534:
17:
336:
Kirkpatrick, J. Davy; Cushing, Michael C.; Gelino, Christopher R.; Griffith, Roger L.; Skrutskie, Michael F.; Marsh, Kenneth A.; Wright, Edward L.; Mainzer, A.; Eisenhardt, Peter R.; McLean, Ian S.; Thompson, Maggie A.; Bauer, James M.; Benford, Dominic J.; Bridge, Carrie R.; Lake, Sean E.
274:
479:
220:
Simons, D. A.; Tokunaga, A. T. (February 2002). "The Mauna Kea
Observatories Near-Infrared Filter Set. I: Defining Optimal 1-5 $ \mu$ m Bandpasses".
108:
stars while mostly avoiding opacities from molecular bands and also has access to the 1080 nm He I line which is useful in the study of
171:
472:
129:
20:
Atmospheric windows in the infrared. The J band is the transmission window (1.1 to 1.4 μm) centred on 1.25 micrometres
465:
312:
196:
150:
77:
The J band is a frequent source of ground based observations since the wavelengths it covers pass through
580:
575:
980:
404:
402:
Oppenheimer, B. R. (2013). "Reconnaissance of the HR 8799 Exosolar System I: Near IR Spectroscopy".
875:
488:
273:
Pedretti, Ettore; Piacentini, S.; Corrielli, G.; Osellame, Roberto; Minardi, Stefano (2018-07-09).
925:
339:"The First Hundred Brown Dwarfs Discovered by the Wide-field Infrared Survey Explorer (WISE)"
51:
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8:
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109:
82:
25:
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949:
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33:
895:
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974:
905:
842:
823:
727:
661:
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380:
251:
41:
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277:. In Tuthill, Peter G.; Creech-Eakman, Michelle J.; Mérand, Antoine (eds.).
781:
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16:
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47:
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791:
567:
545:
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90:
67:
59:
959:
719:
519:
287:
275:"A six-apertures discrete beam combiners for J-band interferometry"
272:
243:
63:
422:
355:
828:
814:
55:
335:
852:
847:
837:
809:
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799:
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175:
71:
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590:
504:
93:
emission lines leading to relatively high photometric error.
78:
689:
684:
151:"Very Bright Stars in the 2MASS Point Source Catalog (PSC)"
124:
spectroscopy is also commonly used to observe and research
709:
148:
85:. The waveband does however suffer from contamination by
50:
is the brightest near-IR source in the sky with a J band
222:
54:
of −2.99. The next brightest stars in the J band are
279:Optical and Infrared Interferometry and Imaging VI
172:"Simbad object query:Jmag<-2 & Vmag>-9"
972:
219:
142:
473:
487:
329:
401:
343:The Astrophysical Journal Supplement Series
281:. Vol. 10701. SPIE. pp. 316–325.
549:
480:
466:
164:
421:
354:
286:
233:
395:
149:R. Cutri and M. Skrutskie (2009-09-07).
15:
153:. The Two Micron All Sky Survey at IPAC
973:
461:
36:(1.1 to 1.4 μm) centred on 1.25
197:"Infrared Astronomy Optical Filters"
13:
532:
14:
992:
96:It can be used to scrutinize the
34:atmospheric transmission window
266:
213:
189:
1:
135:
7:
581:Ultra-high-energy gamma ray
74:is the 9th brightest star.
10:
997:
576:Very-high-energy gamma ray
440:10.1088/0004-637X/768/1/24
373:10.1088/0067-0049/197/2/19
130:directly imaged exoplanets
934:
861:
790:
718:
670:
612:
589:
566:
495:
405:The Astrophysical Journal
489:Electromagnetic spectrum
537:
70:(−2.1). In the J band
21:
536:
178:Astronomical Database
19:
112:interactions around
622:Extreme ultraviolet
432:2013ApJ...768...24O
365:2011ApJS..197...19K
297:2018SPIE10701E..16P
201:www.andovercorp.com
627:Vacuum ultraviolet
538:
414:Cornell University
305:10.1117/12.2312033
110:circumstellar disk
83:atmospheric gasses
26:infrared astronomy
22:
968:
967:
672:Visible (optical)
988:
981:Infrared imaging
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235:astro-ph/0110594
228:(792): 169–179.
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337:(2011-12-01).
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244:10.1086/338544
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314:9781510619555
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127:
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115:
114:T-Tauri stars
111:
107:
103:
99:
94:
92:
88:
84:
80:
75:
73:
69:
65:
61:
57:
53:
49:
45:
43:
42:near-infrared
39:
35:
32:refers to an
31:
27:
18:
735:
540:
409:
403:
397:
346:
342:
331:
278:
268:
225:
221:
215:
204:. Retrieved
200:
191:
180:. Retrieved
166:
155:. Retrieved
144:
126:brown dwarfs
95:
76:
66:(−2.2), and
46:
29:
23:
955:Medium wave
632:Lyman-alpha
614:Ultraviolet
553:wavelengths
546:frequencies
510:Ultraviolet
98:photosphere
87:water vapor
38:micrometres
936:Wavelength
792:Microwaves
604:Hard X-ray
599:Soft X-ray
568:Gamma rays
500:Gamma rays
288:1809.01260
206:2023-04-01
182:2012-08-22
157:2011-12-28
136:References
106:supergiant
89:lines and
81:and other
48:Betelgeuse
950:Shortwave
945:Microwave
525:Microwave
423:1303.2627
381:0067-0049
356:1108.4677
349:(2): 19.
323:119458175
252:0004-6280
91:hydroxide
68:Aldebaran
60:R Doradus
52:magnitude
975:Category
960:Longwave
720:Infrared
520:Infrared
389:16850733
64:Arcturus
62:(−2.6),
58:(−2.7),
40:(in the
551:longer
544:higher
515:Visible
448:7173368
428:Bibcode
361:Bibcode
293:Bibcode
260:7880289
56:Antares
853:L band
848:S band
843:C band
838:X band
824:K band
810:Q band
805:V band
800:W band
705:Orange
700:Yellow
680:Violet
591:X-rays
505:X-rays
446:
416:: 24.
387:
379:
321:
311:
258:
250:
176:SIMBAD
122:K-band
79:clouds
72:Sirius
30:J band
28:, the
938:types
863:Radio
759:Bands
732:Bands
695:Green
530:Radio
444:S2CID
418:arXiv
412:(1).
385:S2CID
351:arXiv
319:S2CID
283:arXiv
256:S2CID
230:arXiv
116:. J,
102:giant
833:band
819:band
777:LWIR
755:MWIR
750:SWIR
690:Cyan
685:Blue
377:ISSN
309:ISBN
248:ISSN
128:and
120:and
104:and
926:ELF
921:SLF
916:ULF
911:VLF
891:VHF
886:UHF
881:SHF
876:EHF
871:THF
782:FIR
728:NIR
710:Red
662:UVA
657:UVB
652:UVC
647:NUV
642:MUV
637:FUV
436:doi
410:768
369:doi
347:197
301:doi
240:doi
226:114
100:of
44:).
24:In
977::
906:LF
901:MF
896:HF
769:,
765:,
761::
742:,
738:,
734::
442:.
434:.
426:.
408:.
383:.
375:.
367:.
359:.
345:.
341:.
317:.
307:.
299:.
291:.
254:.
246:.
238:.
224:.
199:.
174:.
132:.
831:u
829:K
817:a
815:K
773:)
771:N
767:M
763:L
757:(
746:)
744:H
740:K
736:J
730:(
556:→
542:←
481:e
474:t
467:v
450:.
438::
430::
420::
391:.
371::
363::
353::
325:.
303::
295::
285::
262:.
242::
232::
209:.
185:.
160:.
118:H
Text is available under the Creative Commons Attribution-ShareAlike License. Additional terms may apply.
