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K band (infrared)

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used in astronomy are sets of filters or detectors that have well-defined windows of absorption, based around a central peak detection frequency and where the edges of the detection window are typically reported where sensitivity drops below 50% of peak. Various organizations have defined systems
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Practical Handbook on Image Processing for Scientific and Technical Applications
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with various peak frequencies and cutoffs in the K band, including K
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Table 1., Filter sets used at Mauna Kea and the South Pole.
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are typically preferred for observing in this band.
94:"Specifications for Astronomical Infrared Filters" 178:Monthly Notices of the Royal Astronomical Society 916: 100:. Institute for Astronomy, University of Hawaii 899: 842: 218: 151:. Materials Research Forum LLC. p. 138. 232: 906: 892: 849: 835: 294:        225: 211: 189: 171: 138: 111: 92:Tokunaga, Alan T. (September 10, 2001). 91: 917: 206: 144: 117: 858: 801: 148:Detectors and Sources for THz and IR 13: 277: 85: 14: 951: 862: 805: 785: 773: 761: 749: 737: 725: 145:Sizov, Fedir F. (May 5, 2020). 118:Jahne, Bernd (March 15, 2004). 26:atmospheric transmission window 165: 1: 78: 878:. You can help Knowledge by 821:. You can help Knowledge by 7: 326:Ultra-high-energy gamma ray 66: 10: 956: 857: 800: 321:Very-high-energy gamma ray 679: 606: 535: 463: 415: 357: 334: 311: 240: 124:. RC Press. p. 109. 925:Electromagnetic spectrum 234:Electromagnetic spectrum 172:Jun Zhang (June 2023). 874:-related article is a 817:-related article is a 282: 281: 191:10.1093/mnras/stad775 36:136 THz range). 28:centered on 2.2  367:Extreme ultraviolet 48:Photometric systems 372:Vacuum ultraviolet 283: 98:www.ifa.hawaii.edu 73:Absolute magnitude 18:infrared astronomy 887: 886: 830: 829: 713: 712: 417:Visible (optical) 947: 930:Infrared imaging 908: 901: 894: 866: 859: 851: 844: 837: 809: 802: 790: 789: 788: 778: 777: 776: 766: 765: 764: 754: 753: 742: 741: 740: 730: 729: 721: 304: 302: 295: 288: 227: 220: 213: 204: 203: 197: 195: 193: 184:(4): 5624–5635. 169: 163: 162: 142: 136: 135: 115: 109: 108: 106: 105: 89: 54: 955: 954: 950: 949: 948: 946: 945: 944: 935:Astronomy stubs 915: 914: 913: 912: 856: 855: 798: 796: 786: 784: 774: 772: 762: 760: 748: 738: 736: 724: 716: 714: 709: 675: 602: 577: 563: 531: 459: 411: 353: 330: 307: 300: 293: 286: 284: 236: 231: 201: 200: 170: 166: 159: 143: 139: 132: 116: 112: 103: 101: 90: 86: 81: 69: 62: 58: 52: 12: 11: 5: 953: 943: 942: 937: 932: 927: 911: 910: 903: 896: 888: 885: 884: 867: 854: 853: 846: 839: 831: 828: 827: 810: 795: 794: 782: 770: 758: 746: 734: 711: 710: 708: 707: 702: 697: 692: 686: 684: 677: 676: 674: 673: 668: 663: 658: 653: 648: 643: 638: 633: 628: 623: 618: 612: 610: 604: 603: 601: 600: 595: 590: 585: 580: 575: 571: 566: 561: 557: 552: 547: 541: 539: 533: 532: 530: 529: 524: 519: 497: 492: 469: 467: 461: 460: 458: 457: 452: 447: 442: 437: 432: 427: 421: 419: 413: 412: 410: 409: 404: 399: 394: 389: 384: 379: 374: 369: 363: 361: 355: 354: 352: 351: 346: 340: 338: 332: 331: 329: 328: 323: 317: 315: 309: 308: 306: 305: 272: 267: 262: 257: 252: 247: 241: 238: 237: 230: 229: 222: 215: 207: 199: 198: 164: 157: 137: 130: 110: 83: 82: 80: 77: 76: 75: 68: 65: 60: 56: 9: 6: 4: 3: 2: 952: 941: 940:Physics stubs 938: 936: 933: 931: 928: 926: 923: 922: 920: 909: 904: 902: 897: 895: 890: 889: 883: 881: 877: 873: 868: 865: 861: 860: 852: 847: 845: 840: 838: 833: 832: 826: 824: 820: 816: 811: 808: 804: 803: 799: 793: 783: 781: 771: 769: 759: 757: 752: 747: 745: 735: 733: 728: 723: 722: 719: 706: 703: 701: 698: 696: 693: 691: 688: 687: 685: 682: 678: 672: 669: 667: 664: 662: 659: 657: 654: 652: 649: 647: 644: 642: 639: 637: 634: 632: 629: 627: 624: 622: 619: 617: 614: 613: 611: 609: 605: 599: 596: 594: 591: 589: 586: 584: 581: 579: 572: 570: 567: 565: 558: 556: 553: 551: 548: 546: 543: 542: 540: 538: 534: 528: 525: 523: 520: 517: 513: 509: 505: 501: 498: 496: 493: 490: 486: 482: 478: 474: 471: 470: 468: 466: 462: 456: 453: 451: 448: 446: 443: 441: 438: 436: 433: 431: 428: 426: 423: 422: 420: 418: 414: 408: 405: 403: 400: 398: 395: 393: 390: 388: 385: 383: 380: 378: 375: 373: 370: 368: 365: 364: 362: 360: 356: 350: 347: 345: 342: 341: 339: 337: 333: 327: 324: 322: 319: 318: 316: 314: 310: 303: 299: 292: 280: 276: 273: 271: 268: 266: 263: 261: 258: 256: 253: 251: 248: 246: 243: 242: 239: 235: 228: 223: 221: 216: 214: 209: 208: 205: 192: 187: 183: 179: 175: 168: 160: 158:9781644900758 154: 150: 149: 141: 133: 131:9780849390302 127: 123: 122: 114: 99: 95: 88: 84: 74: 71: 70: 64: 49: 45: 43: 39: 35: 34:near-infrared 31: 27: 23: 19: 880:expanding it 869: 823:expanding it 812: 797: 792:Solar System 484: 285: 181: 177: 167: 147: 140: 120: 113: 102:. Retrieved 97: 87: 46: 21: 15: 780:Outer space 768:Spaceflight 700:Medium wave 377:Lyman-alpha 359:Ultraviolet 298:wavelengths 291:frequencies 255:Ultraviolet 919:Categories 681:Wavelength 537:Microwaves 349:Hard X-ray 344:Soft X-ray 313:Gamma rays 245:Gamma rays 104:2021-11-05 79:References 815:astronomy 744:Astronomy 695:Shortwave 690:Microwave 270:Microwave 42:detectors 705:Longwave 465:Infrared 265:Infrared 67:See also 32:(in the 872:physics 732:Physics 718:Portals 296:longer 289:higher 260:Visible 59:, and K 55:, and K 40:-based 598:L band 593:S band 588:C band 583:X band 569:K band 555:Q band 550:V band 545:W band 450:Orange 445:Yellow 425:Violet 336:X-rays 250:X-rays 155:  128:  38:HgCdTe 24:is an 22:K band 20:, the 870:This 813:This 756:Stars 683:types 608:Radio 504:Bands 477:Bands 440:Green 275:Radio 876:stub 819:stub 578:band 564:band 522:LWIR 500:MWIR 495:SWIR 435:Cyan 430:Blue 153:ISBN 126:ISBN 61:dark 671:ELF 666:SLF 661:ULF 656:VLF 636:VHF 631:UHF 626:SHF 621:EHF 616:THF 527:FIR 473:NIR 455:Red 407:UVA 402:UVB 397:UVC 392:NUV 387:MUV 382:FUV 186:doi 182:521 16:In 921:: 651:LF 646:MF 641:HF 514:, 510:, 506:: 487:, 483:, 479:: 180:. 176:. 96:. 63:. 30:μm 907:e 900:t 893:v 882:. 850:e 843:t 836:v 825:. 720:: 576:u 574:K 562:a 560:K 518:) 516:N 512:M 508:L 502:( 491:) 489:H 485:K 481:J 475:( 301:→ 287:← 226:e 219:t 212:v 194:. 188:: 161:. 134:. 107:. 57:S 53:′

Index

infrared astronomy
atmospheric transmission window
μm
near-infrared
HgCdTe
detectors
Photometric systems
Absolute magnitude
"Specifications for Astronomical Infrared Filters"
Practical Handbook on Image Processing for Scientific and Technical Applications
ISBN
9780849390302
Detectors and Sources for THz and IR
ISBN
9781644900758
"Sky-brightness measurements in J, H, and Ks bands at DOME A with NISBM and early results"
doi
10.1093/mnras/stad775
v
t
e
Electromagnetic spectrum
Gamma rays
X-rays
Ultraviolet
Visible
Infrared
Microwave
Radio

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