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The Palomar Transient Factory: System Overview, Performance, and First Results
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The Palomar Transient Factory (PTF) is a fully-automated, wide-field survey aimed at a systematic exploration of the optical transient sky. The transient survey is performed using a new 8.1 square degree camera installed on the 48 inch Samuel Oschin telescope at Palomar Observatory; colors and light curves for detected transients are obtained with the automated Palomar 60 inch telescope. PTF uses 80% of the 1.2 m and 50% of the 1.5 m telescope time. With an exposure of 60 s the survey reaches a depth of m g ′ ≈ 21.3 and m R ≈ 20.6 (5σ, median seeing). Four major experiments are planned for the five-year project: (1) a 5 day cadence supernova search; (2) a rapid transient search with cadences between 90 s and 1 day; (3) a search for eclipsing binaries and transiting planets in Orion; and (4) a 3π sr deep H-alpha survey. PTF provides automatic, real-time transient classification and follow-up, as well as a database including every source detected in each frame. This paper summarizes the PTF project, including several months of on-sky performance tests of the new survey camera, the observing plans, and the data reduction strategy. We conclude by detailing the first 51 PTF optical transient detections, found in commissioning data.
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“Recent surveys have shown the power of measuring variability of celestial sources for studying gravitational lensing, searching for SNe, determining the physical properties of gamma-ray burst sources, discovering gravitational wave counterparts, probing the structure of active galactic nuclei ( AGNs ) , studying variable star populations, discovering exoplanets, and many other subjects at the fore”
From LSST: From Science Drivers to Reference Design and Anticipated Data Products (2019) · cites this paper as Law et al. 2009
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Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
Self-citationAstronomical Data Analysis Software and Systems
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Self-citationThe Palomar-Quest Digital Synoptic Sky SurveyPreprint
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Self-citationAutomated Probabilistic Classification of Transients and VariablesPreprint
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Self-citationTowards a real‐time transient classification engine
Bloom, J. S., Starr, D., Butler, N., Nugent, P., Rischard, M., Eads, D. R., & Poznanski, D. (2008) · Astronomische Nachrichten · doi:10.1002/asna.200710957 · Cited by 22 · cited 2×
“The Bayesian framework for event clustering is given in Bloom et al. (2008).”
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Lyu, J., Rieke, G. H., & Smith, P. S. (2019) · The Astrophysical Journal · doi:10.3847/1538-4357/ab481d · Cited by 74
Deciphering the extreme X-ray variability of the nuclear transient eRASSt J045650.3−203750
Liu, T., Malyali, A., Krumpe, M., Homan, D., Goodwin, A. J., Grotova, I., Kawka, A., Rau, A., Merloni, A., Anderson, G. E., et al. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202244805 · Cited by 74
Self-citationEnvironment-derived constraints on the progenitors of low-luminosity Type I supernovae★
Lyman, J. D., James, P. A., Perets, H. B., Anderson, J. P., Gal‐Yam, A., Mazzali, P. A., & Percival, S. M. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1038 · Cited by 74
“The former identified eight SNe in this group (SN2000ds, SN2001co, SN2003H, SN2003dg, SN2003dr, SN2005cz, SN2005E and SN2007ke) and the latter identified three additional objects in this class from the Palomar Transient Factory survey (Law et al. 2009; Rau et al. 2009, henceforth PTF).”
BackgroundSelf-citationTHE SUBLUMINOUS AND PECULIAR TYPE Ia SUPERNOVA PTF 09dav
Sullivan, M., Kasliwal, M. M., Nugent, P., Howell, D. A., Thomas, R. C., Ofek, E. O., Arcavi, I., Blake, S., Cooke, J., Gal‐Yam, A., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/732/2/118 · Cited by 74
“This SN was discovered as part of the Palomar Transient Factory (PTF14; Rau et al. 2009; Law et al. 2009), a five year project surveying the optically transient sky.”
BackgroundSelf-citationIdeas for Citizen Science in Astronomy
Marshall, P. J., Lintott, C. J., & Fletcher, L. N. (2015) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081913-035959 · Cited by 84
“Data from the Palomar Transient Factory (Law et al. 2009) was automatically processed and images of candidate supernovae uploaded on a nightly basis; this triggered an email to volunteers who, upon responding, were shown the new image, a reference image and the difference between the two.”
MethodThe superluminous supernova PS1-11ap: bridging the gap between low and high redshift
McCrum, M. G., Smartt, S. J., Kotak, R., Rest, A., Jerkstrand, A., Inserra, C., Rodney, S., Chen, T. W., Howell, D. A., Huber, M. E., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1923 · Cited by 73
“Recent wide field surveys, such as the Palomar Transient Factory (PTF) (Law et al. 2009; Rau et al. 2009) and Pan-STARRS1 (PS1) (Kaiser et al. 2010) have uncovered that the schema for classifying the highly luminous and energetic endpoints of massive stars known as supernovae (SNe) may be more…”
BackgroundSelf-citationSystematically Bridging the Gap Between Novae and Supernovae
Kasliwal, M. M. (2012) · Publications of the Astronomical Society of Australia · doi:10.1071/as11061 · Cited by 73
“The Palomar Transient Factory is a fully automated, wide-field survey aimed at a systematic exploration of explosions and variable phenomena in optical wavelengths.”
MethodSelf-citationSupernova spectra below strong circumstellar interaction
Leloudas, G., Hsiao, E. Y., Johansson, J., Maeda, K., Moriya, T. J., Nordin, J., Petrushevska, T., Silverman, J. M., Sollerman, J., Stritzinger, M. D., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201322035 · Cited by 73
“Silverman et al. (2013) reported on the discovery of additional SNe Ia-CSM in archival and Palomar Transient Factory (PTF; Law et al. 2009) data, raising the total number to 16 objects.”
BackgroundThe Palomar Transient Factory photometric catalog 1.0
Ofek, E. O., Laher, R., Surace, J., Levitan, D., Sesar, B., Horesh, A., Law, N., van Eyken, J. C., Kulkarni, S. R., Prince, T. A., et al. (2012) · Publications of the Astronomical Society of the Pacific · doi:10.1086/666978 · Cited by 72
“The Palomar Transient Factory15 (PTF; Law et al. 2009; Rau et al. 2009) is a synoptic survey designed to explore the transient sky and to study stellar variability.”
BackgroundSelf-citationTHE INFRARED LIGHT CURVE OF SN 2011fe IN M101 AND THE DISTANCE TO M101
Matheson, T., Joyce, R. R., Allen, L. E., Saha, A., Silva, D. R., Wood‐Vasey, W. M., Adams, J. J., Anderson, R. E., Beck, T. L., Bentz, M. C., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/754/1/19 · Cited by 72
“Supernova (SN) 2011fe was discovered soon after explosion in the nearby galaxy M101 (NGC 5457) by the Palomar Transient Factory (Rau et al. 2009; Law et al. 2009) on 2011 August 24.167 UT (all calendar dates herein are UT) and rapidly classified as a supernova of Type Ia (SN Ia; Nugent et al.…”
BackgroundInfluentialSecond-generation microlensing planet surveys: a realistic simulation
Shvartzvald, Y., & Maoz, D. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.20014.x · Cited by 71
“(iv) The Palomar Observatory 1.2m Oschin telescope in California with the PTF camera, with a 7.8 deg2 field of view (Law et al. 2009) and a cadence of ∼40 minutes.”
MethodInfluentialBen-Ami, S., Gal‐Yam, A., Mazzali, P. A., Gnat, O., Modjaz, M., Rabinak, I., Sullivan, M., Bildsten, L., Poznanski, D., Yaron, O., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/785/1/37 · Cited by 71
Self-citationTHE HOST GALAXIES OF FAST-EJECTA CORE-COLLAPSE SUPERNOVAE
Kelly, P. L., Filippenko, A. V., Modjaz, M., & Kocevski, D. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/789/1/23 · Cited by 70
“We study the host galaxies of both nearby (z < 0.2) core-collapse SNe discovered by “galaxy-untargeted” transient searches (e.g., the Palomar Transient Factory (PTF); Rau et al. 2009; Law et al. 2009), which do not target specific potential hosts or z < 1.2 LGRBs detected by γ -ray satellites.”
BackgroundInfluentialSelf-citationKOOLS–IFU: Kyoto Okayama Optical Low-dispersion Spectrograph with optical-fiber Integral Field Unit
Matsubayashi, K., Ohta, K., Iwamuro, F., Iwata, I., Kambe, E., Tsutsui, H., Izumiura, H., Yoshida, M., & Hattori, T. (2019) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psz087 · Cited by 70
CHIMERA: a wide-field, multi-colour, high-speed photometer at the prime focus of the Hale telescope
Harding, L. K., Hallinan, G., Milburn, J., Gardner, P., Konidaris, N. P., Singh, N., Shao, M., Sandhu, J. S., Kyne, G., & Schlichting, H. E. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw094 · Cited by 70
“…binaries, flaring stars, pulsing white dwarfs and transiting planets, and will be well placed for follow-up observations of short-duration transients discovered by the intermediate Palomar Transient Factory (iPTF, Law et al. 2009; Rau et al. 2009), and the upcoming Zwicky Transient Facility (ZTF)2.”
BackgroundiPTF 16asu: A Luminous, Rapidly Evolving, and High-velocity Supernova
Whitesides, L., Lunnan, R., Kasliwal, M., Perley, D., Corsi, A., Cenko, S. B., Blagorodnova, N., Cao, Y., Cook, D., Doran, G., et al. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa99de · Cited by 58
“The Intermediate Palomar Transient Factory project is a scientific collaboration among the California Institute of Technology; Los Alamos National Laboratory; the University of Wisconsin, Milwaukee; the Oskar Klein Center; the Weizmann Institute of Science; the TANGO Program of the University System of Taiwan; and the…”
MethodInfluentialSelf-citationSesar, B., Stuart, J. S., Ivezić, Ž., Morgan, D. P., Becker, A. C., & Woźniak, P. R. (2011) · The Astronomical Journal · doi:10.1088/0004-6256/142/6/190
“• The Palomar Transient Factory (PTF;Law et al. 2009 and Rau et al. 2009) is an on- going wide-area, two-band (SDSS-g′ and Mould-R filters), deep (R ∼ 20.6, g′ ∼ 21.3) survey aimed at systematic exploration of the optical transient sky.”
BackgroundInfluential1000 cataclysmic variables from the Catalina Real-time Transient Survey
Breedt, E., Gänsicke, B. T., Drake, A. J., Rodríguez-Gil, P., Parsons, S. G., Marsh, T. R., Szkody, P., Schreiber, M. R., & Djorgovski, S. G. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu1377 · Cited by 69
“…active large area transient surveys include the Catalina Realtime Transient Survey (CRTS, Drake et al. 2009), the Palomar Transient Factory (PTF, Law et al. 2009), the Mobile Astronomical System of the Telescope Robots (MASTER, Lipunov et al. 2010) and the All Sky Automated Survey (ASAS,…”
BackgroundSelf-citationFIRST SEARCHES FOR OPTICAL COUNTERPARTS TO GRAVITATIONAL-WAVE CANDIDATE EVENTS
Aasi, J., Abadie, J., Abbott, B. P., Abbott, R., Abbott, T. D., Abernathy, M. R., Accadia, T., Acernese, F., Adams, C., Adams, T., et al. (2014) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/211/1/7 · Cited by 68
Intermediate Palomar Transient Factory: Realtime Image Subtraction Pipeline
Cao, Y., Nugent, P. E., & Kasliwal, M. M. (2016) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/128/969/114502 · Cited by 68
“Since 2013, as the successor of PTF (Law et al. 2009), iPTF have been performing several fast-cadence experiments to systematically search for and characterize young SNe and fast-evolving transients.”
BackgroundSelf-citationThe ANTARES Astronomical Time-domain Event Broker
Matheson, T., Stubens, C., Wolf, N., Lee, C., Narayan, G., Saha, A., Scott, A., Soraisam, M., Bolton, A. S., Hauger, B., et al. (2021) · The Astronomical Journal · doi:10.3847/1538-3881/abd703 · Cited by 68
EXPANDED VERY LARGE ARRAY OBSERVATIONS OF THE RADIO EVOLUTION OF SN 2011dh
Krauss, M. I., Soderberg, A. M., Chomiuk, L., Zauderer, B. A., Brunthaler, A., Bietenholz, M. F., Chevalier, R. A., Fransson, C., & Rupen, M. (2012) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/750/2/l40 · Cited by 68
“However, rapid optical followup observations from the Palomar Transient Factory (Law et al. 2009) pointed to a compact progenitor star, as evidenced by its short-lived (∆t ≈ 1 day) coolingenvelope emission (Arcavi et al. 2011).”
BackgroundCensus of the Local Universe (CLU) Narrowband Survey. I. Galaxy Catalogs from Preliminary Fields
Cook, D., Kasliwal, M., Sistine, A. V., Kaplan, D., Sutter, J., Kupfer, T., Shupe, D., Laher, R., Masci, F., Dale, D., et al. (2017) · Astrophysical Journal · doi:10.3847/1538-4357/ab2131 · Cited by 54
Self-citationSuyu, S. H., Huber, S., Cañameras, R., Kromer, M., Schuldt, S., Taubenberger, S., Yıldırım, A., Bonvin, V., Chan, J. H. H., Courbin, F., et al. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202037757 · Cited by 68
“Two years after the SN Refsdal event was the first discovery of a strongly lensed Type Ia SN by Goobar et al. (2017) in the intermediate Palomar Transient Factory (Law et al. 2009), namely the iPTF16geu system.”
BackgroundGreen, P. J., Pulgarin-Duque, L., Anderson, S. F., MacLeod, C. L., Eracleous, M., Ruan, J. J., Runnoe, J. C., Graham, M. J., Roulston, B. R., Schneider, D. P., et al. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac743f · Cited by 67
“We obtained g- and r-band photometry from the following sources: Pan-STARRS1 (PS1; Kaiser et al. 2010), Palomar Transient Factory (PTF; Law et al. 2009), Zwicky Transient Facility (ZTF; Bellm et al. 2019) Data Release 3 and SDSS (York et al. 2000).”
MethodTHE UNUSUAL TEMPORAL AND SPECTRAL EVOLUTION OF THE TYPE IIn SUPERNOVA 2011ht
Roming, P. W. A., Pritchard, T. A., Prieto, J. L., Kochanek, C. S., Fryer, C. L., Davidson, K., Humphreys, R. M., Bayless, A. J., Beacom, J. F., Brown, P. J., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/751/2/92 · Cited by 66
“…dedicated SNe follow-up programs and telescopes (e.g., Filippenko et al. 2001; Bloom et al. 2006; Hamuy et al. 2006; Quimby 2006; Drake et al. 2009; Law et al. 2009; Rau et al. 2009), SNe IIn are now being studied more frequently in both the optical and near-IR (e.g., Pastorello et al. 2002;…”
BackgroundA GRANULATION “FLICKER”-BASED MEASURE OF STELLAR SURFACE GRAVITY
Bastien, F. A., Stassun, K. G., Basri, G., & Pepper, J. A. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/818/1/43 · Cited by 67
“Wide-field photometric surveys, such as the Palomar Transient Factory (PTF; Law et al. 2009), Pan-STARRS (Jewitt 2003), and the Large Synoptic Survey Telescope (LSST; Becker et al. 2007) are becoming a larger part of astronomical science and would initially seem to be potential sources of flicker…”
BackgroundEldridge, J. J., Xiao, L., Stanway, E. R., Rodrigues, N., & Guo, N. (2018) · Publications of the Astronomical Society of Australia · doi:10.1017/pasa.2018.47 · Cited by 66
“However, SNe are more likely to be found early with the current generation of automated surveys (e.g. Law et al. 2009; Shappee et al. 2012) which also observe sources over an extended period with a well-defined cadence.”
BackgroundEnvironments of interacting transients: impostors and Type IIn supernovae
Habergham, S. M., Anderson, J. P., James, P. A., & Lyman, J. D. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu684 · Cited by 66
“Silverman et al. (2013) studied SNIIn detected by the Palomar Transient Factory (PTF; Rau et al. 2009; Law et al. 2009) and found that ∼10 per cent of explosions classified as SNIIn were more likely to be thermonuclear supernovae, interacting with a dense CSM.”
BackgroundSN 2010jp (PTF10aaxi): a jet in a Type II supernova
Smith, N., Cenko, S. B., Butler, N., Bloom, J. S., Kasliwal, M. M., Horesh, A., Kulkarni, S. R., Law, N. M., Nugent, P., Ofek, E. O., et al. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.20104.x · Cited by 66
“SN 2010jp (PTFaaxi) SN 2010jp was discovered on 2010 Nov. 11.3 by Maza et al. (2010), and was found independently on 2010 Nov. 16 as PTF10aaxi in the course of the Palomar Transient Factory (PTF; Law et al. 2009; Rau et al. 2009), as we describe below.”
MethodInfluentialSelf-citationPTF 10fqs: A LUMINOUS RED NOVA IN THE SPIRAL GALAXY MESSIER 99
Kasliwal, M. M., Kulkarni, S. R., Arcavi, I., Quimby, R. M., Ofek, E. O., Nugent, P., Jacobsen, J., Gal-Yam, A., Green, Y., Yaron, O., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/730/2/134 · Cited by 66
“(e.g. Bildsten et al. 2007; Metzger et al. 2009; Shen et al. 2010; Moriya et al. 2010) The Palomar Transient Factory2 (PTF; see Rahmer et al. 2008; Law et al. 2009; Rau et al. 2009) was designed to undertake a systematic exploration of the transient sky in the optical bands.”
BackgroundSelf-citationThe ASAS-SN bright supernova catalogue – I. 2013–2014
Holoien, T. W. S., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Prieto, J. L., Brimacombe, J. R., Bersier, D., Bishop, D. W., Dong, S., Brown, J. S., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw2273 · Cited by 66
“…Transient Survey (CRTS; Drake et al. 2009), the CHilean Automatic Supernova sEarch (CHASE; Pignata et al. 2009), the Palomar Transient Factory (PTF; Law et al. 2009), the Gaia transient survey (Hodgkin et al. 2013), the La Silla-QUEST (LSQ) Low Redshift Supernova Survey (Baltay et al. 2013), the…”
BackgroundFrohmaier, C., Angus, C. R., Vincenzi, M., Sullivan, M., Smith, M., Nugent, P., Cenko, S. B., Gal‐Yam, A., Kulkarni, S. R., Law, N. M., et al. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa3607 · Cited by 66
Self-citationTRACING THE ORPHAN STREAM TO 55 kpc WITH RR LYRAE STARS
Sesar, B., Grillmair, C. J., Cohen, J. G., Bellm, E. C., Bhalerao, V., Levitan, D., Laher, R. R., Ofek, E. O., Surace, J., Tang, S., et al. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/776/1/26 · Cited by 64
“The PTF11 (Law et al. 2009; Rau et al. 2009) is a synoptic survey designed to explore the transient sky.”
BackgroundSelf-citationTartaglia, L., Pastorello, A., Sullivan, M., Baltay, C., Rabinowitz, D. L., Nugent, P., Drake, A. J., Djorgovski, S. G., Gal‐Yam, A., Fabrika, S., et al. (2016) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stw675 · Cited by 65
“Archival data from different surveys, namely LSQ, the Intermediate Palomar Transient Factory (iPTF4; Law et al. 2009; Rau et al. 2009, where the transient was designated as iPTF13ajw) and the Catalina Real-Time Transient Survey (CRTS5; Drake et al. 2009; Djorgovski et al. 2012) revealed an outburst…”
MethodSelf-citationDISCOVERY AND REDSHIFT OF AN OPTICAL AFTERGLOW IN 71 deg 2 : iPTF13bxl AND GRB 130702A
Singer, L. P., Cenko, S. B., Kasliwal, M. M., Perley, D. A., Ofek, E. O., Brown, D. A., Nugent, P., Kulkarni, S. R., Corsi, A., Frail, D. A., et al. (2013) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/776/2/l34 · Cited by 65
“The Palomar Transient Factory (PTF; Law et al. 2009) is developing the necessary instrumentation, algorithms, and observational discipline to detect optical counterparts to GBM GRBs.”
BackgroundSelf-citationGone without a bang: an archivalHSTsurvey for disappearing massive stars
Reynolds, T., Fraser, M., & Gilmore, G. F. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1809 · Cited by 65
“Within our distance limit, systematic surveys such as the Catalina Real Time Transient Survey (Drake et al. 2009), the Palomar Transient Survey (Law et al. 2009), the Lick Observatory SN Search (Leaman et al. 2011), PanSTARRS-1 (Kaiser et al. 2010) and ASAS-SN (Shappee et al. 2014) ensure that most SNe are detected (a…”
BackgroundPTF1 J071912.13+485834.0: AN OUTBURSTING AM CVn SYSTEM DISCOVERED BY A SYNOPTIC SURVEY
Levitan, D., Fulton, B. J., Groot, P., Kulkarni, S. R., Ofek, E. O., Prince, T. A., Shporer, A., Bloom, J. S., Cenko, S. B., Kasliwal, M. M., et al. (2011) · The Astrophysical Journal · doi:10.1088/0004-637x/739/2/68 · Cited by 65
“In a typical night, up to ∼ 2, 000 deg2 are observed to a depth of R ∼ 20.6 (Law et al. 2009; Rau et al. 2009).”
BackgroundInfluentialSelf-citationHillenbrand, L. A., Miller, A. A., Covey, K. R., Carpenter, J. M., Cenko, S. B., Silverman, J. M., Muirhead, P. S., Fischer, W. J., Crepp, J. R., Bloom, J. S., et al. (2013) · The Astronomical Journal · doi:10.1088/0004-6256/145/3/59 · Cited by 65
“PTF 10nvg, in the North America Nebula region of recent star formation, was identified by the Palomar Transient Factory (PTF; Law et al. 2009; Rau et al. 2009) on 2010 July 8, as an optical transient based on automatic discovery and classification codes (Bloom et al. 2011).”
BackgroundMethodSelf-citationCorsi, A., Gal‐Yam, A., Kulkarni, S. R., Frail, D. A., Mazzali, P. A., Cenko, S. B., Kasliwal, M. M., Cao, Y., Horesh, A., Palliyaguru, N., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/830/1/42 · Cited by 65
“…of 15 SNe discovered by the Palomar Transient Factory and/or intermediate Palomar Transient Factory (PTF/iPTF, hereafter we use PTF for simplicity; Law et al. 2009; Rau et al. 2009), optimized to search for off-axis GRBs, namely, a sample of BLIcs selected blindly in random galaxies (mostly…”
MethodSelf-citationJiang, J.-A., Doi, M., Maeda, K., & Shigeyama, T. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aadb9a · Cited by 65
SN2019dge: A Helium-rich Ultra-stripped Envelope Supernova
Yao, Y.-H., De, K., Kasliwal, M., Ho, A., Schulze, S., Li, Z.-H., Kulkarni, S., Fruchter, A., Rubin, D., Perley, D., et al. (2020) · Astrophysical Journal · doi:10.3847/1538-4357/abaa3d · Cited by 49
“We also performed forced photometry on archival PTF/iPTF difference images spanning 2009 May 07 to 2016 Jun 13 (Law et al. 2009; Rau et al. 2009).”
MethodSelf-citationiPTF14yb: THE FIRST DISCOVERY OF A GAMMA-RAY BURST AFTERGLOW INDEPENDENT OF A HIGH-ENERGY TRIGGER
Cenko, S. B., Urban, A. L., Perley, D. A., Horesh, A., Corsi, A., Fox, D. B., Cao, Y., Kasliwal, M. M., Lien, A. Y., Arcavi, I., et al. (2015) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/803/2/l24 · Cited by 64
“To that end, we present here the discovery by the Intermediate Palomar Transient Factory (iPTF; Law et al. 2009) of iPTF14yb, a luminous (Mr ≈ −27.8 mag), rapidly fading optical transient at redshift z = 1.9733.”
MethodInfluentialSelf-citationMiller, A. A., Cao, Y., Piro, A. L., Blagorodnova, N., Bue, B. D., Cenko, S. B., Dhawan, S., Ferretti, R., Fox, O. D., Fremling, C., et al. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aaa01f · Cited by 64
“17 Survey observations were conducted with the CFH12K camera (Rahmer et al. 2008) on the Palomar Observatory 48-inch telescope (P48; Law et al. 2009).”
MethodSelf-citationTaggart, K., & Perley, D. A. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab174 · Cited by 64
“…SN catalogues exist, including the Dark Energy Survey (Flaugher 2005), Catalina Real-Time Survey (Drake et al. 2009), the Palomar Transient Factory (Law et al. 2009), SuperNova Legacy Survey (Bazin et al. 2009), Pan-STARRS (Kaiser et al. 2002), La Silla Quest (Hadjiyska et al. 2012), the Gaia…”
MethodAN ACCRETING WHITE DWARF NEAR THE CHANDRASEKHAR LIMIT IN THE ANDROMEDA GALAXY
Tang, S., Bildsten, L., Wolf, W. M., Li, K. L., Kong, A. K. H., Cao, Y., Cenko, S. B., Cia, A. D., Kasliwal, M. M., Kulkarni, S. R., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/786/1/61 · Cited by 63
“During our nightly monitoring of M31 in the intermediate Palomar Transient Factory (iPTF; hereafter called simply PTF; Law et al. 2009), we discovered a transient at the location of a known nova in M31 (Tang et al. 2013), and confirmed it to be a RN with a recurrence time of 1yr with four optical…”
BackgroundSelf-citationWhimper of a Bang: Documenting the Final Days of the Nearby Type Ia Supernova 2011fe
Shappee, B. J., Stanek, K. Z., Kochanek, C. S., & Garnavich, P. M. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/aa6eab · Cited by 63
“SN 2011fe was discovered less than one day after the explosion by the Palomar Transient Factory (Law et al. 2009) in a sparse region of the outer disk of the well-studied, face-on spiral M101.”
BackgroundLIMB-DARKENING COEFFICIENTS FOR ECLIPSING WHITE DWARFS
Gianninas, A., Strickland, B. D., Kilic, M., & Bergeron, P. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/766/1/3 · Cited by 63
“In the future, we expect projects like the Large Synoptic Survey Telescope (LSST; Ivezic et al. 2008), Palomar Transient Factory (PTF; Law et al. 2009; Rau et al. 2009), and Panoramic Survey Telescope and Rapid Response System (Pan-STARRS; Tonry et al. 2012) to uncover thousands of new eclipsing…”
BackgroundPROPERTIES AND EVOLUTION OF THE REDBACK MILLISECOND PULSAR BINARY PSR J2129–0429
Bellm, E. C., Kaplan, D. L., Breton, R. P., Phinney, E. S., Bhalerao, V. B., Camilo, F., Dahal, S., Djorgovski, S. G., Drake, A. J., Hessels, J. W. T., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/816/2/74 · Cited by 63
“In Figure 8 we show the LINEAR, CRTS, PTF, P60 r¢, and LCOGT r¢ photometry from 2003–2014.”
MethodInfluentialSelf-citationThe bumpy light curve of Type IIn supernova iPTF13z over 3 years
Nyholm, A., Sollerman, J., Taddia, F., Fremling, C., Moriya, T. J., Ofek, E. O., Gal-Yam, A., Cia, A. D., Roy, R., Kasliwal, M. M., et al. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201629906 · Cited by 63
“The transient iPTF13z was first detected in an image taken in the Mould R band (Law et al. 2009) on 2013 February 1.48 UT1 with the 1.2 m Samuel Oschin telescope (P48; Rahmer et al. 2008) on Palomar Mountain (California, USA).”
MethodInfluentialSelf-citationTHE TIME DOMAIN SPECTROSCOPIC SURVEY: VARIABLE SELECTION AND ANTICIPATED RESULTS
Morganson, E., Green, P. J., Anderson, S. F., Ruan, J. J., Myers, A. D., Eracleous, M., Kelly, B. C., Badenes, C., Bañados, E., Blanton, M. R., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/806/2/244 · Cited by 62
“…in the Southern Hemisphere (Hadjiyska et al. 2012), the Catalina Sky Survey (Drake et al. 2009), the Palomar Transient Factory (PTF, Law et al. 2009), All-Sky Automated Survey (ASAS, Pojmanski 2002), the Lincoln Near-Earth Asteroid Research survey (LINEAR, Palaversa et al. 2013)…”
The ASAS-SN bright supernova catalogue – III. 2016
Holoien, T. W. S., Brown, J. S., Stanek, K. Z., Kochanek, C. S., Shappee, B. J., Prieto, J. L., Dong, S., Brimacombe, J. R., Bishop, D. W., Bose, S., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1544 · Cited by 62
The very energetic, broad-lined Type Ic supernova 2010ah (PTF10bzf) in the context of GRB/SNe
Mazzali, P. A., Walker, E. S., Pian, E., Tanaka, M., Corsi, A., Hattori, T., & Gal‐Yam, A. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt605 · Cited by 62
“The bright, broad-lined SNIc SN2010ah was discovered by the Palomar Transient Factory (PTF, Law et al. 2009; Rau et al. 2009) on 23 Feb 2010 in a galaxy at a redshift z = 0 .”
Self-citationModjaz, M., Bianco, F., Siwek, M., Huang, S., Perley, D., Fierroz, D., Liu, Y., Arcavi, I., Gal-yam, A., Filippenko, A., et al. (2019) · Astrophysical Journal · doi:10.3847/1538-4357/ab4185 · Cited by 49
Self-citationFrohmaier, C., Sullivan, M., Nugent, P., Smith, M., Dimitriadis, G., Bloom, J. S., Cenko, S. B., Kasliwal, M. M., Kulkarni, S. R., Maguire, K., et al. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz807 · Cited by 62
“Largearea rolling surveys, such as the Palomar Transient Factory (PTF; Rau et al. 2009; Law et al. 2009), the Catalina Real-Time Transient Survey (CRTS Drake et al. 2009), PanSTARRS (Kaiser et al. 2010), the La Silla Quest Variability Survey (Baltay et al. 2013), the All-Sky Automated Survey for…”
BackgroundSelf-citationSheng, Z., Wang, T., Jiang, N., Ding, J., Cai, Z., Guo, H., Sun, L., Dou, L., & Yang, C. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab5af9 · Cited by 61
Berkeley Supernova Ia Program – V. Late-time spectra of Type Ia Supernovae
Silverman, J. M., Ganeshalingam, M., & Filippenko, A. V. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts674 · Cited by 61
“…et al. 2012) has gathered, published, and analysed their SN Ia spectral data, larger transient searches such as the Palomar Transient Factory (PTF; Rau et al. 2009; Law et al. 2009) and Pan-STARRS (Kaiser et al. 2002) will be able to add significantly to the number of late-time SN Ia spectra.”
MethodSelf-citationZackay, B., & Ofek, E. O. (2017) · The Astrophysical Journal · doi:10.3847/1538-4357/836/2/187 · Cited by 61
“Coaddition is playing, and will play, a major role in ongoing and future surveys (e.g., SDSS, York et al. 2000; PanSTARRS, Kaiser et al. 2002; PTF, Law et al. 2009, DES, The Dark Energy Survey Collaboration 2005; LSST, Ivezic et al. 2008).”
BackgroundMethodSelf-citationInteracting supernovae from wide massive binary systems
Ercolino, A., Jin, H., Langer, N., & Dessart, L. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202347646 · Cited by 60
A UV resonance line echo from a shell around a hydrogen-poor superluminous supernova
Lunnan, R., Fransson, C., Vreeswijk, P. M., Woosley, S. E., Leloudas, G., Perley, D. A., Quimby, R., Yan, L., Blagorodnova, N., Bue, B., et al. (2018) · Nature Astronomy · doi:10.1038/s41550-018-0568-z · Cited by 60
Self-citationAn extremely energetic supernova from a very massive star in a dense medium
Nicholl, M., Blanchard, P. K., Berger, E., Chornock, R., Margutti, R., Gómez, S., Lunnan, R., Miller, A. A., Fong, W., Terreran, G., et al. (2020) · Nature Astronomy · doi:10.1038/s41550-020-1066-7 · Cited by 60
“n lines at a redshift of z =0:2657, and hence an absolute magnitude of M = 22:5 0:08mag at the time of discovery (Methods). A search of archival images from the intermediate Palomar Transient Factory [11] revealed a rising light curve going back to at least 2015 December 02 UT, with maximum brightness on 2016 January…”
BackgroundSelf-citationType IIn supernova light-curve properties measured from an untargeted survey samplE
Nyholm, A., Sollerman, J., Tartaglia, L., Taddia, F., Fremling, C., Blagorodnova, N., Filippenko, A. V., Gal‐Yam, A., Howell, D. A., Karamehmetoglu, E., et al. (2020) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201936097/pdf · Cited by 60
Self-citationAbbott, B. P., Abbott, R., Abbott, T. M. C., Abernathy, M. R., Acernese, F., Ackley, K., Adams, C., Adams, T., Addesso, P., Adhikari, R. X., et al. (2016) · The Astrophysical Journal Supplement Series · doi:10.3847/0067-0049/225/1/8 · Cited by 59
Yao, Y., Lu, W., Guolo, M., Pasham, D. R., Gezari, S., Гильфанов, М. Р., Gendreau, K. C., Harrison, F. A., Cenko, S. B., Kulkarni, S. R., et al. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac898a · Cited by 59
“…Sky Survey (SDSS, Alam et al. 2015), the All-Sky Automated Survey for SuperNovae (ASAS-SN; Shappee et al. 2014), the Palomar Transient Factory (PTF; Law et al. 2009; Rau et al. 2009), the intermediate PTF (iPTF), the Asteroid Terrestrialimpact Last Alert System (Tonry et al. 2018), and the Zwicky…”
BackgroundSelf-citationNEWT: A RESTful service for building High Performance Computing web applications
Cholia, S., Skinner, D. E., & Boverhof, J. (2010) · Grid Computing Environments · doi:10.1109/gce.2010.5676125 · Cited by 59
Neutrinos from Choked Jets Accompanied by Type-II Supernovae
He, H.-N., Kusenko, A., Nagataki, S., Fan, Y.-Z., & Wei, D.-M. (2018) · The Astrophysical Journal · doi:10.3847/1538-4357/aab360 · Cited by 59
“…al. 2012; Aartsen et al. 2015c), namely the Robotic Optical Transient Search Experiment (ROTSE; Akerlof et al. 2003), the Palomar Transient Factory (Law et al. 2009; Rau et al. 2009), and the Swift satellite (Gehrels et al. 2004), as well as the Subaru Hyper-Suprime-Cam with a field of view (FOV)…”
BackgroundVery high-energy gamma-ray follow-up program using neutrino triggers from IceCube
IceCube Collaboration, Aartsen, M. G., Abraham, K., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., Andeen, K., et al. (2016) · Journal of Instrumentation · doi:10.1088/1748-0221/11/11/p11009 · Cited by 58
“5◦ (angular resolution), from any direction) alerts are sent to the Robotic Optical Transient Search Experiment (ROTSE) [31]1 and the Palomar Transient Factory (PTF) [32] for optical observations, and to Swift [33, 34] for X-ray follow-up, depending on the multiplet’s significance.”
BackgroundInfluentialcatsHTM: A Tool for Fast Accessing and Cross-matching Large Astronomical Catalogs
Soumagnac, M. T., & Ofek, E. O. (2018) · Publications of the Astronomical Society of the Pacific · doi:10.1088/1538-3873/aac410 · Cited by 58
“For example, surveys like Pan-STARRS (Chambers et al. 2016) and the Palomar Transient Factory (Law et al. 2009) generated a large number of transient candidates which have to be cross-matched with multiple catalogs in order to be vetted, classified and followed up.”
MethodSelf-citationOPTICAL AND NEAR-INFRARED OBSERVATIONS OF SN 2013DX ASSOCIATED WITH GRB 130702A
Toy, V., Cenko, S. B., Silverman, J. M., Butler, N., Cucchiara, A., Watson, A. M., Bersier, D., Perley, D. A., Margutti, R., Bellm, E. C., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/818/1/79 · Cited by 58
“Employing the wide-field imaging and rapid transient identification capabilities of the Intermediate Palomar Transient Factory (iPTF; Law et al. 2009; Rau et al. 2009), Singer et al. (2013b) discovered the optical afterglow of GRB 130702A.”
MethodSelf-citationDIGITAL ACCESS TO A SKY CENTURY AT HARVARD: INITIAL PHOTOMETRY AND ASTROMETRY
Laycock, S., Tang, S., Grindlay, J. E., Los, E., Simcoe, R., & Mink, J. D. (2010) · The Astronomical Journal · doi:10.1088/0004-6256/140/4/1062 · Cited by 58
“Time domain astronomy is undergoing a revolution, with new dedicated facilities such as ASAS (Pojmanski 1997), Pan-STARRS (Kaiser et al. 2002), and the Palomar Transient Factory (Law et al. 2009) recently coming on line, and LSST Claver et al. (2004) on the near horizon.”
Hachinger, S., Mazzali, P. A., Sullivan, M., Ellis, R. S., Maguire, K., Gal‐Yam, A., Howell, D. A., Nugent, P., Baron, E., Cooke, J., et al. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts492 · Cited by 58
“We also make use of five ground-based optical spectra, taken with Gemini-N with GMOS and the William Herschel Telescope 1 Discoverers of PTF10ygu in ‘Galaxy Zoo Supernovae’: Peter Woolliams, tracey, Graham Dungworth, lpspieler, John P Langridge, Elisabeth Baeten, Tomas Raudys, adam elbourne, Robert Gagliano.”
MethodInfluentialSelf-citationBen-Ami, S., Gal‐Yam, A., Filippenko, A. V., Mazzali, P. A., Modjaz, M., Yaron, O., Arcavi, I., Cenko, S. B., Horesh, A., Howell, D. A., et al. (2012) · The Astrophysical Journal Letters · doi:10.1088/2041-8205/760/2/l33 · Cited by 58
“The Palomar Transient Factory (PTF; Law et al. 2009; Rau et al. 2009) is a wide-field untargeted sky survey which explores the transient optical sky.”
BackgroundSelf-citationTHE HIGH CADENCE TRANSIENT SURVEY (HITS). I. SURVEY DESIGN AND SUPERNOVA SHOCK BREAKOUT CONSTRAINTS
Förster, F., Maureira, J. C., Martín, J. S., Hamuy, M., Martínez-Palomera, J., Huijse, P., Cabrera-Vives, G., Galbany, L., de Jaeger, T., González-Gaitán, S., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/832/2/155 · Cited by 58
“The advent of a new generation of large field–of– view astronomical optical CCD cameras already operational (e.g. iPTF, Law et al. 2009; SkyMapper, Keller et al. 2007; Pan–STARRS, Hodapp et al. 2004; OmegaCam, Kuijken et al. 2002; DECam, Flaugher et al. 2015; Hyper Suprime–Cam, Furusawa et al.…”
BackgroundSelf-citationDeep-learnt classification of light curves
Mahabal, A. A., Sheth, K. N., Gieseke, F. C., Pai, A., Djorgovski, S. G., Drake, A. J., & Graham, M. J. (2017) · IEEE Symposium Series on Computational Intelligence (SSCI) · doi:10.1109/ssci.2017.8280984 · Cited by 71
“We demonstrate this on a set of variables from CRTS-S a Southern set corresponding to the main training set used here [10], and corresponding PTF data [11].”
MethodSelf-citationMachine learning search for variable stars
Pashchenko, I. N., Sokolovsky, K. V., & Gavras, P. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx3222 · Cited by 57
“…et al. 2017), NMW (Sokolovsky, Korotkiy & Lebedev 2014), NSVS (Woźniak et al. 2004), Pan-STARRS (Kaiser et al. 2010, Chambers et al. 2016), PTF (Law et al. 2009), SuperWASP (Butters et al. 2010), TrES (Alonso et al. 2007), VVV (Minniti et al. 2010) with even 19 https://www.aavso.org/vsx/ c©…”
iPTF SEARCH FOR AN OPTICAL COUNTERPART TO GRAVITATIONAL-WAVE TRANSIENT GW150914
Kasliwal, M. M., Cenko, S. B., Singer, L. P., Corsi, A., Cao, Y., Barlow, T., Bhalerao, V., Bellm, E., Cook, D., Duggan, G. E., et al. (2016) · The Astrophysical Journal Letters · doi:10.3847/2041-8205/824/2/l24 · Cited by 57
“Here, we present the intermediate Palomar Transient Factory (iPTF) follow-up effort. iPTF uses the Samuel Oschin 48-inch telescope on Palomar mountain equipped with the CFH12K camera with a field-of-view of 7.1 deg2 (Law et al. 2009).”
MethodInfluentialSelf-citationTEMPLATE RR LYRAE Hα, Hβ, AND Hγ VELOCITY CURVES
Sesar, B. (2012) · The Astronomical Journal · doi:10.1088/0004-6256/144/4/114 · Cited by 56
“Then there are multi-epoch, wide-area surveys such as the LINEAR (Sesar et al. 2011) and PTF (Law et al. 2009), which are currently finding thousands of RR Lyrae stars within 30 kpc from the Sun (Sesar 2011).”
Long-term photometric behaviour of outbursting AM CVn systems
Levitan, D., Groot, P., Prince, T. A., Kulkarni, S. R., Laher, R. R., Ofek, E. O., Sesar, B., & Surace, J. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2105 · Cited by 57
“SDSSJ1721+2733 Porb = 38.1 min HJD(t0) = 2456078.0 −10 0 10 20 30 40 50 60 70 16 17 18 19 20 CRTSJ0450–0931 Porb = 47.3 min HJD(t0) = 2456253.9 −10 0 10 20 30 40 50 60 70 15 16 17 18 19 20 PTF1J1523+1845 HJD(t0) = 2455384.8 −10 0 10 20 30 40 50 60 70 18 19 20 21 22 23 SDSSJ1240–0159 Porb = 37.4 min HJD(t0) = 2453469.8…”
MethodInfluentialSelf-citationPTF10ops - a subluminous, normal-width light curve Type Ia supernova in the middle of nowhere
Maguire, K., Sullivan, M., Thomas, R. C., Nugent, P., Howell, D. A., Gal‐Yam, A., Arcavi, I., Ben-Ami, S., Blake, S., Botyanszki, J., et al. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19526.x · Cited by 57
“In this paper, we present the discovery and analysis of the SN Ia, PTF10ops, which was discovered by the Palomar TransientFactory (PTF, Rau et al. 2009; Law et al. 2009).”
MethodSelf-citationMULTIWAVELENGTH OBSERVATIONS OF THE REDBACK MILLISECOND PULSAR J1048+2339
Deneva, J. S., Ray, P. S., Camilo, F., Halpern, J. P., Wood, K. S., Cromartie, H. T., Ferrara, E. C., Kerr, M. T., Ransom, S. M., Wolff, M. T., et al. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/823/2/105 · Cited by 57
“PSRJ1048+2339 has a 20th magnitude optical counterpart detected by SDSS, CRTS, PTF, and Pan-STARRS, whose intensity modulation matches the pulsar orbital period.”
MethodInfluentialBOLOMETRIC AND UV LIGHT CURVES OF CORE-COLLAPSE SUPERNOVAE
Pritchard, T. A., Roming, P. W. A., Brown, P. J., Bayless, A. J., & Frey, L. H. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/787/2/157 · Cited by 56
“…Infrared Imaging Telescope (Bloom et al. 2006), Caltech Core Collapse Program(Gal-Yam et al. 2007), Palomar Transient Factory (Rau et al. 2009; Law et al. 2009), and the efforts of the Center for Astrophysics Supernova (SN) Group, nearby CCSNe are now being more frequently monitored in both…”
BackgroundSilverman, J. M., Ganeshalingam, M., Li, W., & Filippenko, A. V. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.21526.x · Cited by 56
“New large-scale surveys are already obtaining SN Ia data, and they are observing to higher redshifts and gathering larger amounts of data than what is in the BSNIP sample (e.g., Rau et al. 2009; Law et al. 2009; Kaiser et al. 2002).”
BackgroundSelf-citationREVEALING TYPE Ia SUPERNOVA PHYSICS WITH COSMIC RATES AND NUCLEAR GAMMA RAYS
Horiuchi, S., & Beacom, J. F. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/723/1/329 · Cited by 56
“With next-generation surveys such as the Palomar Transient Factory (Law et al. 2009), SNIa measurements are becoming more complete.”
MethodBellm, E. C., & Kulkarni, S. R. (2017) · Nature Astronomy · doi:10.1038/s41550-017-0071 · Cited by 56
Self-citationDiscovery of the Luminous, Decades-long, Extragalactic Radio Transient FIRST J141918.9+394036
Law, C. J., Gaensler, B. M., Metzger, B. D., Ofek, E. O., & Sironi, L. (2018) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/aae5f3 · Cited by 56
“Today, a new generation of highenergy, optical, and radio sky surveys are being conducted with a focus on sensitivity to time-domain phenomena like supernovae and GRBs (Gehrels et al. 2004; Law et al. 2009; Mooley et al. 2016).”
BackgroundSelf-citationChen, Z., Yan, L., Kangas, T., Lunnan, R., Schulze, S., Sollerman, J., Perley, D. A., Chen, T. W., Taggart, K., Hinds, K.-R., et al. (2023) · The Astrophysical Journal · doi:10.3847/1538-4357/aca161 · Cited by 55
“For example, the Palomar Transient Factory (PTF; Law et al. 2009), the PanSTARRS1 Medium Deep Survey (PS1 MDS; Chambers et al. 2016), the Catalina Real-time Transient Survey (Drake et al. 2009), the All-Sky Automated Survey for SuperNovae (ASASSN; Shappee 2014), the Dark Energy Survey (DES; The…”
MethodSelf-citationAbbasi, R. U., Abdou, Y., Abu-Zayyad, T., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Allen, M. M., Altmann, D., Andeen, K., et al. (2012) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201118071 · Cited by 55
“Because of the successful operation of the optical followup program with ROTSE, the program was extended in August 2010 to the Palomar transient factory (PTF) (Law et al. 2009; Rau et al. 2009), which will provide deeper images and a fast processing pipeline including a spectroscopic follow-up of interesting SN candid…”
MethodWalker, E. S., Hook, I., Sullivan, M., Howell, D. A., Astier, P., Balland, C., Basa, S., Bronder, T. J., Carlberg, R. G., Conley, A., et al. (2010) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2010.17519.x · Cited by 55
“Current and future surveys such as the Nearby Supernova Factory (Aldering et al. 2002), Palomar Transient Factory (Law et al. 2009), SkyMapper (Keller et al. 2007) and Pan-STARRS (Kaiser 2004) will largely address this problem.”
MethodSelf-citationGraham, M. L., Nugent, P., Sullivan, M., Filippenko, A. V., Cenko, S. B., Silverman, J. M., Clubb, K. I., & Zheng, W. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1888 · Cited by 55
“SN 2011fe was discovered by the Palomar Transient Factory (Rau et al. 2009; Law et al. 2009) within hours of its explosion on 23.7 Aug. 2011 (dates are UT throughout this paper) and spectroscopically classified as a normal SN Ia (Nugent et al. 2011).”
BackgroundInfluentialSelf-citationCovey, K. R., Agüeros, M. A., Law, N. M., Liu, J., Ahmadi, A., Laher, R. R., Levitan, D., Sesar, B., & Surace, J. (2016) · The Astrophysical Journal · doi:10.3847/0004-637x/822/2/81 · Cited by 55
“The PTF infrastructure is described in Law et al. (2009); we focus here on the components associated with the P48, which we used to conduct our monitoring campaign.”
MethodSelf-citationCovariate-Assisted Ranking and Screening for Large-Scale Two-Sample Inference
Cai, T., Sun, W., & Wang, W. (2019) · Journal of the Royal Statistical Society Series B (Statistical Methodology) · doi:10.1111/rssb.12304 · Cited by 55
Determining the recurrence time-scale of long-lasting YSO outbursts
Peña, C. C., Naylor, T., & Morrell, S. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz1019 · Cited by 55
“However, the addition of literature data and inspection of images provided by the Palomar Transient Factory (PTF Law et al. 2009) reveals that the faint R magnitudes are probably part of the “normal” variability of the source, which seems to be characterised by irregular, short-term variability…”
BackgroundFast luminous blue transients from newborn black holes
Kashiyama, K., & Quataert, E. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1164 · Cited by 55
“The above properties are broadly consistent with some of the rapid blue transients detected by Pan-STARRS and PTF.”
BackgroundInfluentialLaw, N. M., Kraus, A. L., Street, R. A., Fulton, B. J., Hillenbrand, L. A., Shporer, A., Lister, T. A., Baranec, C. J., Bloom, J. S., Bui, K., et al. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/757/2/133 · Cited by 54
“We used the Lucky Imaging plus adaptive optics pipeline described in Law et al. (2009b) to perform the image alignment, along with frame selection at the 10% level to boost the imaging resolution.”
MethodSelf-citationThe late-time light curve of the Type Ia supernova SN 2011fe
Dimitriadis, G., Sullivan, M., Kerzendorf, W., Ruiter, A. J., Seitenzahl, I. R., Taubenberger, S., Doran, G. B., Gal‐Yam, A., Laher, R. R., Maguire, K., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx683 · Cited by 54
“The PTF (Law et al. 2009; Rau et al. 2009) was a rolling, wide-field transient survey, operating from 2009 to 2012, using the CFH12k camera (Rahmer et al. 2008) mounted on the Samuel Oschin 48-inch telescope at the Palomar Observatory (P48).”
MethodSelf-citationSinger, L. P., Kasliwal, M. M., Cenko, S. B., Perley, D. A., Anderson, G. E., Anupama, G. C., Arcavi, I., Bhalerao, V., Bue, B., Cao, Y., et al. (2015) · The Astrophysical Journal · doi:10.1088/0004-637x/806/1/52 · Cited by 54
“Deep synoptic optical surveys including the Palomar Transient Factory (PTF; Rau et al. 2009; Law et al. 2009) and Pan-STARRS (Kaiser et al. 2010) have revealed a wealth of new transient and variable phenomena across a wide range of characteristic luminosities and time scales (Kasliwal 2011).”
BackgroundSelf-citationExtending the supernova Hubble diagram toz~ 1.5 with theEuclidspace mission
Astier, P., Balland, C., Brescia, M., Cappellaro, E., Carlberg, R. G., Cavuoti, S., Valle, M. D., Gangler, É., Goobar, A., Guy, J., et al. (2014) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201423551 · Cited by 54
“We have not incorporated such a sample in our forecast, but one could argue that existing facilities (e.g. PTF Law et al. 2009; Skymapper Keller et al. 2007) could deliver it soon.”
BackgroundSelf-citationPoint-source and diffuse high-energy neutrino emission from Type IIn supernovae
Πετροπούλου, Μ., Coenders, S., Vasilopoulos, G., Kamble, A., & Sironi, L. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1251 · Cited by 54
“Interestingly, a SN IIn was recently discovered in a search with the Palomar Transient Factory (PTF) (Law et al. 2009) following an IceCube neutrino doublet trigger alert.”
BackgroundMethodBurdge, K. B., Fuller, J., Phinney, E. S., van Roestel, J., Claret, A., Cukanovaite, E., Fusillo, N. P. G., Coughlin, M. W., Kaplan, D. L., Kupfer, T., et al. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab53e5 · Cited by 54
“After imposing the photometric color cut, we cross-matched the resulting sample with the archival Palomar Transient Factory (PTF; Law et al. 2009) photometric database.”
MethodSelf-citationSecond Data Release of the All-sky NOIRLab Source Catalog
Nidever, D. L., Dey, A., Fasbender, K. M., Juneau, S., Meisner, A., Wishart, J., Scott, A., Matt, K., Nikutta, R., & Pucha, R. (2021) · The Astronomical Journal · doi:10.3847/1538-3881/abd6e1 · Cited by 54
“The NSC expands the search carried out by projects such as the Palomar Transient Factory (Law et al. 2009), ZTF, CSS, and PS1, and the ones that will soon be possible with the Rubin Observatory’s LSST.”
Method
Metadata
- Authors
- Law, N. M., Kulkarni, S. R., Dekany, R. G., Ofek, E. O., Quimby, R. M., Nugent, P. E., Surace, J., Grillmair, C. C., Bloom, J. S., Kasliwal, M. M., Bildsten, L., Brown, T., Cenko, S. B., Ciardi, D., Croner, E., Djorgovski, S. G., van Eyken, J., Filippenko, A. V., Fox, D. B., Gal-Yam, A., Hale, D., Hamam, N., Helou, G., Henning, J., Howell, D. A., Jacobsen, J., Laher, R., Mattingly, S., McKenna, D., Pickles, A., Poznanski, D., Rahmer, G., Rau, A., Rosing, W., Shara, M., Smith, R., Starr, D., Sullivan, M., Velur, V., Walters, R., & Zolkower, J.
- Affiliations
- California Institute of Technology (US)
- Lawrence Berkeley National Laboratory (US)
- University of California, Berkeley (US)
- University of California, Santa Barbara (US)
- Las Cumbres Observatory Global Telescope Network (US)
- Pennsylvania State University (US)
- American Museum of Natural History (US)
- University of Oxford (GB)
- ORCID
- Law, Nicholas M.
- Kulkarni, Shrinivas R.
- Dekany, Richard G.
- Ofek, Eran O.
- Quimby, Robert M.
- Nugent, Peter E.
- Surace, Jason
- Bloom, Joshua S.
- Kasliwal, Mansi M.
- Bildsten, Lars
- Cenko, S. Bradley
- Ciardi, David
- Djorgovski, S. George
- Filippenko, Alexei V.
- Fox, Derek B.
- Hale, David
- Howell, D. Andrew
- Laher, Russ
- Poznanski, Dovi
- Rahmer, Gustavo
- Rau, Arne
- Shara, Michael
- Smith, Roger
- Sullivan, Mark
- Walters, Richard
- Venue
- Publications of the Astronomical Society of the Pacific
- Publisher
- IOP Publishing
- Published
- 2009-12
- Volume
- 121
- Issue
- 886
- Pages
- 1395-1408
- ISSN
- 0004-6280 (ISSN-L)
- 1538-3873
- OpenAlex
- W2083217178
- Cited by
- 1,141
- References
- 7
- Citations by year
- 2026: 30 · 2025: 44 · 2024: 50 · 2023: 40 · 2022: 54 · 2021: 61 · 2020: 74 · 2019: 99 · 2018: 92 · 2017: 115 · 2016: 114 · 2015: 76 · 2014: 69 · 2013: 64 · 2012: 65
- FWCI
- 26.68
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- Publications of the Astronomical Society of the Pacific (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- Max Planck Institute for Plasma Physics (submittedVersion)
- Max Planck Digital Library (submittedVersion)
- MPG.PuRe (Max Planck Society) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Science Foundation (0540352, 0607485, 0507734)
- U.S. Department of Energy (DE‐FG02‐, FC02-06ER41453, FG02-08ER41563)
- National Aeronautics and Space Administration (NNX08AM04G)
- Alfred P. Sloan Foundation
- California Institute of Technology
- University of Oxford
- Minerva Foundation
- Weizmann Institute of Science
- Israel Science Foundation
- Lawrence Berkeley National Laboratory
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Gamma-ray bursts and supernovae
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Keywords
- Palomar Transient Factory, optical transients, supernova search, transient survey, light curves, transient classification, H-alpha survey, eclipsing binaries, transiting exoplanets, Orion
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