K2's Campaign 9 (K2C9) will conduct a ̃3.7 deg<SUP>2</SUP> survey toward the Galactic bulge from 2016 April 22 through July 2 that will leverage the spatial separation between K2 and the Earth to facilitate measurement of the microlens parallax π <SUB>E</SUB> for ≳ 170 microlensing events. These will include several that are planetary in nature as well as many short-timescale microlensing events, which are potentially indicative of free-floating planets (FFPs). These satellite parallax measurements will in turn allow for the direct measurement of the masses of and distances to the lensing systems. In this article we provide an overview of the K2C9 space- and ground-based microlensing survey. Specifically, we detail the demographic questions that can be addressed by this program, including the frequency of FFPs and the Galactic distribution of exoplanets, the observational parameters of K2C9, and the array of resources dedicated to concurrent observations. Finally, we outline the avenues through which the larger community can become involved, and generally encourage participation in K2C9, which constitutes an important pathfinding mission and community exercise in anticipation of WFIRST.

Henderson, C.b., Poleski, R., Penny, M., Street, R.a., Bennett, D.p., Hogg, D.w., et al. (2016). Campaign 9 of the K2 mission: Observational parameters, scientific drivers, and community involvement for a simultaneous space-and ground-based microlensing survey. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 128(970), 124401 [10.1088/1538-3873/128/970/124401].

Campaign 9 of the K2 mission: Observational parameters, scientific drivers, and community involvement for a simultaneous space-and ground-based microlensing survey

Mancini L.;
2016-01-01

Abstract

K2's Campaign 9 (K2C9) will conduct a ̃3.7 deg2 survey toward the Galactic bulge from 2016 April 22 through July 2 that will leverage the spatial separation between K2 and the Earth to facilitate measurement of the microlens parallax π E for ≳ 170 microlensing events. These will include several that are planetary in nature as well as many short-timescale microlensing events, which are potentially indicative of free-floating planets (FFPs). These satellite parallax measurements will in turn allow for the direct measurement of the masses of and distances to the lensing systems. In this article we provide an overview of the K2C9 space- and ground-based microlensing survey. Specifically, we detail the demographic questions that can be addressed by this program, including the frequency of FFPs and the Galactic distribution of exoplanets, the observational parameters of K2C9, and the array of resources dedicated to concurrent observations. Finally, we outline the avenues through which the larger community can become involved, and generally encourage participation in K2C9, which constitutes an important pathfinding mission and community exercise in anticipation of WFIRST.
2016
Pubblicato
Rilevanza internazionale
Articolo
Esperti anonimi
Settore FIS/05 - ASTRONOMIA E ASTROFISICA
English
Henderson, C.b., Poleski, R., Penny, M., Street, R.a., Bennett, D.p., Hogg, D.w., et al. (2016). Campaign 9 of the K2 mission: Observational parameters, scientific drivers, and community involvement for a simultaneous space-and ground-based microlensing survey. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 128(970), 124401 [10.1088/1538-3873/128/970/124401].
Henderson, Cb; Poleski, R; Penny, M; Street, Ra; Bennett, Dp; Hogg, Dw; Scott Gaudi, B; Zhu, W; Barclay, T; Barentsen, G; Howell, Sb; Mullally, F; Udalski, A; Szymanski, Mk; Skowron, J; Mroz, P; Kozlowski, S; Wyrzykowski, L; Pietrukowicz, P; Soszynski, I; Ulaczyk, K; Pawlak, M; Sumi, T; Abe, F; Asakura, Y; Barry, Rk; Bhattacharya, A; Bond, Ia; Donachie, M; Freeman, M; Fukui, A; Hirao, Y; Itow, Y; Koshimoto, N; Li, Mca; Ling, Ch; Masuda, K; Matsubara, Y; Muraki, Y; Nagakane, M; Ohnishi, K; Oyokawa, H; Rattenbury, N; Saito, T; Sharan, A; Sullivan, Dj; Tristram, Pj; Yonehara, A; Bachelet, E; Bramich, Dm; Cassan, A; Dominik, M; Figuera Jaimes, R; Horne, K; Hundertmark, M; Mao, S; Ranc, C; Schmidt, R; Snodgrass, C; Steele, Ia; Tsapras, Y; Wambsganss, J; Bozza, V; Burgdorf, Mj; Jorgensen, Ug; Calchi Novati, S; Ciceri, S; D'Ago, G; Evans, Df; Hessman, Fv; Hinse, Tc; Husser, T-; Mancini, L; Popovas, A; Rabus, M; Rahvar, S; Scarpetta, G; Skottfelt, J; Southworth, J; Unda-Sanzana, E; Bryson, St; Caldwell, Da; Haas, Mr; Larson, K; Mccalmont, K; Packard, M; Peterson, C; Putnam, D; Reedy, L; Ross, S; Van Cleve, Je; Akeson, R; Batista, V; Beaulieu, J-; Beichman, Ca; Bryden, G; Ciardi, D; Cole, A; Coutures, C; Foreman-Mackey, D; Fouque, P; Friedmann, M; Gelino, C; Kaspi, S; Kerins, E; Korhonen, H; Lang, D; Lee, C-; Lineweaver, Ch; Maoz, D; Marquette, J-; Mogavero, F; Morales, Jc; Nataf, D; Pogge, Rw; Santerne, A; Shvartzvald, Y; Suzuki, D; Tamura, M; Tisserand, P; Wang, D
Articolo su rivista
File in questo prodotto:
File Dimensione Formato  
137-2016-PASP-128-124401.pdf

solo utenti autorizzati

Licenza: Copyright dell'editore
Dimensione 3.97 MB
Formato Adobe PDF
3.97 MB Adobe PDF   Visualizza/Apri   Richiedi una copia

I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.

Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/204859
Citazioni
  • ???jsp.display-item.citation.pmc??? ND
  • Scopus 51
  • ???jsp.display-item.citation.isi??? 48
social impact