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 | NGC 4051 | 180.7952 | 44.5393 | 180.156844 | 44.817625 | 159.255387 | 40.346248 | 148.86124636 | 70.08047443 | 126.4079 | 54793.7 | 2008-11-23 16:48:00 | 54795.572025463 | 2008-11-25 13:43:43 | 703023020 | 78.3855 | 70 | 78.3935 | 78.3855 | 0 | 78.3939 | 1 | 1 | 0 | 1 | 1 | 0 | 0 | 62.7604 | 62.7604 | 161.7358 | 0 | PROCESSED | 57544.5729513889 | 2016-06-05 13:45:03 | 54557 | 2008-04-01 00:00:00 | 54811.74875 | 2008-12-11 17:58:12 | 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/ver3.0/703023020/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '703023020'
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