PL612 LOFAR station sensitivity measurements in the context of its application for pulsar observations
The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium...
Ausführliche Beschreibung
Autor*in: |
Błaszkiewicz, L.P. [verfasserIn] |
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Format: |
E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
2018transfer abstract |
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Schlagwörter: |
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Umfang: |
14 |
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Übergeordnetes Werk: |
Enthalten in: Posttranscriptional actions of triiodothyronine on - Bargi-Souza, Paula ELSEVIER, 2018, including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU), Amsterdam [u.a.] |
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Übergeordnetes Werk: |
volume:62 ; year:2018 ; number:7 ; day:1 ; month:10 ; pages:1904-1917 ; extent:14 |
Links: |
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DOI / URN: |
10.1016/j.asr.2018.06.047 |
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Katalog-ID: |
ELV043863256 |
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520 | |a The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. | ||
520 | |a The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. | ||
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650 | 7 | |a LOFAR – low frequencies |2 Elsevier | |
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700 | 1 | |a Froń, A. |4 oth | |
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700 | 1 | |a Dąbrowski, B. |4 oth | |
700 | 1 | |a Kotulak, K. |4 oth | |
700 | 1 | |a Hajduk, M. |4 oth | |
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10.1016/j.asr.2018.06.047 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001042.pica (DE-627)ELV043863256 (ELSEVIER)S0273-1177(18)30546-5 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Błaszkiewicz, L.P. verfasserin aut PL612 LOFAR station sensitivity measurements in the context of its application for pulsar observations 2018transfer abstract 14 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. Sensitivity – pulsar's observation Elsevier Instrumentation Elsevier LOFAR – low frequencies Elsevier Lewandowski, W. oth Krankowski, A. oth Kijak, J. oth Froń, A. oth Sidorowicz, T. oth Dąbrowski, B. oth Kotulak, K. oth Hajduk, M. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:62 year:2018 number:7 day:1 month:10 pages:1904-1917 extent:14 https://doi.org/10.1016/j.asr.2018.06.047 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 62 2018 7 1 1001 1904-1917 14 |
spelling |
10.1016/j.asr.2018.06.047 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001042.pica (DE-627)ELV043863256 (ELSEVIER)S0273-1177(18)30546-5 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Błaszkiewicz, L.P. verfasserin aut PL612 LOFAR station sensitivity measurements in the context of its application for pulsar observations 2018transfer abstract 14 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. Sensitivity – pulsar's observation Elsevier Instrumentation Elsevier LOFAR – low frequencies Elsevier Lewandowski, W. oth Krankowski, A. oth Kijak, J. oth Froń, A. oth Sidorowicz, T. oth Dąbrowski, B. oth Kotulak, K. oth Hajduk, M. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:62 year:2018 number:7 day:1 month:10 pages:1904-1917 extent:14 https://doi.org/10.1016/j.asr.2018.06.047 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 62 2018 7 1 1001 1904-1917 14 |
allfields_unstemmed |
10.1016/j.asr.2018.06.047 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001042.pica (DE-627)ELV043863256 (ELSEVIER)S0273-1177(18)30546-5 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Błaszkiewicz, L.P. verfasserin aut PL612 LOFAR station sensitivity measurements in the context of its application for pulsar observations 2018transfer abstract 14 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. Sensitivity – pulsar's observation Elsevier Instrumentation Elsevier LOFAR – low frequencies Elsevier Lewandowski, W. oth Krankowski, A. oth Kijak, J. oth Froń, A. oth Sidorowicz, T. oth Dąbrowski, B. oth Kotulak, K. oth Hajduk, M. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:62 year:2018 number:7 day:1 month:10 pages:1904-1917 extent:14 https://doi.org/10.1016/j.asr.2018.06.047 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 62 2018 7 1 1001 1904-1917 14 |
allfieldsGer |
10.1016/j.asr.2018.06.047 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001042.pica (DE-627)ELV043863256 (ELSEVIER)S0273-1177(18)30546-5 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Błaszkiewicz, L.P. verfasserin aut PL612 LOFAR station sensitivity measurements in the context of its application for pulsar observations 2018transfer abstract 14 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. Sensitivity – pulsar's observation Elsevier Instrumentation Elsevier LOFAR – low frequencies Elsevier Lewandowski, W. oth Krankowski, A. oth Kijak, J. oth Froń, A. oth Sidorowicz, T. oth Dąbrowski, B. oth Kotulak, K. oth Hajduk, M. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:62 year:2018 number:7 day:1 month:10 pages:1904-1917 extent:14 https://doi.org/10.1016/j.asr.2018.06.047 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 62 2018 7 1 1001 1904-1917 14 |
allfieldsSound |
10.1016/j.asr.2018.06.047 doi /cbs_pica/cbs_olc/import_discovery/elsevier/einzuspielen/GBV00000000001042.pica (DE-627)ELV043863256 (ELSEVIER)S0273-1177(18)30546-5 DE-627 ger DE-627 rakwb eng 610 570 VZ 44.89 bkl Błaszkiewicz, L.P. verfasserin aut PL612 LOFAR station sensitivity measurements in the context of its application for pulsar observations 2018transfer abstract 14 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. Sensitivity – pulsar's observation Elsevier Instrumentation Elsevier LOFAR – low frequencies Elsevier Lewandowski, W. oth Krankowski, A. oth Kijak, J. oth Froń, A. oth Sidorowicz, T. oth Dąbrowski, B. oth Kotulak, K. oth Hajduk, M. oth Enthalten in Elsevier Science Bargi-Souza, Paula ELSEVIER Posttranscriptional actions of triiodothyronine on 2018 including COSPAR information bulletin : the official journal of the Committee on Space Research (COSPAR), a scientific committee of the International Council of Scientific Unions (ICSU) Amsterdam [u.a.] (DE-627)ELV000905844 volume:62 year:2018 number:7 day:1 month:10 pages:1904-1917 extent:14 https://doi.org/10.1016/j.asr.2018.06.047 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHA 44.89 Endokrinologie VZ AR 62 2018 7 1 1001 1904-1917 14 |
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PL612 LOFAR station sensitivity measurements in the context of its application for pulsar observations |
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The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. |
abstractGer |
The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. |
abstract_unstemmed |
The Low Frequency Array (LOFAR) is relatively new interferometric radio telescope. LOFAR operates in poorly explored part of the spectrum (10–240 MHz). In this frequency range pulsars are bright, and LOFAR observations of pulsars are import for probing fundamental physics and the interstellar medium. In this work we present the description of the international LOFAR station frontend and backend parameters related to pulsar observations with a single LOFAR station, based on observations with the Polish station, located in Bałdy near Olsztyn. We present new results from observations aimed at better characterizing the telescope sensitivity. These measurements are important for efficient planning of pulsar observating campaigns. Observations show good sensitivity for pulsar measurements above 25° elevation and show the noise level rises significantly for elevations below 25°. |
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PL612 LOFAR station sensitivity measurements in the context of its application for pulsar observations |
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