Cited by 1,141Gamma-ray bursts and supernovaeAstronomy and Astrophysical ResearchStellar, planetary, and galactic studies

The Palomar Transient Factory: System Overview, Performance, and First Results

Open access
Law, Nicholas M., Kulkarni, Shrinivas R., Dekany, Richard G., Ofek, Eran O., Quimby, Robert M., Nugent, Peter E., Surace, Jason, Grillmair, Carl C. +33 more·2009·Publications of the Astronomical Society of the Pacific

Abstract

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.

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Integrity signals

Registry

Crossref · 10.1086/648598

Cites

7 of 7 references verified0 citation errors · 0 not checkable

Statistics

Claims the paper makes

The claims and statistics of this paper haven’t been checked yet.

Run the check — free, no account needed. It reads the open-access text and checks the sources it cites.

A few free checks a day · papers already verified open instantly · results are public

Claims other papers make about this one

Each is checked against this paper’s own text: does it say what the citing paper says it does?

  • Recent surveys have shown the power of measuring variability of celestial sources for studying gravitational lensing, supernovae, gamma-ray bursts, gravitational wave counterparts, active galactic nuclei, variable stars, exoplanets, and other forefront astrophysics.

    “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

Self-check

Percentages, sums and reported differences re-computed from the paper’s own numbers.

The self-check needs the paper’s full text.

Cites

Flagged first, then by citations

Research works printed but not linked: 6

  1. M. S. acknowledges sup- port from the Royal Society and the University of Oxford Fell Fund. REFERENCES
  2. Aldering, G., Adam, G., Antilogus, P., Astier, P., Bacon, R., Bongard, S., Bonnaud, C., Copin, Y., et al. 2002, Proc. SPIE, 4836, 61
  3. Ashe, M. C., Bonati, M., & Heathcote, S. 2002, Proc. SPIE, 4848, 508
  4. Cuillandre, J.-C., Luppino, G. A., Starr, B. M., & Isani, S. 2000, Proc. SPIE, 4008, 1010
  5. Mahabal, A., Djorgovski, S. G., Williams, R., Drake, A., Donalek, C., Graham, M., Moghaddam, B., Turmon, M., et al. 2008b, in AIP Conf. Ser. 1082, 287-293
  6. Rahmer, G., Smith, R., Velur, V., Hale, D., Law, N., Bui, K., Petrie, H., & Dekany, R. 2008, Proc. SPIE, 7014

Cited by

Sorted by citations

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)
Venue
Publications of the Astronomical Society of the Pacific
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
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

About these checks

Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.

Statistics and arithmetic are recomputed, not judged.

Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.

What counts as a claim ›How we measure confidence ›How we check this ›

Are you an author, or do you see a problem with this page? Request a review