eprintid: 10090597 rev_number: 16 eprint_status: archive userid: 608 dir: disk0/10/09/05/97 datestamp: 2020-01-28 12:08:10 lastmod: 2021-09-23 22:29:45 status_changed: 2020-01-28 12:08:10 type: article metadata_visibility: show creators_name: Kos, J creators_name: Zwitter, T creators_name: Grebel, EK creators_name: Bienayme, O creators_name: Binney, J creators_name: Bland-Hawthorn, J creators_name: Freeman, KC creators_name: Gibson, BK creators_name: Gilmore, G creators_name: Kordopatis, G creators_name: Navarro, JF creators_name: Parker, Q creators_name: Reid, WA creators_name: Seabroke, G creators_name: Siebert, A creators_name: Siviero, A creators_name: Steinmetz, M creators_name: Watson, F creators_name: Wyse, RFG title: DIFFUSE INTERSTELLAR BAND AT 8620 angstrom IN RAVE: A NEW METHOD FOR DETECTING THE DIFFUSE INTERSTELLAR BAND IN SPECTRA OF COOL STAR ispublished: pub divisions: UCL divisions: B04 divisions: C06 divisions: F63 note: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions. abstract: Diffuse interstellar bands (DIBs) are usually observed in spectra of hot stars, where interstellar lines are rarely blended with stellar ones. The need for hot stars is a strong limitation in the number of sightlines we can observe and their distribution in the Galaxy, as hot stars are rare and concentrated in the Galactic plane. We are introducing a new method, where interstellar lines can be observed in spectra of cool stars in large spectroscopic surveys. The method is completely automated and does not require prior knowledge of the stellar parameters. The main step is a construction of the stellar spectrum, which is done by finding other observed spectra that lack interstellar features and are otherwise very similar to the spectrum in question. Such spectra are then combined into a single stellar spectrum template, matching the stellar component of the observed spectrum. We demonstrate the performance of this new method on a sample of 482,430 Radial Velocity Experiment survey spectra. However, many spectra have to be combined (48 on average) in order to achieve a signal-to-noise ratio high enough to measure the profile of the DIB at 8620 Å, hence limiting the spatial information about the interstellar medium. We compare its equivalent width with extinction maps and with Bayesian reddening, calculated for individual stars, and provide a linear relation between the equivalent width and reddening. Separately from the introduced method, we calculate equivalent widths of the DIB in spectra of hot stars with known extinction and compare all three linear relations. date: 2013-11-07 date_type: published publisher: IOP PUBLISHING LTD official_url: https://doi.org/10.1088/0004-637X/778/2/86 oa_status: green full_text_type: pub language: eng primo: open primo_central: open_green verified: verified_manual elements_id: 905336 doi: 10.1088/0004-637X/778/2/86 lyricists_name: Seabroke, George lyricists_id: GMSEA14 actors_name: Jayawardana, Anusha actors_id: AJAYA51 actors_role: owner full_text_status: public publication: The Astrophysical Journal volume: 778 number: 2 article_number: 86 pages: 11 issn: 1538-4357 citation: Kos, J; Zwitter, T; Grebel, EK; Bienayme, O; Binney, J; Bland-Hawthorn, J; Freeman, KC; ... Wyse, RFG; + view all <#> Kos, J; Zwitter, T; Grebel, EK; Bienayme, O; Binney, J; Bland-Hawthorn, J; Freeman, KC; Gibson, BK; Gilmore, G; Kordopatis, G; Navarro, JF; Parker, Q; Reid, WA; Seabroke, G; Siebert, A; Siviero, A; Steinmetz, M; Watson, F; Wyse, RFG; - view fewer <#> (2013) DIFFUSE INTERSTELLAR BAND AT 8620 angstrom IN RAVE: A NEW METHOD FOR DETECTING THE DIFFUSE INTERSTELLAR BAND IN SPECTRA OF COOL STAR. The Astrophysical Journal , 778 (2) , Article 86. 10.1088/0004-637X/778/2/86 <https://doi.org/10.1088/0004-637X%2F778%2F2%2F86>. Green open access document_url: https://discovery.ucl.ac.uk/id/eprint/10090597/1/Seabroke_Kos_2013_ApJ_778_86.pdf