A NICMOS-3 based spectrograph for near infrared astronomy
Abstract We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension. This accommod...
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| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1994 |
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| Umfang: |
2 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: Experimental astronomy - 1989, 3(1994) vom: Jan./Apr., Seite 189-190 |
| Übergeordnetes Werk: |
volume:3 ; year:1994 ; month:01/04 ; pages:189-190 ; extent:2 |
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| 520 | |a Abstract We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension. This accommodates the broad wavelength range while providing extensive coverage in the spatial dimension. | ||
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(DE-627)NLEJ193933551 DE-627 ger DE-627 rakwb eng A NICMOS-3 based spectrograph for near infrared astronomy 1994 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension. This accommodates the broad wavelength range while providing extensive coverage in the spatial dimension. Springer Online Journal Archives 1860-2002 Rudy, R. J. oth Dotan, Y. oth Warren, D. W. oth Young, R. M. oth in Experimental astronomy 1989 3(1994) vom: Jan./Apr., Seite 189-190 (DE-627)NLEJ188994203 (DE-600)2012330-9 1572-9508 nnns volume:3 year:1994 month:01/04 pages:189-190 extent:2 http://dx.doi.org/10.1007/BF00430161 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 3 1994 1/4 189-190 2 |
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(DE-627)NLEJ193933551 DE-627 ger DE-627 rakwb eng A NICMOS-3 based spectrograph for near infrared astronomy 1994 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension. This accommodates the broad wavelength range while providing extensive coverage in the spatial dimension. Springer Online Journal Archives 1860-2002 Rudy, R. J. oth Dotan, Y. oth Warren, D. W. oth Young, R. M. oth in Experimental astronomy 1989 3(1994) vom: Jan./Apr., Seite 189-190 (DE-627)NLEJ188994203 (DE-600)2012330-9 1572-9508 nnns volume:3 year:1994 month:01/04 pages:189-190 extent:2 http://dx.doi.org/10.1007/BF00430161 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 3 1994 1/4 189-190 2 |
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(DE-627)NLEJ193933551 DE-627 ger DE-627 rakwb eng A NICMOS-3 based spectrograph for near infrared astronomy 1994 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension. This accommodates the broad wavelength range while providing extensive coverage in the spatial dimension. Springer Online Journal Archives 1860-2002 Rudy, R. J. oth Dotan, Y. oth Warren, D. W. oth Young, R. M. oth in Experimental astronomy 1989 3(1994) vom: Jan./Apr., Seite 189-190 (DE-627)NLEJ188994203 (DE-600)2012330-9 1572-9508 nnns volume:3 year:1994 month:01/04 pages:189-190 extent:2 http://dx.doi.org/10.1007/BF00430161 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 3 1994 1/4 189-190 2 |
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(DE-627)NLEJ193933551 DE-627 ger DE-627 rakwb eng A NICMOS-3 based spectrograph for near infrared astronomy 1994 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension. This accommodates the broad wavelength range while providing extensive coverage in the spatial dimension. Springer Online Journal Archives 1860-2002 Rudy, R. J. oth Dotan, Y. oth Warren, D. W. oth Young, R. M. oth in Experimental astronomy 1989 3(1994) vom: Jan./Apr., Seite 189-190 (DE-627)NLEJ188994203 (DE-600)2012330-9 1572-9508 nnns volume:3 year:1994 month:01/04 pages:189-190 extent:2 http://dx.doi.org/10.1007/BF00430161 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 3 1994 1/4 189-190 2 |
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A NICMOS-3 based spectrograph for near infrared astronomy |
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Abstract We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension. This accommodates the broad wavelength range while providing extensive coverage in the spatial dimension. |
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Abstract We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension. This accommodates the broad wavelength range while providing extensive coverage in the spatial dimension. |
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Abstract We describe a design for a compact cooled spectrograph which incorporates two cameras and two collimators to achieve high throughput from 0.8 to 2.5μm. The spectrograph utilizes multiple NICMOS 3 arrays, specially mounted to minimize their separation in the spectral dimension. This accommodates the broad wavelength range while providing extensive coverage in the spatial dimension. |
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