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
1 NGC3227 155.8768 19.8689 155.194236 20.122276 150.38752 9.143295 216.98468368 55.44605831 113.2489 54782.1173032407 2008-11-12 02:48:55 54783.7293865741 2008-11-13 17:30:19 703022030 56.5715 50 56.5772 56.5852 0 56.5715 2 2 0 2 1 0 0 50.2231 50.2231 139.2698 1 PROCESSED 57544.401724537 2016-06-05 09:38:29 54557 2008-04-01 00:00:00 54797.3603356482 2008-11-27 08:38:53 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031013 We propose a 2 month Suzaku monitoring program of 7 weekly 50ksec observations of the normal type 1 AGN, NGC3227. Variations of the Warm Absorber will determine its location in NGC5548, discriminating between models and determining the mass loss rate in the WA wind. This mdot will provide a calibration at low M_BH/Mdot(Edd) compared with our Cycle 2 NGC5548 measurement 'cosmological feedback' models from AGN to galaxy formation. Simultaneously, the XIS and HXD spectra will study changes, or lack thereof, in the reflection components (narrow Fe-K, Compton Hump), again delimiting their location and choosing among models. The summed spectrum will determine the high energy continuum break, and any broad Fe-K or high ionization edge. EXTRAGALACTIC COMPACT SOURCES 7 A MARTIN ELVIS USA 3 AO3 NGC3227 MONITORING: KEY TO AGN STRUCTURE AND COSMIC FEEDBACK XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703022030/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '703022030'

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