The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe
ABSTRACT We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 no...
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| Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2022-03, Vol.512 (3), p.3195-3214 |
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| creator | Zheng, WeiKang Stahl, Benjamin E de Jaeger, Thomas Filippenko, Alexei V Wang, Shan-Qin Gan, Wen-Pei Brink, Thomas G Altunin, Ivan Baer-Way, Raphael Bigley, Andrew Blanchard, Kyle Blanchard, Peter K Bradley, James Cargill, Samantha K Casper, Chadwick Chapman, Teagan Chander, Vidhi Channa, Sanyum Choi, Byung Yun Choksi, Nick Chu, Matthew Clubb, Kelsey I Cohen, Daniel P Dalba, Paul A deGraw, Asia de Kouchkovsky, Maxime Ellison, Michael Falcon, Edward Fox, Ori D Fuller, Kiera Ganeshalingam, Mohan Girish, Nachiket Gould, Carolina Halevi, Goni Halle, Andrew Hayakawa, Kevin T Hardy, Romain Hestenes, Julia Hoffman, Andrew M Hyland, Michael Jeffers, Benjamin T Jennings, Connor Kandrashoff, Michael T Khodanian, Anthony Kim, Minkyu Kim, Haejung Kislak, Michelle E Krishnan, Daniel Kumar, Sahana Kumar, Snehaa Ganesh Leja, Joel Leonard, Erin J Li, Gary Z Li, Weidong Lian, Ji-Shun Liu, Evelyn Lowe, Thomas B Lu, Philip Ma, Emily Mason, Michelle N May, Michael McAllister, Kyle McGinness, Emma Modak, Shaunak Molloy, Jeffrey Murakami, Yukei S Nayak, Omnarayani Perera, Derek Pina, Kenia Punjabi, Druv Rikhter, Andrew Ross, Timothy W Sipple, Jackson Soler, Costas Stegman, Samantha Stephens, Haynes Sunseri, James Tang, Kevin Taylor, Stephen Thrasher, Patrick Van Dyk, Schuyler D Wang, Xiang-Gao Wayland, Jeremy Wilkins, Andrew Yagubyan, Abel Yuk, Heechan Yunus, Sameen Zhang, Keto D |
| description | ABSTRACT
We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 normal SNe Ic, 1 peculiar SN Ic, 10 SNe Ic-BL, 15 SNe IIb, 1 ambiguous SN IIb/Ib/c, and 2 superluminous SNe. Our follow-up photometry has (on a per-SN basis) a mean coverage of 81 photometric points (median of 58 points) and a mean cadence of 3.6 d (median of 1.2 d). From our full sample, a subset of 38 SNe have pre-maximum coverage in at least one passband, allowing for the peak brightness of each SN in this subset to be quantitatively determined. We describe our data collection and processing techniques, with emphasis toward our automated photometry pipeline, from which we derive publicly available data products to enable and encourage further study by the community. Using these data products, we derive host-galaxy extinction values through the empirical colour evolution relationship and, for the first time, produce accurate rise-time measurements for a large sample of SESNe in both optical and infrared passbands. By modelling multiband light curves, we find that SNe Ic tend to have lower ejecta masses and lower ejecta velocities than SNe Ib and IIb, but higher 56Ni masses. |
| doi_str_mv | 10.1093/mnras/stac723 |
| format | Article |
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We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 normal SNe Ic, 1 peculiar SN Ic, 10 SNe Ic-BL, 15 SNe IIb, 1 ambiguous SN IIb/Ib/c, and 2 superluminous SNe. Our follow-up photometry has (on a per-SN basis) a mean coverage of 81 photometric points (median of 58 points) and a mean cadence of 3.6 d (median of 1.2 d). From our full sample, a subset of 38 SNe have pre-maximum coverage in at least one passband, allowing for the peak brightness of each SN in this subset to be quantitatively determined. We describe our data collection and processing techniques, with emphasis toward our automated photometry pipeline, from which we derive publicly available data products to enable and encourage further study by the community. Using these data products, we derive host-galaxy extinction values through the empirical colour evolution relationship and, for the first time, produce accurate rise-time measurements for a large sample of SESNe in both optical and infrared passbands. By modelling multiband light curves, we find that SNe Ic tend to have lower ejecta masses and lower ejecta velocities than SNe Ib and IIb, but higher 56Ni masses.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/stac723</identifier><language>eng</language><publisher>United States: Oxford University Press</publisher><subject>ASTRONOMY AND ASTROPHYSICS ; distances and redshifts ; galaxies ; supernovae</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2022-03, Vol.512 (3), p.3195-3214</ispartof><rights>2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society 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(LBNL), Berkeley, CA (United States)</creatorcontrib><title>The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe</title><title>Monthly notices of the Royal Astronomical Society</title><description>ABSTRACT
We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 normal SNe Ic, 1 peculiar SN Ic, 10 SNe Ic-BL, 15 SNe IIb, 1 ambiguous SN IIb/Ib/c, and 2 superluminous SNe. Our follow-up photometry has (on a per-SN basis) a mean coverage of 81 photometric points (median of 58 points) and a mean cadence of 3.6 d (median of 1.2 d). From our full sample, a subset of 38 SNe have pre-maximum coverage in at least one passband, allowing for the peak brightness of each SN in this subset to be quantitatively determined. We describe our data collection and processing techniques, with emphasis toward our automated photometry pipeline, from which we derive publicly available data products to enable and encourage further study by the community. Using these data products, we derive host-galaxy extinction values through the empirical colour evolution relationship and, for the first time, produce accurate rise-time measurements for a large sample of SESNe in both optical and infrared passbands. By modelling multiband light curves, we find that SNe Ic tend to have lower ejecta masses and lower ejecta velocities than SNe Ib and IIb, but higher 56Ni masses.</description><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>distances and redshifts</subject><subject>galaxies</subject><subject>supernovae</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNqF0DtPwzAUhmELgUQojOwWE0uoL4njsKGqXKSKDikbUuQ4xySQxJHtFvXfE2h3prM8-qTzInRNyR0lOZ_3g1N-7oPSGeMnKKJcpDHLhThFESE8jWVG6Tm68P6TEJJwJiL0vmkAr1r9hdeVB7dTwbo9LrYjuMHuFC5AOd1gY7vOfsfbEY_OfjjV3-OxscH2ECZeq6Cwgw6UB2wNzggulsUrXKIzozoPV8c7Q2-Py83iOV6tn14WD6tYJ4SFuBaszhMm04QkNWMsTQVNZE5JCpSbSnDGDaTCVEaCJkpWlVHMQM2nF7Ssgc_QzWHX-tCWXrcBdKPtMIAOJZUyYZmcUHxA2lnvHZhydG2v3L6kpPztV_71K4_9Jn97HN2O_9AfQ1dzdQ</recordid><startdate>20220331</startdate><enddate>20220331</enddate><creator>Zheng, WeiKang</creator><creator>Stahl, 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Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe</title><author>Zheng, WeiKang ; Stahl, Benjamin E ; de Jaeger, Thomas ; Filippenko, Alexei V ; Wang, Shan-Qin ; Gan, Wen-Pei ; Brink, Thomas G ; Altunin, Ivan ; Baer-Way, Raphael ; Bigley, Andrew ; Blanchard, Kyle ; Blanchard, Peter K ; Bradley, James ; Cargill, Samantha K ; Casper, Chadwick ; Chapman, Teagan ; Chander, Vidhi ; Channa, Sanyum ; Choi, Byung Yun ; Choksi, Nick ; Chu, Matthew ; Clubb, Kelsey I ; Cohen, Daniel P ; Dalba, Paul A ; deGraw, Asia ; de Kouchkovsky, Maxime ; Ellison, Michael ; Falcon, Edward ; Fox, Ori D ; Fuller, Kiera ; Ganeshalingam, Mohan ; Girish, Nachiket ; Gould, Carolina ; Halevi, Goni ; Halle, Andrew ; Hayakawa, Kevin T ; Hardy, Romain ; Hestenes, Julia ; Hoffman, Andrew M ; Hyland, Michael ; Jeffers, Benjamin T ; Jennings, Connor ; Kandrashoff, Michael T ; Khodanian, Anthony ; Kim, Minkyu ; Kim, Haejung ; Kislak, Michelle E ; Krishnan, Daniel ; Kumar, Sahana ; Kumar, Snehaa Ganesh ; Leja, Joel ; Leonard, Erin J ; Li, Gary Z ; Li, Weidong ; Lian, Ji-Shun ; Liu, Evelyn ; Lowe, Thomas B ; Lu, Philip ; Ma, Emily ; Mason, Michelle N ; May, Michael ; McAllister, Kyle ; McGinness, Emma ; Modak, Shaunak ; Molloy, Jeffrey ; Murakami, Yukei S ; Nayak, Omnarayani ; Perera, Derek ; Pina, Kenia ; Punjabi, Druv ; Rikhter, Andrew ; Ross, Timothy W ; Sipple, Jackson ; Soler, Costas ; Stegman, Samantha ; Stephens, Haynes ; Sunseri, James ; Tang, Kevin ; Taylor, Stephen ; Thrasher, Patrick ; Van Dyk, Schuyler D ; Wang, Xiang-Gao ; Wayland, Jeremy ; Wilkins, Andrew ; Yagubyan, Abel ; Yuk, Heechan ; Yunus, Sameen ; Zhang, Keto D</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c402t-d62d94285404d2225561489105e13fb6323fe56fbf8ec0a8bbfa2fed3432c8de3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>ASTRONOMY AND ASTROPHYSICS</topic><topic>distances and redshifts</topic><topic>galaxies</topic><topic>supernovae</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Zheng, WeiKang</creatorcontrib><creatorcontrib>Stahl, Benjamin E</creatorcontrib><creatorcontrib>de Jaeger, Thomas</creatorcontrib><creatorcontrib>Filippenko, Alexei V</creatorcontrib><creatorcontrib>Wang, Shan-Qin</creatorcontrib><creatorcontrib>Gan, Wen-Pei</creatorcontrib><creatorcontrib>Brink, Thomas G</creatorcontrib><creatorcontrib>Altunin, Ivan</creatorcontrib><creatorcontrib>Baer-Way, Raphael</creatorcontrib><creatorcontrib>Bigley, Andrew</creatorcontrib><creatorcontrib>Blanchard, Kyle</creatorcontrib><creatorcontrib>Blanchard, Peter K</creatorcontrib><creatorcontrib>Bradley, James</creatorcontrib><creatorcontrib>Cargill, Samantha K</creatorcontrib><creatorcontrib>Casper, Chadwick</creatorcontrib><creatorcontrib>Chapman, Teagan</creatorcontrib><creatorcontrib>Chander, Vidhi</creatorcontrib><creatorcontrib>Channa, Sanyum</creatorcontrib><creatorcontrib>Choi, Byung Yun</creatorcontrib><creatorcontrib>Choksi, Nick</creatorcontrib><creatorcontrib>Chu, Matthew</creatorcontrib><creatorcontrib>Clubb, Kelsey I</creatorcontrib><creatorcontrib>Cohen, Daniel P</creatorcontrib><creatorcontrib>Dalba, Paul A</creatorcontrib><creatorcontrib>deGraw, Asia</creatorcontrib><creatorcontrib>de Kouchkovsky, Maxime</creatorcontrib><creatorcontrib>Ellison, Michael</creatorcontrib><creatorcontrib>Falcon, Edward</creatorcontrib><creatorcontrib>Fox, Ori D</creatorcontrib><creatorcontrib>Fuller, Kiera</creatorcontrib><creatorcontrib>Ganeshalingam, Mohan</creatorcontrib><creatorcontrib>Girish, Nachiket</creatorcontrib><creatorcontrib>Gould, Carolina</creatorcontrib><creatorcontrib>Halevi, Goni</creatorcontrib><creatorcontrib>Halle, Andrew</creatorcontrib><creatorcontrib>Hayakawa, Kevin T</creatorcontrib><creatorcontrib>Hardy, Romain</creatorcontrib><creatorcontrib>Hestenes, Julia</creatorcontrib><creatorcontrib>Hoffman, Andrew M</creatorcontrib><creatorcontrib>Hyland, Michael</creatorcontrib><creatorcontrib>Jeffers, Benjamin T</creatorcontrib><creatorcontrib>Jennings, Connor</creatorcontrib><creatorcontrib>Kandrashoff, Michael T</creatorcontrib><creatorcontrib>Khodanian, Anthony</creatorcontrib><creatorcontrib>Kim, Minkyu</creatorcontrib><creatorcontrib>Kim, Haejung</creatorcontrib><creatorcontrib>Kislak, Michelle E</creatorcontrib><creatorcontrib>Krishnan, Daniel</creatorcontrib><creatorcontrib>Kumar, Sahana</creatorcontrib><creatorcontrib>Kumar, Snehaa Ganesh</creatorcontrib><creatorcontrib>Leja, Joel</creatorcontrib><creatorcontrib>Leonard, Erin J</creatorcontrib><creatorcontrib>Li, Gary Z</creatorcontrib><creatorcontrib>Li, Weidong</creatorcontrib><creatorcontrib>Lian, Ji-Shun</creatorcontrib><creatorcontrib>Liu, Evelyn</creatorcontrib><creatorcontrib>Lowe, Thomas B</creatorcontrib><creatorcontrib>Lu, Philip</creatorcontrib><creatorcontrib>Ma, Emily</creatorcontrib><creatorcontrib>Mason, Michelle N</creatorcontrib><creatorcontrib>May, Michael</creatorcontrib><creatorcontrib>McAllister, Kyle</creatorcontrib><creatorcontrib>McGinness, Emma</creatorcontrib><creatorcontrib>Modak, Shaunak</creatorcontrib><creatorcontrib>Molloy, Jeffrey</creatorcontrib><creatorcontrib>Murakami, Yukei S</creatorcontrib><creatorcontrib>Nayak, Omnarayani</creatorcontrib><creatorcontrib>Perera, Derek</creatorcontrib><creatorcontrib>Pina, Kenia</creatorcontrib><creatorcontrib>Punjabi, Druv</creatorcontrib><creatorcontrib>Rikhter, Andrew</creatorcontrib><creatorcontrib>Ross, Timothy W</creatorcontrib><creatorcontrib>Sipple, Jackson</creatorcontrib><creatorcontrib>Soler, Costas</creatorcontrib><creatorcontrib>Stegman, Samantha</creatorcontrib><creatorcontrib>Stephens, Haynes</creatorcontrib><creatorcontrib>Sunseri, James</creatorcontrib><creatorcontrib>Tang, Kevin</creatorcontrib><creatorcontrib>Taylor, Stephen</creatorcontrib><creatorcontrib>Thrasher, Patrick</creatorcontrib><creatorcontrib>Van Dyk, Schuyler D</creatorcontrib><creatorcontrib>Wang, Xiang-Gao</creatorcontrib><creatorcontrib>Wayland, Jeremy</creatorcontrib><creatorcontrib>Wilkins, Andrew</creatorcontrib><creatorcontrib>Yagubyan, Abel</creatorcontrib><creatorcontrib>Yuk, Heechan</creatorcontrib><creatorcontrib>Yunus, Sameen</creatorcontrib><creatorcontrib>Zhang, Keto D</creatorcontrib><creatorcontrib>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Zheng, WeiKang</au><au>Stahl, Benjamin E</au><au>de Jaeger, Thomas</au><au>Filippenko, Alexei V</au><au>Wang, Shan-Qin</au><au>Gan, Wen-Pei</au><au>Brink, Thomas G</au><au>Altunin, Ivan</au><au>Baer-Way, Raphael</au><au>Bigley, Andrew</au><au>Blanchard, Kyle</au><au>Blanchard, Peter K</au><au>Bradley, James</au><au>Cargill, Samantha K</au><au>Casper, Chadwick</au><au>Chapman, Teagan</au><au>Chander, Vidhi</au><au>Channa, Sanyum</au><au>Choi, Byung Yun</au><au>Choksi, Nick</au><au>Chu, Matthew</au><au>Clubb, Kelsey I</au><au>Cohen, Daniel P</au><au>Dalba, Paul A</au><au>deGraw, Asia</au><au>de Kouchkovsky, Maxime</au><au>Ellison, Michael</au><au>Falcon, Edward</au><au>Fox, Ori D</au><au>Fuller, Kiera</au><au>Ganeshalingam, Mohan</au><au>Girish, Nachiket</au><au>Gould, Carolina</au><au>Halevi, Goni</au><au>Halle, Andrew</au><au>Hayakawa, Kevin T</au><au>Hardy, Romain</au><au>Hestenes, Julia</au><au>Hoffman, Andrew M</au><au>Hyland, Michael</au><au>Jeffers, Benjamin T</au><au>Jennings, Connor</au><au>Kandrashoff, Michael T</au><au>Khodanian, Anthony</au><au>Kim, Minkyu</au><au>Kim, Haejung</au><au>Kislak, Michelle E</au><au>Krishnan, Daniel</au><au>Kumar, Sahana</au><au>Kumar, Snehaa Ganesh</au><au>Leja, Joel</au><au>Leonard, Erin J</au><au>Li, Gary Z</au><au>Li, Weidong</au><au>Lian, Ji-Shun</au><au>Liu, Evelyn</au><au>Lowe, Thomas B</au><au>Lu, Philip</au><au>Ma, Emily</au><au>Mason, Michelle N</au><au>May, Michael</au><au>McAllister, Kyle</au><au>McGinness, Emma</au><au>Modak, Shaunak</au><au>Molloy, Jeffrey</au><au>Murakami, Yukei S</au><au>Nayak, Omnarayani</au><au>Perera, Derek</au><au>Pina, Kenia</au><au>Punjabi, Druv</au><au>Rikhter, Andrew</au><au>Ross, Timothy W</au><au>Sipple, Jackson</au><au>Soler, Costas</au><au>Stegman, Samantha</au><au>Stephens, Haynes</au><au>Sunseri, James</au><au>Tang, Kevin</au><au>Taylor, Stephen</au><au>Thrasher, Patrick</au><au>Van Dyk, Schuyler D</au><au>Wang, Xiang-Gao</au><au>Wayland, Jeremy</au><au>Wilkins, Andrew</au><au>Yagubyan, Abel</au><au>Yuk, Heechan</au><au>Yunus, Sameen</au><au>Zhang, Keto D</au><aucorp>Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>2022-03-31</date><risdate>2022</risdate><volume>512</volume><issue>3</issue><spage>3195</spage><epage>3214</epage><pages>3195-3214</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>ABSTRACT
We present BVRI and unfiltered (Clear) light curves of 70 stripped-envelope supernovae (SESNe), observed between 2003 and 2020, from the Lick Observatory Supernova Search follow-up program. Our SESN sample consists of 19 spectroscopically normal SNe Ib, 2 peculiar SNe Ib, six SNe Ibn, 14 normal SNe Ic, 1 peculiar SN Ic, 10 SNe Ic-BL, 15 SNe IIb, 1 ambiguous SN IIb/Ib/c, and 2 superluminous SNe. Our follow-up photometry has (on a per-SN basis) a mean coverage of 81 photometric points (median of 58 points) and a mean cadence of 3.6 d (median of 1.2 d). From our full sample, a subset of 38 SNe have pre-maximum coverage in at least one passband, allowing for the peak brightness of each SN in this subset to be quantitatively determined. We describe our data collection and processing techniques, with emphasis toward our automated photometry pipeline, from which we derive publicly available data products to enable and encourage further study by the community. Using these data products, we derive host-galaxy extinction values through the empirical colour evolution relationship and, for the first time, produce accurate rise-time measurements for a large sample of SESNe in both optical and infrared passbands. By modelling multiband light curves, we find that SNe Ic tend to have lower ejecta masses and lower ejecta velocities than SNe Ib and IIb, but higher 56Ni masses.</abstract><cop>United States</cop><pub>Oxford University Press</pub><doi>10.1093/mnras/stac723</doi><tpages>20</tpages><orcidid>https://orcid.org/0000-0002-7232-101X</orcidid><orcidid>https://orcid.org/0000-0002-5257-1804</orcidid><orcidid>https://orcid.org/0000-0003-2238-1572</orcidid><orcidid>https://orcid.org/0000-0002-0094-9182</orcidid><orcidid>https://orcid.org/0000-0003-0690-1056</orcidid><orcidid>https://orcid.org/0000-0002-9955-8797</orcidid><orcidid>https://orcid.org/0000-0002-3169-3167</orcidid><orcidid>https://orcid.org/0000-0002-5221-2342</orcidid><orcidid>https://orcid.org/0000-0001-6755-1315</orcidid><orcidid>https://orcid.org/0000-0002-8342-3804</orcidid><orcidid>https://orcid.org/0000-0001-9038-9950</orcidid><orcidid>https://orcid.org/0000-0002-4297-5506</orcidid><orcidid>https://orcid.org/0000000231693167</orcidid><orcidid>https://orcid.org/0000000167551315</orcidid><orcidid>https://orcid.org/0000000190389950</orcidid><orcidid>https://orcid.org/000000027232101X</orcidid><orcidid>https://orcid.org/0000000299558797</orcidid><orcidid>https://orcid.org/0000000200949182</orcidid><orcidid>https://orcid.org/0000000252212342</orcidid><orcidid>https://orcid.org/0000000242975506</orcidid><orcidid>https://orcid.org/0000000306901056</orcidid><orcidid>https://orcid.org/0000000283423804</orcidid><orcidid>https://orcid.org/0000000322381572</orcidid><orcidid>https://orcid.org/0000000252571804</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | ISSN: 0035-8711 |
| ispartof | Monthly notices of the Royal Astronomical Society, 2022-03, Vol.512 (3), p.3195-3214 |
| issn | 0035-8711 1365-2966 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1884278 |
| source | Oxford Open |
| subjects | ASTRONOMY AND ASTROPHYSICS distances and redshifts galaxies supernovae |
| title | The Lick Observatory Supernova Search follow-up program: photometry data release of 70 SESNe |
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