Difference: RCF (38 vs. 39)

Revision 392020-12-08 - MelissaLynngraham

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META TOPICPARENT	name="TransientWorkingGroup"

We are performing a flux limited transient survey based on the MSIP all sky survey. The standard in this field is set by ASAS-SN which is by our estimate complete to less than 17 mag. The experimental goal of the ZTF RCF project is to classify transients (which are mostly SNe) to a peak magnitude, m_p of about 18.5 mag. In practice, this means classifying transients which are a few tenths mag fainter (~18.75). Flux limited surveys serve many purposes, and are essential for e.g., computing rates. We have a specific novel goal: use SN of type Ia to evaluate the red-shift completeness factor (RCF) of catalog(s) of nearby (<200 Mpc). [ http://adsabs.harvard.edu/abs/2017arXiv171004223K

, https://www.dropbox.com/s/nhd3qxnhdxwqjyd/WP_SEDM.pdf?dl=0

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Fremling, Ulf Christoffer (Christoffer) <fremling@caltech.edu>; Adam Miller <amiller@northwestern.edu>; Alison Dugas <adugas@hawaii.edu>; Jesper Sollerman <jesper@astro.su.se>; Daniel Perley <D.A.Perley@ljmu.ac.uk>; Sharma, Yashvi <yssharma@astro.caltech.edu>; Taggart, Kirsty <K.L.Taggart@2016.ljmu.ac.uk>; Suhail Dhawan <suhail.dhawan@fysik.su.se>; Rahul Biswas <rbiswas4@gmail.com>; Melissa Graham <melissalynngraham@gmail.com>; Jakob Nordin <jnordin@physik.hu-berlin.de>; Ariel Goobar <ariel@fysik.su.se>; Neill, James D. (Don) <neill@srl.caltech.edu>; Rachel Bruch <rachel.bruch@weizmann.ac.il>; Rauch, Ludwig <ludwig.rauch@desy.de>; Steve Schulze <steve.schulze@weizmann.ac.il>; Ido Irani <ido.irani@weizmann.ac.il>; Kulkarni, Shrinivas R. (Shri) <srk@astro.caltech.edu>; Jannis Necker <necker@physik.hu-berlin.de>; Kishore Patra <kcpatra@berkeley.edu>; Samantha Goldwasser <samantha.goldwasser@weizmann.ac.il>; Shaunak Modak <shaunakmodak@berkeley.edu>; Andrew Hoffman <andrewmh@berkeley.edu>; Erez Zimmerman <erez.zimmerman@weizmann.ac.il>; yafshar0673@sdsu.edu <yafshar0673@sdsu.edu>; Hall, Xander J. <xhall@caltech.edu>

Redshift Completeness Factor - Papers in Progress

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SN Siblings

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Melissa L. Graham

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Brief Description: Individual analyses of the few SN siblings in the RCF data set thus far and a brief sample (rates) analysis

Status: in preparation at https://www.overleaf.com/read/fdwjbnmtmsxp

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Cosmology with Type II-P distances: Expanding photosphere method

Leads: Jakob Nordin, Peter Nugent, Sarafina Nance, Suhail Dhawan, Ariel Goobar

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