AstroNote 2022-107

Primary tabs

DRAFT
2022-05-12 21:27:49
Type: Announcement-Campaign/Survey
The DESIRT DECam Time Domain Program
Authors: Antonella Palmese (UC Berkeley), Lifan Wang (TAMU), Xingzhuo Chen (TAMU), Lei Hu (Purple Mountain Observatory), Jiawen Yang (TAMU), Segev BenZvi (U of Rochester), Jeff Cooke (Swinburne U), Robert Knop (LBNL), Anand Raichoor (LBNL), Edward F. Schlafly (LLNL), Lauren Aldoroty (TAMU), Dietrich Baade (ESO), Peter Brown (TAMU), Ryan Chornock (UC Berkeley), Tamara Davis (UQ), Kyle Dawson (U of Utah), Melissa Graham (U. of Washington), Xiaosheng Huang (UCSF), Jian Jiang (IMPU), Alex Kim (LBNL), Anton Koekemoer (STScI), Raffaella Margutti (UC Berkeley), Jeremy Mould (Swinburne University), Peter Nugent (LBNL), Ferdinando Patat (ESO), David Schlegel (LBNL), Syed Uddin (TAMU), Xiaofeng Wang (Tsinghua)
Abstract:
We announce the DECam Survey of Intermediate Redshift Transients (DESIRT), a time domain program using the Dark Energy Camera (DECam). We repeatedly observe in g,r,z bands regions of the sky that the Dark Energy Spectroscopic Instrument (DESI) is going to cover around the same time. We reach depths greater than mag 23 in g and r, and 22.6 or better in z band (5 sigma). This program was run in 2021 between March and June, while this semester observations are running between April and the end of July 2022. We will be reporting transient discoveries to the community.

The DECam Survey of Intermediate Redshift Transients (DESIRT; PIs: Palmese & Wang) is a time domain program using the Dark Energy Camera (DECam) on the Blanco 4m Telescope at the Cerro Tololo Interamerican Observatory as part of the DECam Alliance for Transients (DECAT). We are sharing full nights with the other DECAT programs, including the Deep Drilling Fields Program (see Graham et al. 2021), and DESIRT takes data every ~4 nights between April and the end of July 2022, for a total of 90 hours.

 

The DESIRT program is designed to observe regions of the sky that the Dark Energy Spectroscopic Instrument (DESI; DESI Collaboration 2016, arXiv:1611.00036) is going to cover around the same time. We have therefore chosen to start the semester with observations of three equatorial regions: one centered on GAMA 15, a second around RA, dec = 224d, +7d , and a third at RA, dec = 193d, +6d (all J2000), for a total of 24 DECam pointings. Using the nominal DECAT cadence during dark and grey time, we cover these regions in grz bands with exposure times of 50, 70, and 110 seconds respectively, plus a second pass in g band with the same exposure time as the first pass. In bright time, we switch to riz exposures. These exposures reach an r-band depth of ~23.2-23.8 (5 sigma).

 

We promptly process our data on GPUs using the pipeline of Hu, Wang & Chen (2021), and announce new transient discoveries to the TNS using a bot. Public alerts are also being sent to a Kafka broker (public.alerts.ztf.uw.edu:9092 with topic decat_<yyyymmdd>_2022A-388025) following https://decat-webap.lbl.gov/ (Knop et al.)

 

We welcome all members of the astronomical community to use these data for their own analyses and follow-up observations. Our DECam program has no proprietary period, and we also encourage the community to download our images from the NSF NOIRLab archive under Proposal ID 2022A-388025. Note that no DESI data will be released at this time, but we plan to release interesting DESI observations of transients along with publications at a later time.