2024MNRAS.529.3020H


Query : 2024MNRAS.529.3020H

2024MNRAS.529.3020H - Mon. Not. R. Astron. Soc., 529, 3020-3034 (2024/April-2)

The Atacama cosmology telescope: flux upper limits from a targeted search for extragalactic transients.

HERVIAS-CAIMAPO C., NAESS S., HINCKS A.D., CALABRESE E., DEVLIN M.J., DUNKLEY J., DUNNER R., GALLARDO P.A., HILTON M., HO A.Y.Q., HUFFENBERGER K.M., MA X., MADHAVACHERIL M.S., NIEMACK M.D., ORLOWSKI-SCHERER J., PAGE L.A., PARTRIDGE B., PUDDU R., SALATINO M., SIFON C., STAGGS S.T., VARGAS C., VAVAGIAKIS E.M. and WOLLACK E.J.

Abstract (from CDS):

We have performed targeted searches of known extragalactic transient events at millimetre wavelengths using nine seasons (2013-2021) of 98, 150, and 229 GHz Atacama Cosmology Telescope (ACT) observations that mapped ∼40 per cent of the sky for most of the data volume. Our data cover 88 gamma-ray bursts (GRBs), 12 tidal disruption events (TDEs), and 203 other transients, including supernovae (SNe). We stack our ACT observations to increase the signal-to-noise ratio of the maps. In all cases but one, we do not detect these transients in the ACT data. The single candidate detection (event AT2019ppm), seen at ∼5σ significance in our data, appears to be due to active galactic nuclei activity in the host galaxy coincident with a transient alert. For each source in our search we provide flux upper limits. For example, the medians for the 95 per cent confidence upper limits at 98 GHz are 15, 18, and 16 mJy for GRBs, SNe, and TDEs, respectively, in the first month after discovery. The projected sensitivity of future wide-area cosmic microwave background surveys should be sufficient to detect many of these events using the methods described in this paper.

Abstract Copyright: © 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.

Journal keyword(s): methods: data analysis - cosmic background radiation - transients: gamma-ray bursts - transients: supernovae - transients: tidal disruption events

Status at CDS : Large table(s) will be appraised for possible ingestion in VizieR. // All or part of tables of objects could be ingested in SIMBAD with priority 2.

Simbad objects: 24

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Number of rows : 24
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SRGE J013204.6+122236 X 01 32 04.482 +12 22 35.62           ~ 4 0
2 2MASS J01580475-0052221 Sy1 01 58 04.7506373016 -00 52 21.927742716   18.84 18.34     SNII 114 1
3 AT 2019qiz ev 04 46 37.880 -10 13 34.92           ~ 143 0
4 ASASSN -20il SN? 05 03 11.470 -22 48 49.73           ~ 4 0
5 M 42 HII 05 35 16.8 -05 23 15           ~ 4411 0
6 NGC 2110 Sy2 05 52 11.3768668776 -07 27 22.507465392   14.77 13.51 11.86   ~ 712 1
7 AT 2019ppm ev 05 52 11.400 -07 27 23.04           ~ 1 0
8 2MASS J10065085+0141342 G 10 06 50.8773292152 +01 41 34.006164648   18.082   17.032   SNII 127 0
9 SDSS J112849.64+154022.3 G 11 28 49.6469654133 +15 40 22.339118003           ~ 18 0
10 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1
11 SN 2020oi SN* 12 22 54.930 +15 49 24.96           SNIc 77 0
12 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
13 ZW VIII 211 rG 12 48 15.2253025968 +17 46 26.475426228   16.5       ~ 360 0
14 IGR J12580+0134 gam 12 58 05.1 +01 34 26           ~ 50 0
15 SN 2011dh SN* 13 30 05.10555 +47 10 10.9227           SNIIb 445 1
16 iPTF 13bvn SN* 15 00 00.152 +01 52 53.17           SNIb 211 0
17 AT 2019bhf ev 15 09 15.975 +16 14 22.52           ~ 18 0
18 SN 2018cow SN* 16 16 00.254 +22 16 05.10           SNIb 305 0
19 SWIFT J164449.3+573451 G 16 44 47.81184000 +57 35 00.7113480           ~ 533 0
20 SRGE J171423.6+085236 X 17 14 23.614 +08 52 36.90           ~ 4 0
21 2MASX J20570298+1412165 G 20 57 02.9650698480 +14 12 16.295014080           ~ 162 0
22 ASASSN -20mi SN? 21 15 40.241 -49 04 34.62           ~ 3 0
23 AT 2018fyk ev 22 50 16.10 -44 51 53.5           ~ 114 0
24 AT 2019lwu ev 23 11 12.305 -01 00 10.71           ~ 17 0

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