PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects
The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction strategy and data products which are publicly available through the ESO archive as the Spectroscopic Survey Data Release 1...
Gespeichert in:
| Veröffentlicht in: | arXiv.org 2015-05 |
|---|---|
| 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 | Smartt, S J Valenti, S Fraser, M Inserra, C Young, D R Sullivan, M Pastorello, A Benetti, S Gal-Yam, A Knapic, C Molinaro, M Smareglia, R Smith, K W Taubenberger, S Yaron, O Anderson, J P Ashall, C Balland, C Baltay, C Barbarino, C Bauer, F E Baumont, S Bersier, D Blagorodnova, N Bongard, S Botticella, M T Bufano, F Bulla, M Cappellaro, E Campbell, H Cellier-Holzem, F T -W Chen Childress, M J Clocchiatti, A Contreras, C M Dall Ora Danziger, J de Jaeger, T De Cia, A M Della Valle Dennefeld, M Elias-Rosa, N Elman, N Feindt, U Fleury, M Gall, E Gonzalez-Gaitan, S Galbany, L A Morales Garoffolo Greggio, L Guillou, L L Hachinger, S Hadjiyska, E Hage, P E Hillebrandt, W Hodgkin, S Hsiao, E Y James, P A Jerkstrand, A Kangas, T Kankare, E Kotak, R Kromer, M Kuncarayakti, H Leloudas, G Lundqvist, P Lyman, J D Hook, I M Maguire, K Manulis, I Margheim, S J Mattila, S Maund, J R Mazzali, P A McCrum, M McKinnon, R Moreno-Raya, M E Nicholl, M Nugent, P Pain, R Phillips, M M Pignata, G Polshaw, J Pumo, M L Rabinowitz, D Reilly, E Scalzo, R Schmidt, B Sim, S Sollerman, J Taddia, F Tartaglia, L Terreran, G Tomasella, L Turatto, M Walker, E Walton, N A Wyrzykowski, L Yuan, F Zampieri, L |
| description | The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction strategy and data products which are publicly available through the ESO archive as the Spectroscopic Survey Data Release 1 (SSDR1). PESSTO uses the New Technology Telescope with EFOSC2 and SOFI to provide optical and NIR spectroscopy and imaging. We target supernovae and optical transients brighter than 20.5mag for classification. Science targets are then selected for follow-up based on the PESSTO science goal of extending knowledge of the extremes of the supernova population. The EFOSC2 spectra cover 3345-9995A (at resolutions of 13-18 Angs) and SOFI spectra cover 0.935-2.53 micron (resolutions 23-33 Angs) along with JHK imaging. This data release contains spectra from the first year (April 2012 - 2013), consisting of all 814 EFOSC2 spectra and 95 SOFI spectra (covering 298 distinct objects), in standard ESO Phase 3 format. We estimate the accuracy of the absolute flux calibrations for EFOSC2 to be typically 15%, and the relative flux calibration accuracy to be about 5%. The PESSTO standard NIR reduction process does not yet produce high accuracy absolute spectrophotometry but the SOFI JHK imaging will improve this. Future data releases will focus on improving the automated flux calibration of the data products. |
| doi_str_mv | 10.48550/arxiv.1411.0299 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_1411_0299</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2083614813</sourcerecordid><originalsourceid>FETCH-LOGICAL-a513-b4daf613db12f92f27d81faa8cbb7db533ca017faeb33efafb14abd1206b7f003</originalsourceid><addsrcrecordid>eNotkMtqwzAQRUWh0JBm31UZ6NqpHn6luxLSBwQcsPdmZElUIbFdSQ71rp9eJ-lq4M7hMnMIeWB0GedJQp_R_djTksWMLSlfrW7IjAvBojzm_I4svN9TSnma8SQRM_K725RlVcAL-MGd9AhK-8bZPtiuBWwV9K5TQxM8GNcdIXxpMNb5AAoDgtMHjV6DHC-b3SAPtoFNWUDZ6ya4zjddPyXltbszUDlsvdVtgELuJ8Tfk1uDB68X_3NOqrdNtf6ItsX75_p1G2HCRCRjhSZlQknGzYobnqmcGcS8kTJTMhGiQcoyg1oKoQ0ayWKUinGaysxQKubk8Vp7sVP3zh7RjfXZUn22NAFPV2B6-HvQPtT7bnDtdFLNaS5SFudMiD8qxWyp</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2083614813</pqid></control><display><type>article</type><title>PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects</title><source>arXiv.org</source><source>Freely Accessible Journals at publisher websites</source><creator>Smartt, S J ; Valenti, S ; Fraser, M ; Inserra, C ; Young, D R ; Sullivan, M ; Pastorello, A ; Benetti, S ; Gal-Yam, A ; Knapic, C ; Molinaro, M ; Smareglia, R ; Smith, K W ; Taubenberger, S ; Yaron, O ; Anderson, J P ; Ashall, C ; Balland, C ; Baltay, C ; Barbarino, C ; Bauer, F E ; Baumont, S ; Bersier, D ; Blagorodnova, N ; Bongard, S ; Botticella, M T ; Bufano, F ; Bulla, M ; Cappellaro, E ; Campbell, H ; Cellier-Holzem, F ; T -W Chen ; Childress, M J ; Clocchiatti, A ; Contreras, C ; M Dall Ora ; Danziger, J ; de Jaeger, T ; De Cia, A ; M Della Valle ; Dennefeld, M ; Elias-Rosa, N ; Elman, N ; Feindt, U ; Fleury, M ; Gall, E ; Gonzalez-Gaitan, S ; Galbany, L ; A Morales Garoffolo ; Greggio, L ; Guillou, L L ; Hachinger, S ; Hadjiyska, E ; Hage, P E ; Hillebrandt, W ; Hodgkin, S ; Hsiao, E Y ; James, P A ; Jerkstrand, A ; Kangas, T ; Kankare, E ; Kotak, R ; Kromer, M ; Kuncarayakti, H ; Leloudas, G ; Lundqvist, P ; Lyman, J D ; Hook, I M ; Maguire, K ; Manulis, I ; Margheim, S J ; Mattila, S ; Maund, J R ; Mazzali, P A ; McCrum, M ; McKinnon, R ; Moreno-Raya, M E ; Nicholl, M ; Nugent, P ; Pain, R ; Phillips, M M ; Pignata, G ; Polshaw, J ; Pumo, M L ; Rabinowitz, D ; Reilly, E ; Scalzo, R ; Schmidt, B ; Sim, S ; Sollerman, J ; Taddia, F ; Tartaglia, L ; Terreran, G ; Tomasella, L ; Turatto, M ; Walker, E ; Walton, N A ; Wyrzykowski, L ; Yuan, F ; Zampieri, L</creator><creatorcontrib>Smartt, S J ; Valenti, S ; Fraser, M ; Inserra, C ; Young, D R ; Sullivan, M ; Pastorello, A ; Benetti, S ; Gal-Yam, A ; Knapic, C ; Molinaro, M ; Smareglia, R ; Smith, K W ; Taubenberger, S ; Yaron, O ; Anderson, J P ; Ashall, C ; Balland, C ; Baltay, C ; Barbarino, C ; Bauer, F E ; Baumont, S ; Bersier, D ; Blagorodnova, N ; Bongard, S ; Botticella, M T ; Bufano, F ; Bulla, M ; Cappellaro, E ; Campbell, H ; Cellier-Holzem, F ; T -W Chen ; Childress, M J ; Clocchiatti, A ; Contreras, C ; M Dall Ora ; Danziger, J ; de Jaeger, T ; De Cia, A ; M Della Valle ; Dennefeld, M ; Elias-Rosa, N ; Elman, N ; Feindt, U ; Fleury, M ; Gall, E ; Gonzalez-Gaitan, S ; Galbany, L ; A Morales Garoffolo ; Greggio, L ; Guillou, L L ; Hachinger, S ; Hadjiyska, E ; Hage, P E ; Hillebrandt, W ; Hodgkin, S ; Hsiao, E Y ; James, P A ; Jerkstrand, A ; Kangas, T ; Kankare, E ; Kotak, R ; Kromer, M ; Kuncarayakti, H ; Leloudas, G ; Lundqvist, P ; Lyman, J D ; Hook, I M ; Maguire, K ; Manulis, I ; Margheim, S J ; Mattila, S ; Maund, J R ; Mazzali, P A ; McCrum, M ; McKinnon, R ; Moreno-Raya, M E ; Nicholl, M ; Nugent, P ; Pain, R ; Phillips, M M ; Pignata, G ; Polshaw, J ; Pumo, M L ; Rabinowitz, D ; Reilly, E ; Scalzo, R ; Schmidt, B ; Sim, S ; Sollerman, J ; Taddia, F ; Tartaglia, L ; Terreran, G ; Tomasella, L ; Turatto, M ; Walker, E ; Walton, N A ; Wyrzykowski, L ; Yuan, F ; Zampieri, L</creatorcontrib><description>The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction strategy and data products which are publicly available through the ESO archive as the Spectroscopic Survey Data Release 1 (SSDR1). PESSTO uses the New Technology Telescope with EFOSC2 and SOFI to provide optical and NIR spectroscopy and imaging. We target supernovae and optical transients brighter than 20.5mag for classification. Science targets are then selected for follow-up based on the PESSTO science goal of extending knowledge of the extremes of the supernova population. The EFOSC2 spectra cover 3345-9995A (at resolutions of 13-18 Angs) and SOFI spectra cover 0.935-2.53 micron (resolutions 23-33 Angs) along with JHK imaging. This data release contains spectra from the first year (April 2012 - 2013), consisting of all 814 EFOSC2 spectra and 95 SOFI spectra (covering 298 distinct objects), in standard ESO Phase 3 format. We estimate the accuracy of the absolute flux calibrations for EFOSC2 to be typically 15%, and the relative flux calibration accuracy to be about 5%. The PESSTO standard NIR reduction process does not yet produce high accuracy absolute spectrophotometry but the SOFI JHK imaging will improve this. Future data releases will focus on improving the automated flux calibration of the data products.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1411.0299</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Accuracy ; Calibration ; Data reduction ; European Southern Observatory ; Flux ; Imaging ; New technology ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics ; Spectra ; Spectrophotometry ; Spectroscopy ; Spectrum analysis ; Supernovae ; Target recognition</subject><ispartof>arXiv.org, 2015-05</ispartof><rights>2015. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,784,885,27925</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.1411.0299$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1051/0004-6361/201425237$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Smartt, S J</creatorcontrib><creatorcontrib>Valenti, S</creatorcontrib><creatorcontrib>Fraser, M</creatorcontrib><creatorcontrib>Inserra, C</creatorcontrib><creatorcontrib>Young, D R</creatorcontrib><creatorcontrib>Sullivan, M</creatorcontrib><creatorcontrib>Pastorello, A</creatorcontrib><creatorcontrib>Benetti, S</creatorcontrib><creatorcontrib>Gal-Yam, A</creatorcontrib><creatorcontrib>Knapic, C</creatorcontrib><creatorcontrib>Molinaro, M</creatorcontrib><creatorcontrib>Smareglia, R</creatorcontrib><creatorcontrib>Smith, K W</creatorcontrib><creatorcontrib>Taubenberger, S</creatorcontrib><creatorcontrib>Yaron, O</creatorcontrib><creatorcontrib>Anderson, J P</creatorcontrib><creatorcontrib>Ashall, C</creatorcontrib><creatorcontrib>Balland, C</creatorcontrib><creatorcontrib>Baltay, C</creatorcontrib><creatorcontrib>Barbarino, C</creatorcontrib><creatorcontrib>Bauer, F E</creatorcontrib><creatorcontrib>Baumont, S</creatorcontrib><creatorcontrib>Bersier, D</creatorcontrib><creatorcontrib>Blagorodnova, N</creatorcontrib><creatorcontrib>Bongard, S</creatorcontrib><creatorcontrib>Botticella, M T</creatorcontrib><creatorcontrib>Bufano, F</creatorcontrib><creatorcontrib>Bulla, M</creatorcontrib><creatorcontrib>Cappellaro, E</creatorcontrib><creatorcontrib>Campbell, H</creatorcontrib><creatorcontrib>Cellier-Holzem, F</creatorcontrib><creatorcontrib>T -W Chen</creatorcontrib><creatorcontrib>Childress, M J</creatorcontrib><creatorcontrib>Clocchiatti, A</creatorcontrib><creatorcontrib>Contreras, C</creatorcontrib><creatorcontrib>M Dall Ora</creatorcontrib><creatorcontrib>Danziger, J</creatorcontrib><creatorcontrib>de Jaeger, T</creatorcontrib><creatorcontrib>De Cia, A</creatorcontrib><creatorcontrib>M Della Valle</creatorcontrib><creatorcontrib>Dennefeld, M</creatorcontrib><creatorcontrib>Elias-Rosa, N</creatorcontrib><creatorcontrib>Elman, N</creatorcontrib><creatorcontrib>Feindt, U</creatorcontrib><creatorcontrib>Fleury, M</creatorcontrib><creatorcontrib>Gall, E</creatorcontrib><creatorcontrib>Gonzalez-Gaitan, S</creatorcontrib><creatorcontrib>Galbany, L</creatorcontrib><creatorcontrib>A Morales Garoffolo</creatorcontrib><creatorcontrib>Greggio, L</creatorcontrib><creatorcontrib>Guillou, L L</creatorcontrib><creatorcontrib>Hachinger, S</creatorcontrib><creatorcontrib>Hadjiyska, E</creatorcontrib><creatorcontrib>Hage, P E</creatorcontrib><creatorcontrib>Hillebrandt, W</creatorcontrib><creatorcontrib>Hodgkin, S</creatorcontrib><creatorcontrib>Hsiao, E Y</creatorcontrib><creatorcontrib>James, P A</creatorcontrib><creatorcontrib>Jerkstrand, A</creatorcontrib><creatorcontrib>Kangas, T</creatorcontrib><creatorcontrib>Kankare, E</creatorcontrib><creatorcontrib>Kotak, R</creatorcontrib><creatorcontrib>Kromer, M</creatorcontrib><creatorcontrib>Kuncarayakti, H</creatorcontrib><creatorcontrib>Leloudas, G</creatorcontrib><creatorcontrib>Lundqvist, P</creatorcontrib><creatorcontrib>Lyman, J D</creatorcontrib><creatorcontrib>Hook, I M</creatorcontrib><creatorcontrib>Maguire, K</creatorcontrib><creatorcontrib>Manulis, I</creatorcontrib><creatorcontrib>Margheim, S J</creatorcontrib><creatorcontrib>Mattila, S</creatorcontrib><creatorcontrib>Maund, J R</creatorcontrib><creatorcontrib>Mazzali, P A</creatorcontrib><creatorcontrib>McCrum, M</creatorcontrib><creatorcontrib>McKinnon, R</creatorcontrib><creatorcontrib>Moreno-Raya, M E</creatorcontrib><creatorcontrib>Nicholl, M</creatorcontrib><creatorcontrib>Nugent, P</creatorcontrib><creatorcontrib>Pain, R</creatorcontrib><creatorcontrib>Phillips, M M</creatorcontrib><creatorcontrib>Pignata, G</creatorcontrib><creatorcontrib>Polshaw, J</creatorcontrib><creatorcontrib>Pumo, M L</creatorcontrib><creatorcontrib>Rabinowitz, D</creatorcontrib><creatorcontrib>Reilly, E</creatorcontrib><creatorcontrib>Scalzo, R</creatorcontrib><creatorcontrib>Schmidt, B</creatorcontrib><creatorcontrib>Sim, S</creatorcontrib><creatorcontrib>Sollerman, J</creatorcontrib><creatorcontrib>Taddia, F</creatorcontrib><creatorcontrib>Tartaglia, L</creatorcontrib><creatorcontrib>Terreran, G</creatorcontrib><creatorcontrib>Tomasella, L</creatorcontrib><creatorcontrib>Turatto, M</creatorcontrib><creatorcontrib>Walker, E</creatorcontrib><creatorcontrib>Walton, N A</creatorcontrib><creatorcontrib>Wyrzykowski, L</creatorcontrib><creatorcontrib>Yuan, F</creatorcontrib><creatorcontrib>Zampieri, L</creatorcontrib><title>PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects</title><title>arXiv.org</title><description>The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction strategy and data products which are publicly available through the ESO archive as the Spectroscopic Survey Data Release 1 (SSDR1). PESSTO uses the New Technology Telescope with EFOSC2 and SOFI to provide optical and NIR spectroscopy and imaging. We target supernovae and optical transients brighter than 20.5mag for classification. Science targets are then selected for follow-up based on the PESSTO science goal of extending knowledge of the extremes of the supernova population. The EFOSC2 spectra cover 3345-9995A (at resolutions of 13-18 Angs) and SOFI spectra cover 0.935-2.53 micron (resolutions 23-33 Angs) along with JHK imaging. This data release contains spectra from the first year (April 2012 - 2013), consisting of all 814 EFOSC2 spectra and 95 SOFI spectra (covering 298 distinct objects), in standard ESO Phase 3 format. We estimate the accuracy of the absolute flux calibrations for EFOSC2 to be typically 15%, and the relative flux calibration accuracy to be about 5%. The PESSTO standard NIR reduction process does not yet produce high accuracy absolute spectrophotometry but the SOFI JHK imaging will improve this. Future data releases will focus on improving the automated flux calibration of the data products.</description><subject>Accuracy</subject><subject>Calibration</subject><subject>Data reduction</subject><subject>European Southern Observatory</subject><subject>Flux</subject><subject>Imaging</subject><subject>New technology</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><subject>Spectra</subject><subject>Spectrophotometry</subject><subject>Spectroscopy</subject><subject>Spectrum analysis</subject><subject>Supernovae</subject><subject>Target recognition</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2015</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotkMtqwzAQRUWh0JBm31UZ6NqpHn6luxLSBwQcsPdmZElUIbFdSQ71rp9eJ-lq4M7hMnMIeWB0GedJQp_R_djTksWMLSlfrW7IjAvBojzm_I4svN9TSnma8SQRM_K725RlVcAL-MGd9AhK-8bZPtiuBWwV9K5TQxM8GNcdIXxpMNb5AAoDgtMHjV6DHC-b3SAPtoFNWUDZ6ya4zjddPyXltbszUDlsvdVtgELuJ8Tfk1uDB68X_3NOqrdNtf6ItsX75_p1G2HCRCRjhSZlQknGzYobnqmcGcS8kTJTMhGiQcoyg1oKoQ0ayWKUinGaysxQKubk8Vp7sVP3zh7RjfXZUn22NAFPV2B6-HvQPtT7bnDtdFLNaS5SFudMiD8qxWyp</recordid><startdate>20150510</startdate><enddate>20150510</enddate><creator>Smartt, S J</creator><creator>Valenti, S</creator><creator>Fraser, M</creator><creator>Inserra, C</creator><creator>Young, D R</creator><creator>Sullivan, M</creator><creator>Pastorello, A</creator><creator>Benetti, S</creator><creator>Gal-Yam, A</creator><creator>Knapic, C</creator><creator>Molinaro, M</creator><creator>Smareglia, R</creator><creator>Smith, K W</creator><creator>Taubenberger, S</creator><creator>Yaron, O</creator><creator>Anderson, J P</creator><creator>Ashall, C</creator><creator>Balland, C</creator><creator>Baltay, C</creator><creator>Barbarino, C</creator><creator>Bauer, F E</creator><creator>Baumont, S</creator><creator>Bersier, D</creator><creator>Blagorodnova, N</creator><creator>Bongard, S</creator><creator>Botticella, M T</creator><creator>Bufano, F</creator><creator>Bulla, M</creator><creator>Cappellaro, E</creator><creator>Campbell, H</creator><creator>Cellier-Holzem, F</creator><creator>T -W Chen</creator><creator>Childress, M J</creator><creator>Clocchiatti, A</creator><creator>Contreras, C</creator><creator>M Dall Ora</creator><creator>Danziger, J</creator><creator>de Jaeger, T</creator><creator>De Cia, A</creator><creator>M Della Valle</creator><creator>Dennefeld, M</creator><creator>Elias-Rosa, N</creator><creator>Elman, N</creator><creator>Feindt, U</creator><creator>Fleury, M</creator><creator>Gall, E</creator><creator>Gonzalez-Gaitan, S</creator><creator>Galbany, L</creator><creator>A Morales Garoffolo</creator><creator>Greggio, L</creator><creator>Guillou, L L</creator><creator>Hachinger, S</creator><creator>Hadjiyska, E</creator><creator>Hage, P E</creator><creator>Hillebrandt, W</creator><creator>Hodgkin, S</creator><creator>Hsiao, E Y</creator><creator>James, P A</creator><creator>Jerkstrand, A</creator><creator>Kangas, T</creator><creator>Kankare, E</creator><creator>Kotak, R</creator><creator>Kromer, M</creator><creator>Kuncarayakti, H</creator><creator>Leloudas, G</creator><creator>Lundqvist, P</creator><creator>Lyman, J D</creator><creator>Hook, I M</creator><creator>Maguire, K</creator><creator>Manulis, I</creator><creator>Margheim, S J</creator><creator>Mattila, S</creator><creator>Maund, J R</creator><creator>Mazzali, P A</creator><creator>McCrum, M</creator><creator>McKinnon, R</creator><creator>Moreno-Raya, M E</creator><creator>Nicholl, M</creator><creator>Nugent, P</creator><creator>Pain, R</creator><creator>Phillips, M M</creator><creator>Pignata, G</creator><creator>Polshaw, J</creator><creator>Pumo, M L</creator><creator>Rabinowitz, D</creator><creator>Reilly, E</creator><creator>Scalzo, R</creator><creator>Schmidt, B</creator><creator>Sim, S</creator><creator>Sollerman, J</creator><creator>Taddia, F</creator><creator>Tartaglia, L</creator><creator>Terreran, G</creator><creator>Tomasella, L</creator><creator>Turatto, M</creator><creator>Walker, E</creator><creator>Walton, N A</creator><creator>Wyrzykowski, L</creator><creator>Yuan, F</creator><creator>Zampieri, L</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><scope>GOX</scope></search><sort><creationdate>20150510</creationdate><title>PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects</title><author>Smartt, S J ; Valenti, S ; Fraser, M ; Inserra, C ; Young, D R ; Sullivan, M ; Pastorello, A ; Benetti, S ; Gal-Yam, A ; Knapic, C ; Molinaro, M ; Smareglia, R ; Smith, K W ; Taubenberger, S ; Yaron, O ; Anderson, J P ; Ashall, C ; Balland, C ; Baltay, C ; Barbarino, C ; Bauer, F E ; Baumont, S ; Bersier, D ; Blagorodnova, N ; Bongard, S ; Botticella, M T ; Bufano, F ; Bulla, M ; Cappellaro, E ; Campbell, H ; Cellier-Holzem, F ; T -W Chen ; Childress, M J ; Clocchiatti, A ; Contreras, C ; M Dall Ora ; Danziger, J ; de Jaeger, T ; De Cia, A ; M Della Valle ; Dennefeld, M ; Elias-Rosa, N ; Elman, N ; Feindt, U ; Fleury, M ; Gall, E ; Gonzalez-Gaitan, S ; Galbany, L ; A Morales Garoffolo ; Greggio, L ; Guillou, L L ; Hachinger, S ; Hadjiyska, E ; Hage, P E ; Hillebrandt, W ; Hodgkin, S ; Hsiao, E Y ; James, P A ; Jerkstrand, A ; Kangas, T ; Kankare, E ; Kotak, R ; Kromer, M ; Kuncarayakti, H ; Leloudas, G ; Lundqvist, P ; Lyman, J D ; Hook, I M ; Maguire, K ; Manulis, I ; Margheim, S J ; Mattila, S ; Maund, J R ; Mazzali, P A ; McCrum, M ; McKinnon, R ; Moreno-Raya, M E ; Nicholl, M ; Nugent, P ; Pain, R ; Phillips, M M ; Pignata, G ; Polshaw, J ; Pumo, M L ; Rabinowitz, D ; Reilly, E ; Scalzo, R ; Schmidt, B ; Sim, S ; Sollerman, J ; Taddia, F ; Tartaglia, L ; Terreran, G ; Tomasella, L ; Turatto, M ; Walker, E ; Walton, N A ; Wyrzykowski, L ; Yuan, F ; Zampieri, L</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a513-b4daf613db12f92f27d81faa8cbb7db533ca017faeb33efafb14abd1206b7f003</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2015</creationdate><topic>Accuracy</topic><topic>Calibration</topic><topic>Data reduction</topic><topic>European Southern Observatory</topic><topic>Flux</topic><topic>Imaging</topic><topic>New technology</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><topic>Spectra</topic><topic>Spectrophotometry</topic><topic>Spectroscopy</topic><topic>Spectrum analysis</topic><topic>Supernovae</topic><topic>Target recognition</topic><toplevel>online_resources</toplevel><creatorcontrib>Smartt, S J</creatorcontrib><creatorcontrib>Valenti, S</creatorcontrib><creatorcontrib>Fraser, M</creatorcontrib><creatorcontrib>Inserra, C</creatorcontrib><creatorcontrib>Young, D R</creatorcontrib><creatorcontrib>Sullivan, M</creatorcontrib><creatorcontrib>Pastorello, A</creatorcontrib><creatorcontrib>Benetti, S</creatorcontrib><creatorcontrib>Gal-Yam, A</creatorcontrib><creatorcontrib>Knapic, C</creatorcontrib><creatorcontrib>Molinaro, M</creatorcontrib><creatorcontrib>Smareglia, R</creatorcontrib><creatorcontrib>Smith, K W</creatorcontrib><creatorcontrib>Taubenberger, S</creatorcontrib><creatorcontrib>Yaron, O</creatorcontrib><creatorcontrib>Anderson, J P</creatorcontrib><creatorcontrib>Ashall, C</creatorcontrib><creatorcontrib>Balland, C</creatorcontrib><creatorcontrib>Baltay, C</creatorcontrib><creatorcontrib>Barbarino, C</creatorcontrib><creatorcontrib>Bauer, F E</creatorcontrib><creatorcontrib>Baumont, S</creatorcontrib><creatorcontrib>Bersier, D</creatorcontrib><creatorcontrib>Blagorodnova, N</creatorcontrib><creatorcontrib>Bongard, S</creatorcontrib><creatorcontrib>Botticella, M T</creatorcontrib><creatorcontrib>Bufano, F</creatorcontrib><creatorcontrib>Bulla, M</creatorcontrib><creatorcontrib>Cappellaro, E</creatorcontrib><creatorcontrib>Campbell, H</creatorcontrib><creatorcontrib>Cellier-Holzem, F</creatorcontrib><creatorcontrib>T -W Chen</creatorcontrib><creatorcontrib>Childress, M J</creatorcontrib><creatorcontrib>Clocchiatti, A</creatorcontrib><creatorcontrib>Contreras, C</creatorcontrib><creatorcontrib>M Dall Ora</creatorcontrib><creatorcontrib>Danziger, J</creatorcontrib><creatorcontrib>de Jaeger, T</creatorcontrib><creatorcontrib>De Cia, A</creatorcontrib><creatorcontrib>M Della Valle</creatorcontrib><creatorcontrib>Dennefeld, M</creatorcontrib><creatorcontrib>Elias-Rosa, N</creatorcontrib><creatorcontrib>Elman, N</creatorcontrib><creatorcontrib>Feindt, U</creatorcontrib><creatorcontrib>Fleury, M</creatorcontrib><creatorcontrib>Gall, E</creatorcontrib><creatorcontrib>Gonzalez-Gaitan, S</creatorcontrib><creatorcontrib>Galbany, L</creatorcontrib><creatorcontrib>A Morales Garoffolo</creatorcontrib><creatorcontrib>Greggio, L</creatorcontrib><creatorcontrib>Guillou, L L</creatorcontrib><creatorcontrib>Hachinger, S</creatorcontrib><creatorcontrib>Hadjiyska, E</creatorcontrib><creatorcontrib>Hage, P E</creatorcontrib><creatorcontrib>Hillebrandt, W</creatorcontrib><creatorcontrib>Hodgkin, S</creatorcontrib><creatorcontrib>Hsiao, E Y</creatorcontrib><creatorcontrib>James, P A</creatorcontrib><creatorcontrib>Jerkstrand, A</creatorcontrib><creatorcontrib>Kangas, T</creatorcontrib><creatorcontrib>Kankare, E</creatorcontrib><creatorcontrib>Kotak, R</creatorcontrib><creatorcontrib>Kromer, M</creatorcontrib><creatorcontrib>Kuncarayakti, H</creatorcontrib><creatorcontrib>Leloudas, G</creatorcontrib><creatorcontrib>Lundqvist, P</creatorcontrib><creatorcontrib>Lyman, J D</creatorcontrib><creatorcontrib>Hook, I M</creatorcontrib><creatorcontrib>Maguire, K</creatorcontrib><creatorcontrib>Manulis, I</creatorcontrib><creatorcontrib>Margheim, S J</creatorcontrib><creatorcontrib>Mattila, S</creatorcontrib><creatorcontrib>Maund, J R</creatorcontrib><creatorcontrib>Mazzali, P A</creatorcontrib><creatorcontrib>McCrum, M</creatorcontrib><creatorcontrib>McKinnon, R</creatorcontrib><creatorcontrib>Moreno-Raya, M E</creatorcontrib><creatorcontrib>Nicholl, M</creatorcontrib><creatorcontrib>Nugent, P</creatorcontrib><creatorcontrib>Pain, R</creatorcontrib><creatorcontrib>Phillips, M M</creatorcontrib><creatorcontrib>Pignata, G</creatorcontrib><creatorcontrib>Polshaw, J</creatorcontrib><creatorcontrib>Pumo, M L</creatorcontrib><creatorcontrib>Rabinowitz, D</creatorcontrib><creatorcontrib>Reilly, E</creatorcontrib><creatorcontrib>Scalzo, R</creatorcontrib><creatorcontrib>Schmidt, B</creatorcontrib><creatorcontrib>Sim, S</creatorcontrib><creatorcontrib>Sollerman, J</creatorcontrib><creatorcontrib>Taddia, F</creatorcontrib><creatorcontrib>Tartaglia, L</creatorcontrib><creatorcontrib>Terreran, G</creatorcontrib><creatorcontrib>Tomasella, L</creatorcontrib><creatorcontrib>Turatto, M</creatorcontrib><creatorcontrib>Walker, E</creatorcontrib><creatorcontrib>Walton, N A</creatorcontrib><creatorcontrib>Wyrzykowski, L</creatorcontrib><creatorcontrib>Yuan, F</creatorcontrib><creatorcontrib>Zampieri, L</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</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><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Smartt, S J</au><au>Valenti, S</au><au>Fraser, M</au><au>Inserra, C</au><au>Young, D R</au><au>Sullivan, M</au><au>Pastorello, A</au><au>Benetti, S</au><au>Gal-Yam, A</au><au>Knapic, C</au><au>Molinaro, M</au><au>Smareglia, R</au><au>Smith, K W</au><au>Taubenberger, S</au><au>Yaron, O</au><au>Anderson, J P</au><au>Ashall, C</au><au>Balland, C</au><au>Baltay, C</au><au>Barbarino, C</au><au>Bauer, F E</au><au>Baumont, S</au><au>Bersier, D</au><au>Blagorodnova, N</au><au>Bongard, S</au><au>Botticella, M T</au><au>Bufano, F</au><au>Bulla, M</au><au>Cappellaro, E</au><au>Campbell, H</au><au>Cellier-Holzem, F</au><au>T -W Chen</au><au>Childress, M J</au><au>Clocchiatti, A</au><au>Contreras, C</au><au>M Dall Ora</au><au>Danziger, J</au><au>de Jaeger, T</au><au>De Cia, A</au><au>M Della Valle</au><au>Dennefeld, M</au><au>Elias-Rosa, N</au><au>Elman, N</au><au>Feindt, U</au><au>Fleury, M</au><au>Gall, E</au><au>Gonzalez-Gaitan, S</au><au>Galbany, L</au><au>A Morales Garoffolo</au><au>Greggio, L</au><au>Guillou, L L</au><au>Hachinger, S</au><au>Hadjiyska, E</au><au>Hage, P E</au><au>Hillebrandt, W</au><au>Hodgkin, S</au><au>Hsiao, E Y</au><au>James, P A</au><au>Jerkstrand, A</au><au>Kangas, T</au><au>Kankare, E</au><au>Kotak, R</au><au>Kromer, M</au><au>Kuncarayakti, H</au><au>Leloudas, G</au><au>Lundqvist, P</au><au>Lyman, J D</au><au>Hook, I M</au><au>Maguire, K</au><au>Manulis, I</au><au>Margheim, S J</au><au>Mattila, S</au><au>Maund, J R</au><au>Mazzali, P A</au><au>McCrum, M</au><au>McKinnon, R</au><au>Moreno-Raya, M E</au><au>Nicholl, M</au><au>Nugent, P</au><au>Pain, R</au><au>Phillips, M M</au><au>Pignata, G</au><au>Polshaw, J</au><au>Pumo, M L</au><au>Rabinowitz, D</au><au>Reilly, E</au><au>Scalzo, R</au><au>Schmidt, B</au><au>Sim, S</au><au>Sollerman, J</au><au>Taddia, F</au><au>Tartaglia, L</au><au>Terreran, G</au><au>Tomasella, L</au><au>Turatto, M</au><au>Walker, E</au><au>Walton, N A</au><au>Wyrzykowski, L</au><au>Yuan, F</au><au>Zampieri, L</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects</atitle><jtitle>arXiv.org</jtitle><date>2015-05-10</date><risdate>2015</risdate><eissn>2331-8422</eissn><abstract>The Public European Southern Observatory Spectroscopic Survey of Transient Objects (PESSTO) began as a public spectroscopic survey in April 2012. We describe the data reduction strategy and data products which are publicly available through the ESO archive as the Spectroscopic Survey Data Release 1 (SSDR1). PESSTO uses the New Technology Telescope with EFOSC2 and SOFI to provide optical and NIR spectroscopy and imaging. We target supernovae and optical transients brighter than 20.5mag for classification. Science targets are then selected for follow-up based on the PESSTO science goal of extending knowledge of the extremes of the supernova population. The EFOSC2 spectra cover 3345-9995A (at resolutions of 13-18 Angs) and SOFI spectra cover 0.935-2.53 micron (resolutions 23-33 Angs) along with JHK imaging. This data release contains spectra from the first year (April 2012 - 2013), consisting of all 814 EFOSC2 spectra and 95 SOFI spectra (covering 298 distinct objects), in standard ESO Phase 3 format. We estimate the accuracy of the absolute flux calibrations for EFOSC2 to be typically 15%, and the relative flux calibration accuracy to be about 5%. The PESSTO standard NIR reduction process does not yet produce high accuracy absolute spectrophotometry but the SOFI JHK imaging will improve this. Future data releases will focus on improving the automated flux calibration of the data products.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1411.0299</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2015-05 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_arxiv_primary_1411_0299 |
| source | arXiv.org; Freely Accessible Journals at publisher websites |
| subjects | Accuracy Calibration Data reduction European Southern Observatory Flux Imaging New technology Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics Spectra Spectrophotometry Spectroscopy Spectrum analysis Supernovae Target recognition |
| title | PESSTO : survey description and products from the first data release by the Public ESO Spectroscopic Survey of Transient Objects |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-25T06%3A31%3A50IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=PESSTO%20:%20survey%20description%20and%20products%20from%20the%20first%20data%20release%20by%20the%20Public%20ESO%20Spectroscopic%20Survey%20of%20Transient%20Objects&rft.jtitle=arXiv.org&rft.au=Smartt,%20S%20J&rft.date=2015-05-10&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1411.0299&rft_dat=%3Cproquest_arxiv%3E2083614813%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2083614813&rft_id=info:pmid/&rfr_iscdi=true |