Emission Line Galaxies in the STIS Parallel Survey I: Observations and Data Analysis
In the first three years of operation STIS obtained slitless spectra of approximately 2500 fields in parallel to prime HST observations as part of the STIS Parallel Survey (SPS). The archive contains almost 300 fields at high galactic latitude (|b|>30) with spectroscopic exposure times greater th...
Gespeichert in:
| Veröffentlicht in: | arXiv.org 2002-12 |
|---|---|
| Hauptverfasser: | , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | |
| container_title | arXiv.org |
| container_volume | |
| creator | Teplitz, Harry I Collins, Nicholas R Gardner, Jonathan P Hill, Robert S Heap, Sara R Lindler, Don J Rhodes, Jason Woodgate, Bruce E |
| description | In the first three years of operation STIS obtained slitless spectra of approximately 2500 fields in parallel to prime HST observations as part of the STIS Parallel Survey (SPS). The archive contains almost 300 fields at high galactic latitude (|b|>30) with spectroscopic exposure times greater than 3000 seconds. This sample contains 220 fields (excluding special regions and requiring a consistent grating angle) observed between 6 June 1997 and 21 September 2000, with a total survey area of about 160 square arcminutes. At this depth, the SPS detects an average of one emission line galaxy per three fields. We present the analysis of these data, and the identification of 131 low to intermediate redshift galaxies detected by optical emission lines. The sample contains 78 objects with emission lines that we infer to be redshifted [OII]3727 emission at 0.43 |
| doi_str_mv | 10.48550/arxiv.0212576 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2078854579</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2078854579</sourcerecordid><originalsourceid>FETCH-proquest_journals_20788545793</originalsourceid><addsrcrecordid>eNqNy7EKwjAUQNEgCIq6Oj9wtqZpY6ubaNWCoNDu8sSIkZhqXlvav9fBD3C6y7mMjX3uhbGUfIau0bXHhS9kNO-wvggCfxqHQvTYiOjBORfzSEgZ9FmePDWRLiwctFWwQ4ONVgTaQnlXkOVpBid0aIwykFWuVi2kSzheSLkay-9IgPYKGywRVhZNS5qGrHtDQ2r064BNtkm-3k9frnhXisrzo6jcF9NZ8CiOZSijRfCf-gCXcETm</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2078854579</pqid></control><display><type>article</type><title>Emission Line Galaxies in the STIS Parallel Survey I: Observations and Data Analysis</title><source>Free E- Journals</source><creator>Teplitz, Harry I ; Collins, Nicholas R ; Gardner, Jonathan P ; Hill, Robert S ; Heap, Sara R ; Lindler, Don J ; Rhodes, Jason ; Woodgate, Bruce E</creator><creatorcontrib>Teplitz, Harry I ; Collins, Nicholas R ; Gardner, Jonathan P ; Hill, Robert S ; Heap, Sara R ; Lindler, Don J ; Rhodes, Jason ; Woodgate, Bruce E</creatorcontrib><description>In the first three years of operation STIS obtained slitless spectra of approximately 2500 fields in parallel to prime HST observations as part of the STIS Parallel Survey (SPS). The archive contains almost 300 fields at high galactic latitude (|b|>30) with spectroscopic exposure times greater than 3000 seconds. This sample contains 220 fields (excluding special regions and requiring a consistent grating angle) observed between 6 June 1997 and 21 September 2000, with a total survey area of about 160 square arcminutes. At this depth, the SPS detects an average of one emission line galaxy per three fields. We present the analysis of these data, and the identification of 131 low to intermediate redshift galaxies detected by optical emission lines. The sample contains 78 objects with emission lines that we infer to be redshifted [OII]3727 emission at 0.43<z<1.7. The comoving number density of these objects is comparable to that of H-alpha emitting galaxies in the NICMOS parallel observations. One quasar and three probable Seyfert galaxies are detected. Many of the emission-line objects show morphologies suggestive of mergers or interactions. The reduced data are available upon request from the authors.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.0212576</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Data analysis ; Emission analysis ; Morphology ; Object recognition ; Quasars ; Red shift ; Seyfert galaxies</subject><ispartof>arXiv.org, 2002-12</ispartof><rights>2002. This work is published under https://arxiv.org/licenses/assumed-1991-2003/license.html (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>776,780,27902</link.rule.ids></links><search><creatorcontrib>Teplitz, Harry I</creatorcontrib><creatorcontrib>Collins, Nicholas R</creatorcontrib><creatorcontrib>Gardner, Jonathan P</creatorcontrib><creatorcontrib>Hill, Robert S</creatorcontrib><creatorcontrib>Heap, Sara R</creatorcontrib><creatorcontrib>Lindler, Don J</creatorcontrib><creatorcontrib>Rhodes, Jason</creatorcontrib><creatorcontrib>Woodgate, Bruce E</creatorcontrib><title>Emission Line Galaxies in the STIS Parallel Survey I: Observations and Data Analysis</title><title>arXiv.org</title><description>In the first three years of operation STIS obtained slitless spectra of approximately 2500 fields in parallel to prime HST observations as part of the STIS Parallel Survey (SPS). The archive contains almost 300 fields at high galactic latitude (|b|>30) with spectroscopic exposure times greater than 3000 seconds. This sample contains 220 fields (excluding special regions and requiring a consistent grating angle) observed between 6 June 1997 and 21 September 2000, with a total survey area of about 160 square arcminutes. At this depth, the SPS detects an average of one emission line galaxy per three fields. We present the analysis of these data, and the identification of 131 low to intermediate redshift galaxies detected by optical emission lines. The sample contains 78 objects with emission lines that we infer to be redshifted [OII]3727 emission at 0.43<z<1.7. The comoving number density of these objects is comparable to that of H-alpha emitting galaxies in the NICMOS parallel observations. One quasar and three probable Seyfert galaxies are detected. Many of the emission-line objects show morphologies suggestive of mergers or interactions. The reduced data are available upon request from the authors.</description><subject>Data analysis</subject><subject>Emission analysis</subject><subject>Morphology</subject><subject>Object recognition</subject><subject>Quasars</subject><subject>Red shift</subject><subject>Seyfert galaxies</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2002</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNqNy7EKwjAUQNEgCIq6Oj9wtqZpY6ubaNWCoNDu8sSIkZhqXlvav9fBD3C6y7mMjX3uhbGUfIau0bXHhS9kNO-wvggCfxqHQvTYiOjBORfzSEgZ9FmePDWRLiwctFWwQ4ONVgTaQnlXkOVpBid0aIwykFWuVi2kSzheSLkay-9IgPYKGywRVhZNS5qGrHtDQ2r064BNtkm-3k9frnhXisrzo6jcF9NZ8CiOZSijRfCf-gCXcETm</recordid><startdate>20021231</startdate><enddate>20021231</enddate><creator>Teplitz, Harry I</creator><creator>Collins, Nicholas R</creator><creator>Gardner, Jonathan P</creator><creator>Hill, Robert S</creator><creator>Heap, Sara R</creator><creator>Lindler, Don J</creator><creator>Rhodes, Jason</creator><creator>Woodgate, Bruce E</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20021231</creationdate><title>Emission Line Galaxies in the STIS Parallel Survey I: Observations and Data Analysis</title><author>Teplitz, Harry I ; Collins, Nicholas R ; Gardner, Jonathan P ; Hill, Robert S ; Heap, Sara R ; Lindler, Don J ; Rhodes, Jason ; Woodgate, Bruce E</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20788545793</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2002</creationdate><topic>Data analysis</topic><topic>Emission analysis</topic><topic>Morphology</topic><topic>Object recognition</topic><topic>Quasars</topic><topic>Red shift</topic><topic>Seyfert galaxies</topic><toplevel>online_resources</toplevel><creatorcontrib>Teplitz, Harry I</creatorcontrib><creatorcontrib>Collins, Nicholas R</creatorcontrib><creatorcontrib>Gardner, Jonathan P</creatorcontrib><creatorcontrib>Hill, Robert S</creatorcontrib><creatorcontrib>Heap, Sara R</creatorcontrib><creatorcontrib>Lindler, Don J</creatorcontrib><creatorcontrib>Rhodes, Jason</creatorcontrib><creatorcontrib>Woodgate, Bruce E</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Teplitz, Harry I</au><au>Collins, Nicholas R</au><au>Gardner, Jonathan P</au><au>Hill, Robert S</au><au>Heap, Sara R</au><au>Lindler, Don J</au><au>Rhodes, Jason</au><au>Woodgate, Bruce E</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Emission Line Galaxies in the STIS Parallel Survey I: Observations and Data Analysis</atitle><jtitle>arXiv.org</jtitle><date>2002-12-31</date><risdate>2002</risdate><eissn>2331-8422</eissn><abstract>In the first three years of operation STIS obtained slitless spectra of approximately 2500 fields in parallel to prime HST observations as part of the STIS Parallel Survey (SPS). The archive contains almost 300 fields at high galactic latitude (|b|>30) with spectroscopic exposure times greater than 3000 seconds. This sample contains 220 fields (excluding special regions and requiring a consistent grating angle) observed between 6 June 1997 and 21 September 2000, with a total survey area of about 160 square arcminutes. At this depth, the SPS detects an average of one emission line galaxy per three fields. We present the analysis of these data, and the identification of 131 low to intermediate redshift galaxies detected by optical emission lines. The sample contains 78 objects with emission lines that we infer to be redshifted [OII]3727 emission at 0.43<z<1.7. The comoving number density of these objects is comparable to that of H-alpha emitting galaxies in the NICMOS parallel observations. One quasar and three probable Seyfert galaxies are detected. Many of the emission-line objects show morphologies suggestive of mergers or interactions. The reduced data are available upon request from the authors.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.0212576</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2002-12 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_proquest_journals_2078854579 |
| source | Free E- Journals |
| subjects | Data analysis Emission analysis Morphology Object recognition Quasars Red shift Seyfert galaxies |
| title | Emission Line Galaxies in the STIS Parallel Survey I: Observations and Data Analysis |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-30T22%3A43%3A47IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=Emission%20Line%20Galaxies%20in%20the%20STIS%20Parallel%20Survey%20I:%20Observations%20and%20Data%20Analysis&rft.jtitle=arXiv.org&rft.au=Teplitz,%20Harry%20I&rft.date=2002-12-31&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.0212576&rft_dat=%3Cproquest%3E2078854579%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2078854579&rft_id=info:pmid/&rfr_iscdi=true |