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 NGC 4051 180.7984 44.5394 180.160059 44.817725 159.257872 40.347523 148.85547697 70.08163582 138.344 54776.3187847222 2008-11-06 07:39:03 54782.1112731482 2008-11-12 02:40:14 703023010 274.5305 340 274.5305 274.5305 0 274.5305 2 2 0 2 1 0 0 220.1993 220.1993 441.4488 3 PROCESSED 57544.5089930556 2016-06-05 12:12:57 54557 2008-04-01 00:00:00 54795.7746527778 2008-11-25 18:35:30 3.0.22.43 2 Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 031014 The powerful combination of Principal Components Analysis with time-resolved X-ray spectroscopy of Seyfert AGN has shown strong evidence that changes in a complex absorber are the origin of much of observed AGN spectral and flux variability. Large column, high ionization layers of gas may arise in a disk wind, representing a significant new, and possibly dominant, component, responsible for shaping the X-ray spectrum of AGN. The broad bandpass of Suzaku gives us a unique opportunity to model primary and reflected continua and the effects of variable absorbing zones, and test wind and other models. We propose a long 340 ks exposure on the NLSy1 NGC 4051 whose large amplitude of variability and well-studied complex absorption will test those models to the limit EXTRAGALACTIC COMPACT SOURCES 7 A TRACEY TURNER USA 3 AO3 DECONSTRUCTING SEYFERT SPECTRA - TIME FOR A PARADIGM SHIFT? XIS Y https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/703023010/ Quick Look

Used SQL

SELECT * FROM suzaku_master_data WHERE observation_id = '703023010'

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