High-z AGN as seen by Rubin-LSST (Rubin-LSST-16)
LSST-highzAGN
Progetto
RSN1
Attività: Nuova; Data inizio: 2022; Data fine: 2030
angela.bongiorno angela.bongiorno@inaf.it
INAF ha aderito al progetto Rubin-LSST grazie ad un numero elevato di contributi in natura da parte dei ricercatori del nostro ente. Il Team INAF-LSST-highzAGN qui descritto contribuisce a questo sforzo, ottenendo in cambio un numero significativo di diritti per accedere alla survey LSST. Questa scheda descrive il piano di lavoro per i contributi in natura approvati da LSST e per lo sfruttamento del voluminoso e complesso database di LSST. In particolare, il nostro contributo prevede la creazione di immagini multibanda simulate che includano galassie ed AGN e l'estrazione dei cataloghi fotometrici dalle immagini simulate. L'obiettivo scientifico perseguito e' la selezione di un campione esteso di AGN ad alto redshift, da effettuarsi sia con metodi tradizionali che con strumenti innovativi.
INAF recently joined the Rubin Observatory’s Legacy Survey of Space and Time (Rubin-LSST) project thanks to a number of in-kind contributions provided by INAF researchers. The INAF-LSST-highzAGN team presented here will provide one of them gaining a number of Data Rights to access the dataset. This “scheda” includes the planned work for the approved in-kind contribution and for the full exploitation of the voluminous and complex LSST dataset. In particular, for the in-kind contribution we will create simulated multi-band images, including both galaxies and AGN mock catalogs, and realistic catalog-level simulated data extracted from them. Our scientific interest will then be to collect and study the largest sample of high-z AGN to date by using both standard and innovative methods.
Galassie, AGN e loro evoluzione
Struttura | Nfte | N0 | TI 2023 | TI 2024 | TI 2025 | TD 2023 | TD 2024 | TD 2025 | Nex | Extra |
---|---|---|---|---|---|---|---|---|---|---|
O.A. ROMA | 1 | 0 | 0.30 | 0.50 | 0.50 | 0 | 0 | 0 | 0 | 0.00 |
O.A. PADOVA | 1 | 0 | 0.20 | 0.20 | 0.20 | 0 | 0 | 0 | 0 | 0.00 |
OAS BOLOGNA | 1 | 0 | 0.20 | 0.20 | 0.10 | 0 | 0 | 0 | 0 | 0.00 |
O.A. CAPODIMONTE | 1 | 0 | 0.10 | 0.10 | 0.10 | 0 | 0 | 0 | 0 | 0.00 |
O.A. BRERA | 2 | 0 | 0.20 | 0.20 | 0.20 | 0 | 0 | 0 | 0 | 0.00 |
IASF MILANO | 1 | 0 | 0.10 | 0.10 | 0.10 | 0 | 0 | 0 | 0 | 0.00 |
O.A. TRIESTE | 0 | 0 | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0 | 0.00 |
Totali | 7 | 0 | 1.10 | 1.30 | 1.20 | 0.00 | 0.00 | 0.00 | 0 | 0.00 |
# | Struttura | TI 2023 | TI 2024 | TI 2025 | TD 2023 | TD 2024 | TD 2025 | Extra |
---|---|---|---|---|---|---|---|---|
1 | Scuola Normale Superiore di Pisa | 0.10 | 0.10 | 0.00 | 0 | 0 | 0 | 0.00 |
2 | Università di Napoli | 0.00 | 0.00 | 0.00 | 0 | 0 | 0 | 0.00 |
3 | Università Roma3 | 0 | 0 | 0 | 0.20 | 0.20 | 0.20 | 0.00 |
4 | Università Roma Tre | 0.10 | 0.10 | 0.10 | 0 | 0 | 0 | 0.00 |
5 | Univ. degli Studi di Roma Tre | 0 | 0 | 0 | 0.10 | 0.10 | 0.10 | 0.00 |
Totali | 0.20 | 0.20 | 0.10 | 0.30 | 0.30 | 0.30 | 0.00 |
Certi 2023 | Certi 2024 | Certi 2025 | Presunti 2023 | Presunti 2024 | Presunti 2025 |
---|---|---|---|---|---|
18.0 | 0.0 | 0 | 35000.0 | 0.0 | 0 |
<p><span id="docs-internal-guid-c15f6052-7fff-98b6-7ad4-be8e762a489a"></span></p><p dir="ltr" style="line-height:1.38;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:12pt;font-family:Roboto,sans-serif;color:#212529;background-color:#ffffff;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Galassie, AGN e loro evoluzione</span></p>
<p dir="ltr" style="line-height:1.38;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:12pt;font-family:Roboto,sans-serif;color:#212529;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Angela Bongiorno and Andrea Grazian are the PI and Co-PI of the INAF in-kind contribution </span><span style="font-size:12pt;font-family:Roboto,sans-serif;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">“</span><span style="font-size:11pt;font-family:Verdana;color:#000000;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">Simulations of high-z AGNs and galaxies in the LSST survey”, recently approved by the Rubin-LSST Corporation. </span></p><p><span id="docs-internal-guid-13253e85-7fff-044e-a6bd-47d75ebefa17"><br><span style="font-size: 12pt; font-family: Roboto, sans-serif; background-color: transparent; font-variant-numeric: normal; font-variant-east-asian: normal; vertical-align: baseline; white-space: pre-wrap;">The INAF Rubin-LSST AGN team includes a large number of INAF researchers (total FTE TI = 3.2) and has a key role in the Rubin-LSST AGN Science Collaboration contributing in one of the main objectives declared in the </span><span style="font-size: 12pt; font-family: Roboto, sans-serif; background-color: transparent; font-weight: 700; font-variant-numeric: normal; font-variant-east-asian: normal; vertical-align: baseline; white-space: pre-wrap;">AGN Science Collaboration Roadmap</span><span style="font-size: 12pt; font-family: Roboto, sans-serif; background-color: transparent; font-variant-numeric: normal; font-variant-east-asian: normal; vertical-align: baseline; white-space: pre-wrap;"> (Richards, G; Brandt, N; Bauer, F. et al., in prep) i.e. “identify efficient and complete ways to pinpoint the location of actively accreting supermassive black holes (SMBHs)”. </span></span><br></p>
<p dir="ltr" style="line-height:1.38;margin-left: -1pt;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:12pt;font-family:Roboto,sans-serif;color:#212529;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">HPC servers to host data reduction, analysis, and machine learning runs of the</span></p><p dir="ltr" style="line-height:1.38;margin-left: -1pt;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:12pt;font-family:Roboto,sans-serif;color:#212529;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">INAF-LSST-highzAGN Team will be available in the LSST corporation institution. However, local mini servers would be important for developing the software tools for the in-kind contribution and for the scientific exploitation of the LSST catalogs.</span></p><p dir="ltr" style="line-height:1.38;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span id="docs-internal-guid-464c981e-7fff-0924-449e-2a94301879dd"><br></span></p><p dir="ltr" style="line-height:1.38;margin-left: -1pt;text-align: justify;margin-top:0pt;margin-bottom:0pt;"><span style="font-size:12pt;font-family:Roboto,sans-serif;color:#212529;background-color:transparent;font-weight:400;font-style:normal;font-variant:normal;text-decoration:none;vertical-align:baseline;white-space:pre;white-space:pre-wrap;">The INAF-LSST-highzAGN Team has access to a wide variety of instrumentation mounted on 4-10m class telescopes (TNG, NTT, VLT, LBT, Magellan) with the aim of executing a rapid follow-up spectroscopy of the best AGN candidates selected on real LSST catalogs.</span></p><p><span id="docs-internal-guid-b6f8edb2-7fff-dbc7-bbd1-c066fa629c84"><br></span></p>
# | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2023/2024/2025) | FTE Presunte (2023/2024/2025) | Extra | ||
---|---|---|---|---|---|---|---|---|---|---|
1 | angela.bongiorno | angela.bongiorno@inaf.it | O.A. ROMA | Y | RICERCATORE | Coordinator and PI inkind contribution | X X X | X X X | X | |
2 | andrea.grazian | andrea.grazian@inaf.it | O.A. PADOVA | Y | RICERCATORE | Coordinator | X X X | X X X | X | |
3 | marco.mignoli | marco.mignoli@inaf.it | OAS BOLOGNA | Y | RICERCATORE | AGN mock catalog | X X X | X X X | X | |
4 | viola.allevato | viola.allevato@inaf.it | O.A. CAPODIMONTE | Y | RICERCATORE | AGN mock catalog | X X X | X X X | X | |
5 | emiliano.merlin | emiliano.merlin@inaf.it | O.A. ROMA | Y | RICERCATORE | image creation and photometry | X X X | X X X | X | |
6 | roberto.gilli | roberto.gilli@inaf.it | OAS BOLOGNA | Y | PRIMO RICERCATORE | science team member | X X X | X X X | X | |
7 | roberto.decarli | roberto.decarli@inaf.it | OAS BOLOGNA | Y | RICERCATORE | science team member | X X X | X X X | X | |
8 | alberto.moretti | alberto.moretti@inaf.it | O.A. BRERA | Y | RICERCATORE | science team member | X X X | X X X | X | |
9 | giustina.vietri | giustina.vietri@inaf.it | IASF MILANO | Y | RICERCATORE | AGN mock catalog | X X X | X X X | X | |
10 | valentina.dodorico | valentina.dodorico@inaf.it | O.A. TRIESTE | Y | RICERCATORE | high-z AGN selection | X X X | X X X | X | |
11 | alessandro.caccianiga | alessandro.caccianiga@inaf.it | O.A. BRERA | Y | RICERCATORE | team member | X X X | X X X | X |
# | Nome | Struttura | TI | Qualifica | Ruolo nel Progetto | FTE Impegnate (2023/2024/2025) | FTE Presunte (2023/2024/2025) | Extra | |
---|---|---|---|---|---|---|---|---|---|
1 | simona.gallerani | simona.gallerani@sns.it | Scuola Normale Superiore di Pisa | Y | Professore associato | high-z AGN model | [0.1, 0.1, 0] | [0.1, 0.1, 0.0] | 0.0 |
2 | maurizio.paolillo | maurizio.paolillo@unina.it | Università di Napoli | Y | Professore Ordinario | AGN variability | [0, 0, 0] | [0.1, 0.1, 0.0] | 0.0 |
3 | ivano.saccheo | ivano.saccheo@uniroma3.it | Università Roma3 | N | PhD Student | multi-lambda prop of AGN | [0.2, 0.2, 0.2] | [0.2, 0.2, 0.2] | 0.0 |
4 | fabio.lafranca | fabio.lafranca@uniroma3.it | Università Roma Tre | Y | Prof. Ordinario | multi-lambda prop of AGN | [0.1, 0.1, 0.1] | [0.1, 0.1, 0.1] | 0.0 |
5 | federica.ricci | federica.ricci@uniroma3.it | Univ. degli Studi di Roma Tre | N | tempo determinato | multi-lambda prop of AGN | [0.1, 0.1, 0.1] | [0.1, 0.1, 0.1] | 0.0 |
Founding for a 1-year PostDoc for the inkind contribution have been recently approved by INAF (37000). A second year for the PostDoc is foreseen (35000).
# | Provenienza | Certi 2023 (k€) | Certi 2024 (k€) | Certi 2025 (k€) | Presun. 2023 (k€) | Presun. 2024 (k€) | Presun. 2025 (k€) | Totale Certi (k€) | Totale Presunti (k€) |
---|---|---|---|---|---|---|---|---|---|
1 | INAF | 0 | 0 | None | 35000 | 0 | None | 0 | 35000 |
# | Provenienza | Fondi 2023 (€) | Fondi 2024 (€) | Fondi 2025 (€) |
---|---|---|---|---|
1 | INAF - Mini Grant | 18200.0 |