The Doppler method for the detection of exoplanets:
The study of exoplanets is one of the most vibrant fields of astrophysics today. Precise radial velocity (RV, or Doppler) measurements created the field by discovering the first exoplanets. Although employed for more than 30 years, RV measurements are still relevant today; when used with the transit...
Gespeichert in:
1. Verfasser: | |
---|---|
Format: | Elektronisch E-Book |
Sprache: | English |
Veröffentlicht: |
Bristol [England]
IOP Publishing
[2020]
|
Schriftenreihe: | AAS-IOP astronomy. [release 2]
|
Schlagworte: | |
Online-Zugang: | URL des Erstveröffentlichers |
Zusammenfassung: | The study of exoplanets is one of the most vibrant fields of astrophysics today. Precise radial velocity (RV, or Doppler) measurements created the field by discovering the first exoplanets. Although employed for more than 30 years, RV measurements are still relevant today; when used with the transit method it provides the first characterization of exoplanets in terms of its mass, radius, and bulk density. These provide the first clues as to the internal structure of the exoplanet. With this text, Hatzes provides a deep understanding of the Doppler method, including how to achieve RV measurement precision, as well as the challenges, limitations, and potential of the technique. It also covers other aspects of the method such instrumentation, wavelength calibration, finding periodic signals in RV time series, signal interpretation, and Keplerian orbits. It's an essential reference for researchers and graduate students in the field of exoplanets, and additionally stellar spectroscopists and instrumentalists |
Beschreibung: | 1 Online-Ressource illustrations (some color) |
ISBN: | 9780750316897 9780750316880 |
DOI: | 10.1088/2514-3433/ab46a3 |
Internformat
MARC
LEADER | 00000nmm a2200000zc 4500 | ||
---|---|---|---|
001 | BV047877946 | ||
003 | DE-604 | ||
005 | 00000000000000.0 | ||
007 | cr|uuu---uuuuu | ||
008 | 220310s2020 |||| o||u| ||||||eng d | ||
020 | |a 9780750316897 |9 978-0-7503-1689-7 | ||
020 | |a 9780750316880 |9 978-0-7503-1688-0 | ||
024 | 7 | |a 10.1088/2514-3433/ab46a3 |2 doi | |
035 | |a (ZDB-135-IAL)9780750316897 | ||
035 | |a (OCoLC)1304475412 | ||
035 | |a (DE-599)BVBBV047877946 | ||
040 | |a DE-604 |b ger |e rda | ||
041 | 0 | |a eng | |
082 | 0 | |a 523 |2 23 | |
100 | 1 | |a Hatzes, A. P. |e Verfasser |4 aut | |
245 | 1 | 0 | |a The Doppler method for the detection of exoplanets |c A.P. Hatzes |
264 | 1 | |a Bristol [England] |b IOP Publishing |c [2020] | |
300 | |a 1 Online-Ressource |b illustrations (some color) | ||
336 | |b txt |2 rdacontent | ||
337 | |b c |2 rdamedia | ||
338 | |b cr |2 rdacarrier | ||
490 | 0 | |a AAS-IOP astronomy. [release 2] | |
520 | |a The study of exoplanets is one of the most vibrant fields of astrophysics today. Precise radial velocity (RV, or Doppler) measurements created the field by discovering the first exoplanets. Although employed for more than 30 years, RV measurements are still relevant today; when used with the transit method it provides the first characterization of exoplanets in terms of its mass, radius, and bulk density. These provide the first clues as to the internal structure of the exoplanet. With this text, Hatzes provides a deep understanding of the Doppler method, including how to achieve RV measurement precision, as well as the challenges, limitations, and potential of the technique. It also covers other aspects of the method such instrumentation, wavelength calibration, finding periodic signals in RV time series, signal interpretation, and Keplerian orbits. It's an essential reference for researchers and graduate students in the field of exoplanets, and additionally stellar spectroscopists and instrumentalists | ||
650 | 7 | |a Solar system - the Sun & planets |2 bicssc | |
650 | 7 | |a SCIENCE / Astronomy |2 bisacsh | |
650 | 4 | |a Extrasolar planets / Remote sensing | |
650 | 4 | |a Astronomical spectroscopy | |
776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |z 9780750316873 |
776 | 0 | 8 | |i Erscheint auch als |n Druck-Ausgabe |z 9780750317740 |
856 | 4 | 0 | |u https://doi.org/10.1088/2514-3433/ab46a3 |x Verlag |z URL des Erstveröffentlichers |3 Volltext |
912 | |a ZDB-135-IAL | ||
999 | |a oai:aleph.bib-bvb.de:BVB01-033260336 |
Datensatz im Suchindex
_version_ | 1804183473371480064 |
---|---|
adam_txt | |
any_adam_object | |
any_adam_object_boolean | |
author | Hatzes, A. P. |
author_facet | Hatzes, A. P. |
author_role | aut |
author_sort | Hatzes, A. P. |
author_variant | a p h ap aph |
building | Verbundindex |
bvnumber | BV047877946 |
collection | ZDB-135-IAL |
ctrlnum | (ZDB-135-IAL)9780750316897 (OCoLC)1304475412 (DE-599)BVBBV047877946 |
dewey-full | 523 |
dewey-hundreds | 500 - Natural sciences and mathematics |
dewey-ones | 523 - Specific celestial bodies and phenomena |
dewey-raw | 523 |
dewey-search | 523 |
dewey-sort | 3523 |
dewey-tens | 520 - Astronomy and allied sciences |
discipline | Physik |
discipline_str_mv | Physik |
doi_str_mv | 10.1088/2514-3433/ab46a3 |
format | Electronic eBook |
fullrecord | <?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>02452nmm a2200409zc 4500</leader><controlfield tag="001">BV047877946</controlfield><controlfield tag="003">DE-604</controlfield><controlfield tag="005">00000000000000.0</controlfield><controlfield tag="007">cr|uuu---uuuuu</controlfield><controlfield tag="008">220310s2020 |||| o||u| ||||||eng d</controlfield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9780750316897</subfield><subfield code="9">978-0-7503-1689-7</subfield></datafield><datafield tag="020" ind1=" " ind2=" "><subfield code="a">9780750316880</subfield><subfield code="9">978-0-7503-1688-0</subfield></datafield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1088/2514-3433/ab46a3</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(ZDB-135-IAL)9780750316897</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(OCoLC)1304475412</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)BVBBV047877946</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-604</subfield><subfield code="b">ger</subfield><subfield code="e">rda</subfield></datafield><datafield tag="041" ind1="0" ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2=" "><subfield code="a">523</subfield><subfield code="2">23</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Hatzes, A. P.</subfield><subfield code="e">Verfasser</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">The Doppler method for the detection of exoplanets</subfield><subfield code="c">A.P. Hatzes</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="a">Bristol [England]</subfield><subfield code="b">IOP Publishing</subfield><subfield code="c">[2020]</subfield></datafield><datafield tag="300" ind1=" " ind2=" "><subfield code="a">1 Online-Ressource</subfield><subfield code="b">illustrations (some color)</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="490" ind1="0" ind2=" "><subfield code="a">AAS-IOP astronomy. [release 2]</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The study of exoplanets is one of the most vibrant fields of astrophysics today. Precise radial velocity (RV, or Doppler) measurements created the field by discovering the first exoplanets. Although employed for more than 30 years, RV measurements are still relevant today; when used with the transit method it provides the first characterization of exoplanets in terms of its mass, radius, and bulk density. These provide the first clues as to the internal structure of the exoplanet. With this text, Hatzes provides a deep understanding of the Doppler method, including how to achieve RV measurement precision, as well as the challenges, limitations, and potential of the technique. It also covers other aspects of the method such instrumentation, wavelength calibration, finding periodic signals in RV time series, signal interpretation, and Keplerian orbits. It's an essential reference for researchers and graduate students in the field of exoplanets, and additionally stellar spectroscopists and instrumentalists</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">Solar system - the Sun & planets</subfield><subfield code="2">bicssc</subfield></datafield><datafield tag="650" ind1=" " ind2="7"><subfield code="a">SCIENCE / Astronomy</subfield><subfield code="2">bisacsh</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Extrasolar planets / Remote sensing</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Astronomical spectroscopy</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe</subfield><subfield code="z">9780750316873</subfield></datafield><datafield tag="776" ind1="0" ind2="8"><subfield code="i">Erscheint auch als</subfield><subfield code="n">Druck-Ausgabe</subfield><subfield code="z">9780750317740</subfield></datafield><datafield tag="856" ind1="4" ind2="0"><subfield code="u">https://doi.org/10.1088/2514-3433/ab46a3</subfield><subfield code="x">Verlag</subfield><subfield code="z">URL des Erstveröffentlichers</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">ZDB-135-IAL</subfield></datafield><datafield tag="999" ind1=" " ind2=" "><subfield code="a">oai:aleph.bib-bvb.de:BVB01-033260336</subfield></datafield></record></collection> |
id | DE-604.BV047877946 |
illustrated | Illustrated |
index_date | 2024-07-03T19:21:41Z |
indexdate | 2024-07-10T09:24:00Z |
institution | BVB |
isbn | 9780750316897 9780750316880 |
language | English |
oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-033260336 |
oclc_num | 1304475412 |
open_access_boolean | |
physical | 1 Online-Ressource illustrations (some color) |
psigel | ZDB-135-IAL |
publishDate | 2020 |
publishDateSearch | 2020 |
publishDateSort | 2020 |
publisher | IOP Publishing |
record_format | marc |
series2 | AAS-IOP astronomy. [release 2] |
spelling | Hatzes, A. P. Verfasser aut The Doppler method for the detection of exoplanets A.P. Hatzes Bristol [England] IOP Publishing [2020] 1 Online-Ressource illustrations (some color) txt rdacontent c rdamedia cr rdacarrier AAS-IOP astronomy. [release 2] The study of exoplanets is one of the most vibrant fields of astrophysics today. Precise radial velocity (RV, or Doppler) measurements created the field by discovering the first exoplanets. Although employed for more than 30 years, RV measurements are still relevant today; when used with the transit method it provides the first characterization of exoplanets in terms of its mass, radius, and bulk density. These provide the first clues as to the internal structure of the exoplanet. With this text, Hatzes provides a deep understanding of the Doppler method, including how to achieve RV measurement precision, as well as the challenges, limitations, and potential of the technique. It also covers other aspects of the method such instrumentation, wavelength calibration, finding periodic signals in RV time series, signal interpretation, and Keplerian orbits. It's an essential reference for researchers and graduate students in the field of exoplanets, and additionally stellar spectroscopists and instrumentalists Solar system - the Sun & planets bicssc SCIENCE / Astronomy bisacsh Extrasolar planets / Remote sensing Astronomical spectroscopy Erscheint auch als Druck-Ausgabe 9780750316873 Erscheint auch als Druck-Ausgabe 9780750317740 https://doi.org/10.1088/2514-3433/ab46a3 Verlag URL des Erstveröffentlichers Volltext |
spellingShingle | Hatzes, A. P. The Doppler method for the detection of exoplanets Solar system - the Sun & planets bicssc SCIENCE / Astronomy bisacsh Extrasolar planets / Remote sensing Astronomical spectroscopy |
title | The Doppler method for the detection of exoplanets |
title_auth | The Doppler method for the detection of exoplanets |
title_exact_search | The Doppler method for the detection of exoplanets |
title_exact_search_txtP | The Doppler method for the detection of exoplanets |
title_full | The Doppler method for the detection of exoplanets A.P. Hatzes |
title_fullStr | The Doppler method for the detection of exoplanets A.P. Hatzes |
title_full_unstemmed | The Doppler method for the detection of exoplanets A.P. Hatzes |
title_short | The Doppler method for the detection of exoplanets |
title_sort | the doppler method for the detection of exoplanets |
topic | Solar system - the Sun & planets bicssc SCIENCE / Astronomy bisacsh Extrasolar planets / Remote sensing Astronomical spectroscopy |
topic_facet | Solar system - the Sun & planets SCIENCE / Astronomy Extrasolar planets / Remote sensing Astronomical spectroscopy |
url | https://doi.org/10.1088/2514-3433/ab46a3 |
work_keys_str_mv | AT hatzesap thedopplermethodforthedetectionofexoplanets |