In-orbit Performance of UVIT and First Results
Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the N...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Tandon, S. N. [verfasserIn] Hutchings, J. B. [verfasserIn] Ghosh, S. K. [verfasserIn] Subramaniam, A. [verfasserIn] Koshy, G. [verfasserIn] Girish, V. [verfasserIn] Kamath, P. U. [verfasserIn] Kathiravan, S. [verfasserIn] Kumar, A. [verfasserIn] Lancelot, J. P. [verfasserIn] Mahesh, P. K. [verfasserIn] Mohan, R. [verfasserIn] Murthy, J. [verfasserIn] Nagabhushana, S. [verfasserIn] Pati, A. K. [verfasserIn] Postma, J. [verfasserIn] Rao, N. Kameswara [verfasserIn] Sankarasubramanian, K. [verfasserIn] Sreekumar, P. [verfasserIn] Sriram, S. [verfasserIn] Stalin, C. S. [verfasserIn] Sutaria, F. [verfasserIn] Sreedhar, Y. H. [verfasserIn] Barve, I. V. [verfasserIn] Mondal, C. [verfasserIn] Sahu, S. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Journal of astrophysics and astronomy - Bangalore : Springer India, 1980, 38(2017), 2 vom: 19. Juni |
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| Übergeordnetes Werk: |
volume:38 ; year:2017 ; number:2 ; day:19 ; month:06 |
| Links: |
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| DOI / URN: |
10.1007/s12036-017-9445-x |
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| Katalog-ID: |
SPR023996927 |
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| 100 | 1 | |a Tandon, S. N. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a In-orbit Performance of UVIT and First Results |
| 264 | 1 | |c 2017 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 520 | |a Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of %$1.8^{\prime \prime }%$ and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results. | ||
| 650 | 4 | |a Ultraviolet astronomy |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a space astronomy |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a ultraviolet telescopes |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a ultraviolet detectors |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a payloads on AstroSat |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Hutchings, J. B. |e verfasserin |4 aut | |
| 700 | 1 | |a Ghosh, S. K. |e verfasserin |4 aut | |
| 700 | 1 | |a Subramaniam, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Koshy, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Girish, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Kamath, P. U. |e verfasserin |4 aut | |
| 700 | 1 | |a Kathiravan, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Kumar, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Lancelot, J. P. |e verfasserin |4 aut | |
| 700 | 1 | |a Mahesh, P. K. |e verfasserin |4 aut | |
| 700 | 1 | |a Mohan, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Murthy, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Nagabhushana, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Pati, A. K. |e verfasserin |4 aut | |
| 700 | 1 | |a Postma, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Rao, N. Kameswara |e verfasserin |4 aut | |
| 700 | 1 | |a Sankarasubramanian, K. |e verfasserin |4 aut | |
| 700 | 1 | |a Sreekumar, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Sriram, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Stalin, C. S. |e verfasserin |4 aut | |
| 700 | 1 | |a Sutaria, F. |e verfasserin |4 aut | |
| 700 | 1 | |a Sreedhar, Y. H. |e verfasserin |4 aut | |
| 700 | 1 | |a Barve, I. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Mondal, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Sahu, S. |e verfasserin |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Journal of astrophysics and astronomy |d Bangalore : Springer India, 1980 |g 38(2017), 2 vom: 19. Juni |w (DE-627)358454131 |w (DE-600)2096381-6 |x 0973-7758 |7 nnns |
| 773 | 1 | 8 | |g volume:38 |g year:2017 |g number:2 |g day:19 |g month:06 |
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10.1007/s12036-017-9445-x doi (DE-627)SPR023996927 (SPR)s12036-017-9445-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Tandon, S. N. verfasserin aut In-orbit Performance of UVIT and First Results 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of %$1.8^{\prime \prime }%$ and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results. Ultraviolet astronomy (dpeaa)DE-He213 space astronomy (dpeaa)DE-He213 ultraviolet telescopes (dpeaa)DE-He213 ultraviolet detectors (dpeaa)DE-He213 payloads on AstroSat (dpeaa)DE-He213 Hutchings, J. B. verfasserin aut Ghosh, S. K. verfasserin aut Subramaniam, A. verfasserin aut Koshy, G. verfasserin aut Girish, V. verfasserin aut Kamath, P. U. verfasserin aut Kathiravan, S. verfasserin aut Kumar, A. verfasserin aut Lancelot, J. P. verfasserin aut Mahesh, P. K. verfasserin aut Mohan, R. verfasserin aut Murthy, J. verfasserin aut Nagabhushana, S. verfasserin aut Pati, A. K. verfasserin aut Postma, J. verfasserin aut Rao, N. Kameswara verfasserin aut Sankarasubramanian, K. verfasserin aut Sreekumar, P. verfasserin aut Sriram, S. verfasserin aut Stalin, C. S. verfasserin aut Sutaria, F. verfasserin aut Sreedhar, Y. H. verfasserin aut Barve, I. V. verfasserin aut Mondal, C. verfasserin aut Sahu, S. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 38(2017), 2 vom: 19. Juni (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:38 year:2017 number:2 day:19 month:06 https://dx.doi.org/10.1007/s12036-017-9445-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 38 2017 2 19 06 |
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10.1007/s12036-017-9445-x doi (DE-627)SPR023996927 (SPR)s12036-017-9445-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Tandon, S. N. verfasserin aut In-orbit Performance of UVIT and First Results 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of %$1.8^{\prime \prime }%$ and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results. Ultraviolet astronomy (dpeaa)DE-He213 space astronomy (dpeaa)DE-He213 ultraviolet telescopes (dpeaa)DE-He213 ultraviolet detectors (dpeaa)DE-He213 payloads on AstroSat (dpeaa)DE-He213 Hutchings, J. B. verfasserin aut Ghosh, S. K. verfasserin aut Subramaniam, A. verfasserin aut Koshy, G. verfasserin aut Girish, V. verfasserin aut Kamath, P. U. verfasserin aut Kathiravan, S. verfasserin aut Kumar, A. verfasserin aut Lancelot, J. P. verfasserin aut Mahesh, P. K. verfasserin aut Mohan, R. verfasserin aut Murthy, J. verfasserin aut Nagabhushana, S. verfasserin aut Pati, A. K. verfasserin aut Postma, J. verfasserin aut Rao, N. Kameswara verfasserin aut Sankarasubramanian, K. verfasserin aut Sreekumar, P. verfasserin aut Sriram, S. verfasserin aut Stalin, C. S. verfasserin aut Sutaria, F. verfasserin aut Sreedhar, Y. H. verfasserin aut Barve, I. V. verfasserin aut Mondal, C. verfasserin aut Sahu, S. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 38(2017), 2 vom: 19. Juni (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:38 year:2017 number:2 day:19 month:06 https://dx.doi.org/10.1007/s12036-017-9445-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 38 2017 2 19 06 |
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10.1007/s12036-017-9445-x doi (DE-627)SPR023996927 (SPR)s12036-017-9445-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Tandon, S. N. verfasserin aut In-orbit Performance of UVIT and First Results 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of %$1.8^{\prime \prime }%$ and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results. Ultraviolet astronomy (dpeaa)DE-He213 space astronomy (dpeaa)DE-He213 ultraviolet telescopes (dpeaa)DE-He213 ultraviolet detectors (dpeaa)DE-He213 payloads on AstroSat (dpeaa)DE-He213 Hutchings, J. B. verfasserin aut Ghosh, S. K. verfasserin aut Subramaniam, A. verfasserin aut Koshy, G. verfasserin aut Girish, V. verfasserin aut Kamath, P. U. verfasserin aut Kathiravan, S. verfasserin aut Kumar, A. verfasserin aut Lancelot, J. P. verfasserin aut Mahesh, P. K. verfasserin aut Mohan, R. verfasserin aut Murthy, J. verfasserin aut Nagabhushana, S. verfasserin aut Pati, A. K. verfasserin aut Postma, J. verfasserin aut Rao, N. Kameswara verfasserin aut Sankarasubramanian, K. verfasserin aut Sreekumar, P. verfasserin aut Sriram, S. verfasserin aut Stalin, C. S. verfasserin aut Sutaria, F. verfasserin aut Sreedhar, Y. H. verfasserin aut Barve, I. V. verfasserin aut Mondal, C. verfasserin aut Sahu, S. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 38(2017), 2 vom: 19. Juni (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:38 year:2017 number:2 day:19 month:06 https://dx.doi.org/10.1007/s12036-017-9445-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 38 2017 2 19 06 |
| allfieldsGer |
10.1007/s12036-017-9445-x doi (DE-627)SPR023996927 (SPR)s12036-017-9445-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Tandon, S. N. verfasserin aut In-orbit Performance of UVIT and First Results 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of %$1.8^{\prime \prime }%$ and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results. Ultraviolet astronomy (dpeaa)DE-He213 space astronomy (dpeaa)DE-He213 ultraviolet telescopes (dpeaa)DE-He213 ultraviolet detectors (dpeaa)DE-He213 payloads on AstroSat (dpeaa)DE-He213 Hutchings, J. B. verfasserin aut Ghosh, S. K. verfasserin aut Subramaniam, A. verfasserin aut Koshy, G. verfasserin aut Girish, V. verfasserin aut Kamath, P. U. verfasserin aut Kathiravan, S. verfasserin aut Kumar, A. verfasserin aut Lancelot, J. P. verfasserin aut Mahesh, P. K. verfasserin aut Mohan, R. verfasserin aut Murthy, J. verfasserin aut Nagabhushana, S. verfasserin aut Pati, A. K. verfasserin aut Postma, J. verfasserin aut Rao, N. Kameswara verfasserin aut Sankarasubramanian, K. verfasserin aut Sreekumar, P. verfasserin aut Sriram, S. verfasserin aut Stalin, C. S. verfasserin aut Sutaria, F. verfasserin aut Sreedhar, Y. H. verfasserin aut Barve, I. V. verfasserin aut Mondal, C. verfasserin aut Sahu, S. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 38(2017), 2 vom: 19. Juni (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:38 year:2017 number:2 day:19 month:06 https://dx.doi.org/10.1007/s12036-017-9445-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 38 2017 2 19 06 |
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10.1007/s12036-017-9445-x doi (DE-627)SPR023996927 (SPR)s12036-017-9445-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.22 bkl Tandon, S. N. verfasserin aut In-orbit Performance of UVIT and First Results 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of %$1.8^{\prime \prime }%$ and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results. Ultraviolet astronomy (dpeaa)DE-He213 space astronomy (dpeaa)DE-He213 ultraviolet telescopes (dpeaa)DE-He213 ultraviolet detectors (dpeaa)DE-He213 payloads on AstroSat (dpeaa)DE-He213 Hutchings, J. B. verfasserin aut Ghosh, S. K. verfasserin aut Subramaniam, A. verfasserin aut Koshy, G. verfasserin aut Girish, V. verfasserin aut Kamath, P. U. verfasserin aut Kathiravan, S. verfasserin aut Kumar, A. verfasserin aut Lancelot, J. P. verfasserin aut Mahesh, P. K. verfasserin aut Mohan, R. verfasserin aut Murthy, J. verfasserin aut Nagabhushana, S. verfasserin aut Pati, A. K. verfasserin aut Postma, J. verfasserin aut Rao, N. Kameswara verfasserin aut Sankarasubramanian, K. verfasserin aut Sreekumar, P. verfasserin aut Sriram, S. verfasserin aut Stalin, C. S. verfasserin aut Sutaria, F. verfasserin aut Sreedhar, Y. H. verfasserin aut Barve, I. V. verfasserin aut Mondal, C. verfasserin aut Sahu, S. verfasserin aut Enthalten in Journal of astrophysics and astronomy Bangalore : Springer India, 1980 38(2017), 2 vom: 19. Juni (DE-627)358454131 (DE-600)2096381-6 0973-7758 nnns volume:38 year:2017 number:2 day:19 month:06 https://dx.doi.org/10.1007/s12036-017-9445-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 39.22 ASE AR 38 2017 2 19 06 |
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Enthalten in Journal of astrophysics and astronomy 38(2017), 2 vom: 19. Juni volume:38 year:2017 number:2 day:19 month:06 |
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Enthalten in Journal of astrophysics and astronomy 38(2017), 2 vom: 19. Juni volume:38 year:2017 number:2 day:19 month:06 |
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Tandon, S. N. @@aut@@ Hutchings, J. B. @@aut@@ Ghosh, S. K. @@aut@@ Subramaniam, A. @@aut@@ Koshy, G. @@aut@@ Girish, V. @@aut@@ Kamath, P. U. @@aut@@ Kathiravan, S. @@aut@@ Kumar, A. @@aut@@ Lancelot, J. P. @@aut@@ Mahesh, P. K. @@aut@@ Mohan, R. @@aut@@ Murthy, J. @@aut@@ Nagabhushana, S. @@aut@@ Pati, A. K. @@aut@@ Postma, J. @@aut@@ Rao, N. Kameswara @@aut@@ Sankarasubramanian, K. @@aut@@ Sreekumar, P. @@aut@@ Sriram, S. @@aut@@ Stalin, C. S. @@aut@@ Sutaria, F. @@aut@@ Sreedhar, Y. H. @@aut@@ Barve, I. V. @@aut@@ Mondal, C. @@aut@@ Sahu, S. @@aut@@ |
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Tandon, S. N. |
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Tandon, S. N. ddc 520 bkl 39.22 misc Ultraviolet astronomy misc space astronomy misc ultraviolet telescopes misc ultraviolet detectors misc payloads on AstroSat In-orbit Performance of UVIT and First Results |
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520 ASE 39.22 bkl In-orbit Performance of UVIT and First Results Ultraviolet astronomy (dpeaa)DE-He213 space astronomy (dpeaa)DE-He213 ultraviolet telescopes (dpeaa)DE-He213 ultraviolet detectors (dpeaa)DE-He213 payloads on AstroSat (dpeaa)DE-He213 |
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ddc 520 bkl 39.22 misc Ultraviolet astronomy misc space astronomy misc ultraviolet telescopes misc ultraviolet detectors misc payloads on AstroSat |
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ddc 520 bkl 39.22 misc Ultraviolet astronomy misc space astronomy misc ultraviolet telescopes misc ultraviolet detectors misc payloads on AstroSat |
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ddc 520 bkl 39.22 misc Ultraviolet astronomy misc space astronomy misc ultraviolet telescopes misc ultraviolet detectors misc payloads on AstroSat |
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In-orbit Performance of UVIT and First Results |
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In-orbit Performance of UVIT and First Results |
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Tandon, S. N. |
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Journal of astrophysics and astronomy |
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Tandon, S. N. Hutchings, J. B. Ghosh, S. K. Subramaniam, A. Koshy, G. Girish, V. Kamath, P. U. Kathiravan, S. Kumar, A. Lancelot, J. P. Mahesh, P. K. Mohan, R. Murthy, J. Nagabhushana, S. Pati, A. K. Postma, J. Rao, N. Kameswara Sankarasubramanian, K. Sreekumar, P. Sriram, S. Stalin, C. S. Sutaria, F. Sreedhar, Y. H. Barve, I. V. Mondal, C. Sahu, S. |
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Tandon, S. N. |
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10.1007/s12036-017-9445-x |
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in-orbit performance of uvit and first results |
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In-orbit Performance of UVIT and First Results |
| abstract |
Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of %$1.8^{\prime \prime }%$ and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results. |
| abstractGer |
Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of %$1.8^{\prime \prime }%$ and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results. |
| abstract_unstemmed |
Abstract The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within %$\sim %$15% of the estimates, and the spatial resolution in the NUV is found to exceed significantly the design value of %$1.8^{\prime \prime }%$ and it is marginally better in the FUV. Images obtained from UVIT are presented to illustrate the details revealed by the high spatial resolution. The potential of multi-band observations in the ultraviolet with high spatial resolution is illustrated by some results. |
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In-orbit Performance of UVIT and First Results |
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Hutchings, J. B. Ghosh, S. K. Subramaniam, A. Koshy, G. Girish, V. Kamath, P. U. Kathiravan, S. Kumar, A. Lancelot, J. P. Mahesh, P. K. Mohan, R. Murthy, J. Nagabhushana, S. Pati, A. K. Postma, J. Rao, N. Kameswara Sankarasubramanian, K. Sreekumar, P. Sriram, S. Stalin, C. S. Sutaria, F. Sreedhar, Y. H. Barve, I. V. Mondal, C. Sahu, S. |
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| score |
7.4008617 |