DARTS/Astro Query System - SQL Search -
All the tables available for SQL Search and information on each table are listed in the Available Data page. Please see the User Guide for the usage of "SQL Search".
total 1
No. |
object_name
|
center_ra
|
center_dec
|
center_ra_b1950
|
center_dec_b1950
|
center_ecliptic_lon
|
center_ecliptic_lat
|
center_galactic_lon
|
center_galactic_lat
|
roll_angle
|
observation_start_time_mjd
|
observation_start_time
|
observation_end_time_mjd
|
observation_end_time
|
observation_id
|
exposure
|
awarded_exposure
|
xis0_exposure
|
xis1_exposure
|
xis2_exposure
|
xis3_exposure
|
xis0_observation_mode
|
xis1_observation_mode
|
xis2_observation_mode
|
xis3_observation_mode
|
hxd_observation_mode
|
hxd_coarse_clock_rate_exposure
|
hxd_first_clock_rate_exposure
|
hxd_normal_clock_rate_exposure
|
hxd_all_clock_rate_exposure
|
hxd_wam_exposure
|
quantity_of_hxd_burst
|
processing_status
|
processing_date_mjd
|
processing_date
|
public_date_mjd
|
public_date
|
distribution_date_mjd
|
distribution_date
|
processing_version
|
processing_count
|
processing_software
|
proposal_id
|
proposal_abstract
|
proposal_category
|
proposal_category_code
|
proposal_priority
|
pi_name
|
co_pi_name
|
proposal_affiliated_country
|
proposal_cycle
|
observation_type
|
proposal_title
|
main_instrument
|
has_xis_injection
|
data_access_url
|
ql_access_url
|
ql_image_url
|
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1 | IRAS F11119+3257 | 168.6582 | 32.6829 | 167.981225 | 32.955487 | 156.042952 | 25.438757 | 192.21056175 | 68.35212615 | 301.5808 | 56425.1110185185 | 2013-05-13 02:39:52 | 56431.3329050926 | 2013-05-19 07:59:23 | 708038010 | 252.2992 | 250 | 252.3232 | 252.2992 | 0 | 252.3232 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 220.3036 | 220.3036 | 400.8599 | 10 | PROCESSED | 57611.4720717593 | 2016-08-11 11:19:47 | 56858 | 2014-07-20 00:00:00 | 56491.9181828704 | 2013-07-18 22:02:11 | 3.0.22.44 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 081441 | Recent Herschel observations provided a breakthrough in identifying powerful, large-scale molecular outflows in ULIRGs, indicating that AGN feedback can indeed have a strong impact on star formation and galaxy evolution, in accordance with theoretical models. However, observational evidence for the connection between the putative fast nuclear AGN winds required for the formation of these large-scale outflows is missing. X-ray observations of blue-shifted Fe K absorption lines directly probe ultra-fast outflows (UFOs) ejected from the AGN accretion disk with v>10,000km/s. A 250ks Suzaku exposure of the ULIRG F11119+3257 with observed extreme molecular/neutral/ionized outflows would allow to characterize the expected UFO, providing the "smoking gun" evidence for feedback driven by AGN winds. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | FRANCESCO TOMBESI | USA | 8 | AO8 | IRAS F11119+3257: THE "SMOKING GUN" EVIDENCE FOR AGN FEEDBACK | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/708038010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '708038010'
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