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 | NGC3227 | 155.8768 | 19.8687 | 155.194236 | 20.122076 | 150.387594 | 9.143109 | 216.98501654 | 55.44599229 | 109.926 | 54802.6028125 | 2008-12-02 14:28:03 | 54803.7231365741 | 2008-12-03 17:21:19 | 703022060 | 51.4105 | 50 | 51.4105 | 51.4105 | 0 | 51.4105 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 39.6836 | 39.6836 | 96.7818 | 1 | PROCESSED | 57544.6321875 | 2016-06-05 15:10:21 | 54557 | 2008-04-01 00:00:00 | 54812.4432407407 | 2008-12-12 10:38:16 | 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/ver3.0/703022060/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703022060'
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