307: 304: 303: 298: 296: 295: 288: 281: 273: 267: 266: 264:ACBAR Homepage 259: 258:External links 256: 255: 254: 211: 208: 207: 206: 201: 194: 191: 175: 174: 167: 164: 163: 156: 155: 146: 145: 139: 138: 137: 136: 133: 132: 108: 104: 103: 86: 82: 81: 78: 72: 71: 34: 30: 29: 26: 15: 13: 10: 9: 6: 4: 3: 2: 806: 795: 792: 790: 787: 785: 782: 780: 777: 776: 774: 763: 758: 756: 751: 749: 744: 743: 737: 735: 731: 726: 723: 719: 710: 705: 703: 698: 696: 691: 690: 684: 682: 678: 674: 669: 666: 662: 657: 642: 639: 637: 634: 632: 629: 627: 624: 622: 619: 617: 614: 612: 609: 607: 604: 602: 599: 597: 594: 592: 589: 587: 584: 582: 579: 577: 574: 572: 569: 567: 564: 562: 559: 557: 554: 552: 549: 547: 544: 542: 539: 537: 534: 532: 529: 527: 524: 522: 519: 517: 514: 512: 509: 507: 504: 502: 499: 497: 494: 492: 489: 488: 486: 482: 476: 473: 471: 468: 466: 463: 461: 458: 456: 453: 451: 448: 446: 443: 441: 438: 436: 433: 432: 430: 426: 420: 417: 415: 412: 410: 409: 405: 403: 400: 398: 395: 394: 392: 388: 385: 383: 379: 373: 369: 358: 355: 353: 350: 348: 345: 343: 342:Recombination 340: 338: 335: 333: 330: 329: 327: 323: 317: 314: 312: 309: 308: 305: 301: 294: 289: 287: 282: 280: 275: 274: 271: 265: 262: 261: 257: 251: 247: 243: 239: 234: 229: 225: 221: 220: 214: 213: 209: 205: 202: 200: 197: 196: 192: 190: 187: 185: 181: 171: 165: 143: 134: 130: 125: 109: 105: 100: 94: 90: 87: 83: 79: 77: 73: 69: 63: 35: 31: 27: 23: 734:expanding it 727: 681:expanding it 670: 655: 495: 406: 223: 217: 188: 179: 178: 382:Experiments 57: / 33:Coordinates 25:Location(s) 773:Categories 576:LSPE/STRIP 571:Keck Array 566:GroundBIRD 556:COSMOSOMAS 450:LSPE/SWIPE 118:/holzapfel 76:Wavelength 45:44°30′00″W 42:89°59′30″S 616:Saskatoon 591:POLARBEAR 445:BOOMERanG 233:0801.1491 114:.berkeley 636:Tenerife 435:Archeops 414:RELIKT-1 402:LiteBIRD 193:See also 611:QUIJOTE 428:Balloon 366:4-year 325:Effects 238:Bibcode 107:Website 536:CAPMAP 484:Ground 475:TopHat 470:Spider 460:MAXIMA 440:ARCADE 408:Planck 368:Planck 122:/acbar 120:_group 95:  671:This 606:QUIET 601:QUBIC 551:CLASS 511:AMiBA 496:ACBAR 390:Space 228:arXiv 180:ACBAR 168:[ 730:stub 677:stub 596:QUaD 586:OVRO 561:DASI 531:BIMA 521:ATCA 516:APEX 465:QMAP 455:EBEX 419:WMAP 397:COBE 116:.edu 112:bolo 631:SZA 491:ABS 372:CMB 246:doi 224:694 775:: 244:. 236:. 222:. 761:e 754:t 747:v 736:. 708:e 701:t 694:v 683:. 374:. 292:e 285:t 278:v 252:. 248:: 240:: 230:: 172:] 124:/

Index

89°59′30″S 44°30′00″W / 89.9917°S 44.5°W / -89.9917; -44.5
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Wavelength
cosmic microwave background experiment
radio telescope
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bolo.berkeley.edu/holzapfel_group/acbar/
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Arcminute Cosmology Bolometer Array Receiver is located in Antarctica
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Cosmic microwave background
Cosmic microwave background experiments
Observational cosmology
The Astrophysical Journal
arXiv
0801.1491
Bibcode
2009ApJ...694.1200R
doi
10.1088/0004-637X/694/2/1200
ACBAR Homepage
v
t
e
Cosmic microwave background radiation (CMB)
Discovery of CMB radiation
Timeline of CMB astronomy
Cosmic variance
Diffusion damping
Recombination

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