A dataset provided by the European Space Agency

Name SDP_nevans_3
Title Dust, Ice, and Gas In Time (DIGIT)
URL

http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342188037&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342188038&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342188039&instrument_name=PACS&product_level=LEVEL0&compress=true
http://archives.esac.esa.int/hsa/whsa-tap-server/data?retrieval_type=OBSERVATION&observation_id=1342188040&instrument_name=PACS&product_level=LEVEL0&compress=true
DOI https://doi.org/10.5270/esa-jahe6il
Author evans, n.
Description Dust, ice, and gas evolve as they move from envelopes of forming starsinto circumstellar disks where they can become the main buildingblocks of planets. Herschel-PACS is uniquely suited to trace thisevolution through broadband emission from dust, through specificfeatures of solids which reveal elemental composition and watercontent, and through spectral bands of the main icy components. Bothatomic and molecular lines, in particular the O I, H2O and OH lines,will be used to follow the gas, study the interchange between gas andice, and trace the oxygen budget. The gas and dust spectral featuresare at the same time excellent probes of macroscopic parameters, suchas temperature, UV and X-ray fields, density and thermal structuresof envelopes and disks, and dynamical mixing processes.Our sample covers sources with a range inevolutionary state from embedded objects with massive envelopes toweak-line T Tauri stars with dissipating disks, and with a range inluminosity, spectral type, and dust characteristics. Both our high S/NPACS full spectral range scans (complemented by Spitzer mid-IRspectral scans) and our targeted, deep gas-phase line measurementswill have lasting archival value.
Publication
  • First results of the Herschel key program Dust Ice and Gas In Time (DIGIT): Dust and gas spectroscopy of HD 100546 | Sturm B. et al. | Astronomy and Astrophysics Volume 518 id.L129 5 pp. | 518 | 10.1051/0004-6361/201014674 | 2010A&A...518L.129S | http://adsabs.harvard.edu/abs/2010A%26A...518L.129S
  • DIGIT survey of far-infrared lines from protoplanetary discs. II. CO | Meeus Gwendolyn et al. | Astronomy & Astrophysics Volume 559 id.A84 20 pp. | 559 | 10.1051/0004-6361/201321122 | 2013A&A...559A..84M | http://adsabs.harvard.edu/abs/2013A%26A...559A..84M
  • Mass constraints for 15 protoplanetary discs from HD 1-0 | Kama M. et al. | Astronomy and Astrophysics | null | null | 2020A&A...634A..88K |
  • Low abundance strong features: window-dressing crystalline forsterite in the disk wall of HD 100546 | Mulders G. D. et al. | Astronomy & Astrophysics Volume 531 id.A93 17 pp. | 531 | 10.1051/0004-6361/201116770 | 2011A&A...531A..93M | http://adsabs.harvard.edu/abs/2011A%26A...531A..93M
  • The CDF Archive: Herschel PACS and SPIRE Spectroscopic Data Pipeline and Products for Protostars and Young Stellar Objects | Green Joel D. et al. | The Astronomical Journal Volume 151 Issue 3 article id. 75 23 pp. (2016). | 151 | 10.3847/0004-6256/151/3/75 | 2016AJ....151...75G | http://adsabs.harvard.edu/abs/2016AJ....151...75G
  • The warm gas atmosphere of the HD 100546 disk seen by Herschel. Evidence of a gas-rich carbon-poor atmosphere? | Bruderer S. et al. | Astronomy & Astrophysics Volume 541 id.A91 28 pp. | 541 | 10.1051/0004-6361/201118218 | 2012A&A...541A..91B | http://adsabs.harvard.edu/abs/2012A%26A...541A..91B
  • DIGIT survey of far-infrared lines from protoplanetary disks. I. O i C ii OH H2O and CH+ | Fedele D. et al. | Astronomy & Astrophysics Volume 559 id.A77 22 pp. | 559 | 10.1051/0004-6361/201321118 | 2013A&A...559A..77F | http://adsabs.harvard.edu/abs/2013A%26A...559A..77F
Instrument PACS_PacsRangeSpec_
Temporal Coverage 2009-12-11T03:55:45Z/2009-12-11T11:18:01Z
Version SPG v14.2.0
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 2010-01-20T08:53:27Z
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, evans et al., 2010, 'Dust, Ice, and Gas In Time (DIGIT)', SPG v14.2.0, European Space Agency, https://doi.org/10.5270/esa-jahe6il