2023ApJS..264....7C


Query : 2023ApJS..264....7C

2023ApJS..264....7C - Astrophys. J., Suppl. Ser., 264, 7 (2023/January-0)

CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope.

CCAT-PRIME COLLABORATION, ARAVENA M., AUSTERMANN J.E., BASU K., BATTAGLIA N., BERINGUE B., BERTOLDI F., BIGIEL F., BOND J.R., BREYSSE P.C., BROUGHTON C., BUSTOS R., CHAPMAN S.C., CHARMETANT M., CHOI S.K., CHUNG D.T., CLARK S.E., COTHARD N.F., CRITES A.T., DEV A., DOUGLAS K., DUELL C.J., DUNNER R., EBINA H., ERLER J., FICH M., FISSEL L.M., FOREMAN S., FREUNDT R.G., GALLARDO P.A., GAO J., GARCIA P., GIOVANELLI R., GOLEC J.E., GROPPI C.E., HAYNES M.P., HENKE D., HENSLEY B., HERTER T., HIGGINS R., HLOZEK R., HUBER A., HUBER Z., HUBMAYR J., JACKSON R., JOHNSTONE D., KAROUMPIS C., KEATING L.C., KOMATSU E., LI Y., MAGNELLI B., MATTHEWS B.C., MAUSKOPF P.D., McMAHON J.J., MEERBURG P.D., MEYERS J., MURALIDHARA V., MURRAY N.W., NIEMACK M.D., NIKOLA T., OKADA Y., PUDDU R., RIECHERS D.A., ROSOLOWSKY E., ROSSI K., ROTERMUND K., ROY A., SADAVOY S.I., SCHAAF R., SCHILKE P., SCOTT D., SIMON R., SINCLAIR A.K., SIVAKOFF G.R., STACEY G.J., STUTZ A.M., STUTZKI J., TAHANI M., THANJAVUR K., TIMMERMANN R.A., ULLOM J.N., VAN ENGELEN A., VAVAGIAKIS E.M., VISSERS M.R., WHEELER J.D., WHITE S.D.M., ZHU Y. and ZOU B.

Abstract (from CDS):

We present a detailed overview of the science goals and predictions for the Prime-Cam direct-detection camera-spectrometer being constructed by the CCAT-prime collaboration for dedicated use on the Fred Young Submillimeter Telescope (FYST). The FYST is a wide-field, 6 m aperture submillimeter telescope being built (first light in late 2023) by an international consortium of institutions led by Cornell University and sited at more than 5600 m on Cerro Chajnantor in northern Chile. Prime-Cam is one of two instruments planned for FYST and will provide unprecedented spectroscopic and broadband measurement capabilities to address important astrophysical questions ranging from Big Bang cosmology through reionization and the formation of the first galaxies to star formation within our own Milky Way. Prime-Cam on the FYST will have a mapping speed that is over 10 times greater than existing and near-term facilities for high-redshift science and broadband polarimetric imaging at frequencies above 300 GHz. We describe details of the science program enabled by this system and our preliminary survey strategies.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Wide-field telescopes - Astronomical instrumentation - Galaxy evolution - Reionization - Protogalaxies - Time domain astronomy - Observational cosmology - Interstellar dust - Star formation - Sunyaev-Zeldovich effect - Galaxy clusters - Recombination (cosmology)

Simbad objects: 46

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Number of rows : 46
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 NAME Chandra Deep Field-South reg 03 32 28.0 -27 48 30           ~ 2282 1
2 NAME Extended Chandra Deep Field South reg 03 32 30.0 -27 48 20           ~ 862 0
3 NAME Hubble Ultra Deep Field reg 03 32 39.0 -27 47 29           ~ 1900 0
4 NAME Perseus Cloud SFR 03 35.0 +31 13           ~ 1553 0
5 SN 2003bg SN* 04 10 59.43 -31 24 50.4     15.0     SNIc 170 1
6 PMN J0509+0541 BLL 05 09 25.9644373872 +05 41 35.333820420 15.32 14.95 14.78 15.12   ~ 589 2
7 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
8 JW 566 Y*O 05 35 17.990 -05 16 13.63   14.9 18.7   15.757 K7+M1.5 44 0
9 NAME Ori A MoC 05 38 -07.1           ~ 3187 0
10 NAME Ori B MoC 05 41 43.0 -01 54 44           ~ 1498 0
11 NAME Orion Molecular Cloud MoC 05 56 -01.8           ~ 1227 1
12 NAME SEP reg 06 00 00.000 -66 33 38.55           ~ 198 0
13 NAME Vela C Cld 08 57 -43.2           ~ 193 0
14 NAME Pyxis Cluster GlC 09 07 57.80 -37 13 17.0           ~ 123 0
15 SN 2008D SN* 09 09 30.625 +33 08 20.16     17.5     SNIb 458 1
16 SN 1993J SN* 09 55 24.77476 +69 01 13.7026   10.8 12.0     SNIIb 1507 1
17 NAME COSMOS Field reg 10 00 28.60 +02 12 21.0           ~ 3639 0
18 SN 2009bb SN* 10 31 33.92 -39 57 28.2           SNIc 185 1
19 NAME Carina Molecular Cloud Complex MoC 10 43 10 -59 38.2           ~ 97 0
20 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
21 SN 2003L SN* 11 03 12.33 +11 04 38.3     16.9     SNIc 77 1
22 SN 2007bg SN* 11 49 26.18 +51 49 21.8 20.1 19.8 18.8     SNIc-BL 72 1
23 SN 2020oi SN* 12 22 54.930 +15 49 24.96           SNIc 77 0
24 NAME Musca Cld 12 23 -71.3           ~ 258 0
25 M 87 AGN 12 30 49.42338414 +12 23 28.0436859 10.16 9.59 8.63   7.49 ~ 7815 3
26 NAME Proxima Centauri PM* 14 29 42.9461331854 -62 40 46.164680672 14.21 12.95 11.13 9.45 7.41 M5.5Ve 1483 0
27 Lupus 1 Cld 15 43 02.1 -34 09 06           ~ 320 0
28 SN 2018cow SN* 16 16 00.254 +22 16 05.10           SNIb 305 0
29 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3969 1
30 SWIFT J164449.3+573451 G 16 44 47.81184000 +57 35 00.7113480           ~ 533 0
31 GRB 100418A gB 17 05 26.96 +11 27 41.9           ~ 198 0
32 NAME the Pipe Nebula DNe 17 30 -25.0           ~ 442 1
33 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
34 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 4970 3
35 Fermi bn120326056 gB 18 15 37.06 +69 15 35.4           ~ 188 0
36 MAXI J1820+070 LXB 18 20 21.9423816480 +07 11 07.284859440           ~ 511 0
37 NGC 6618 OpC 18 20 47 -16 10.3           ~ 1700 0
38 NAME Serpens Main Cloud MoC 18 29.2 +00 36           ~ 39 0
39 NAME Serpens Cloud SFR 18 29 49 +01 14.8           ~ 1195 1
40 V* V371 Ser Or* 18 29 51.21240 +01 16 39.4860           ~ 132 1
41 NAME Serpens South molecular cloud MoC 18 30 -02.0           ~ 116 0
42 NAME Aql Region reg 18 31.1 -02 10           ~ 456 0
43 SN 2011df SN* 19 27 33.64 +54 23 11.3           SNIa 18 1
44 V* V404 Cyg HXB 20 24 03.8247037434 +33 52 01.961154861           G9/K0III/V 1370 0
45 AT 2020xnd ev 22 20 02.030 -02 50 25.30           ~ 66 0
46 NAME Gould Belt PoG ~ ~           ~ 956 1

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