A dataset provided by the European Space Agency

Name DDT_mgroen01_9
Title The phase-lag distance to the carbon star CW Leo: part II
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342246623&instrument_name=SPIRE&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342254051&instrument_name=SPIRE&product_level=LEVEL0&compress=true
DOI https://doi.org/10.5270/esa-mnqx65o
Author groenewegen, m.
Description This DDT proposal is the successor to proposal DDT_mgroen01_6.In the original proposal we argued that it is possible to obtain aphase-lag distance to the well-known Carbon star CW Leo, and obtained2 epochs of SPIRE time.In this proposal we present first results and demonstrate that the method works and present a first distance estimate.The dominant error is in the phase-lag, and we ask for 2 additional epochs to reduce this error, and obtain a more precise and accurate distance.
Publication
  • The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope | Scicluna P. et al. | Monthly Notices of the Royal Astronomical Society | null | null | 2022MNRAS.512.1091S |
  • PACS and SPIRE range spectroscopy of cool evolved stars | Nicolaes D. et al. | Astronomy & Astrophysics Volume 618 id.A143 42 pp. | 618 | 10.1051/0004-6361/201833168 | 2018A&A...618A.143N | http://adsabs.harvard.edu/abs/2018A%26A...618A.143N
  • Systematic characterization of the Herschel SPIRE Fourier Transform Spectrometer | Hopwood R. et al. | Monthly Notices of the Royal Astronomical Society Volume 449 Issue 3 p.2274-2303 | 449 | 10.1093/mnras/stv353 | 2015MNRAS.449.2274H | http://adsabs.harvard.edu/abs/2015MNRAS.449.2274H
  • An independent distance estimate to CW Leonis | Groenewegen M. A. T. et al. | Astronomy & Astrophysics Volume 543 id.L8 6 pp. | 543 | 10.1051/0004-6361/201219604 | 2012A&A...543L...8G | http://adsabs.harvard.edu/abs/2012A%26A...543L...8G
  • New light on Galactic post-asymptotic giant branch stars - I. First distance catalogue | Vickers Shane B. et al. | Monthly Notices of the Royal Astronomical Society Volume 447 Issue 2 p.1673-1691 | 447 | 10.1093/mnras/stu2383 | 2015MNRAS.447.1673V | http://adsabs.harvard.edu/abs/2015MNRAS.447.1673V
Instrument SPIRE_SpirePhoto_large
Temporal Coverage 2012-06-03T16:57:14Z/2012-10-29T18:13:43Z
Version SPG v14.1.0
Mission Description Herschel was launched on 14 May 2009! It is the fourth cornerstone mission in the ESA science programme. With a 3.5 m Cassegrain telescope it is the largest space telescope ever launched. It is performing photometry and spectroscopy in approximately the 55-671 µm range, bridging the gap between earlier infrared space missions and groundbased facilities.
Creator Contact https://support.cosmos.esa.int/h®erschel/
Date Published 2013-04-29T17:00:32Z
Last Update 2025-01-24
Keywords Herschel, HSC, submillimetre, far-infrared, HIFI, PACS, SPIRE
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, groenewegen et al., 2013, 'The phase-lag distance to the carbon star CW Leo: part II', SPG v14.1.0, European Space Agency, https://doi.org/10.5270/esa-mnqx65o