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 | 1H0419-577 | 66.5116 | -57.211 | 66.267931 | -57.322556 | 29.331877 | -75.671402 | 266.99901337 | -41.98911345 | 55.5914 | 54306.2319328704 | 2007-07-25 05:33:59 | 54309.0835532407 | 2007-07-28 02:00:19 | 702041010 | 205.8628 | 200 | 205.8708 | 205.8708 | 0 | 205.8628 | 2 | 2 | 0 | 2 | 1 | 0 | 0 | 152.8317 | 152.8317 | 246.3578 | 2 | PROCESSED | 57539.3963888889 | 2016-05-31 09:30:48 | 54706 | 2008-08-28 00:00:00 | 54339.7211111111 | 2007-08-27 17:18:24 | 3.0.22.43 | 2 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 021304 | A hotly debated question is whether Seyfert X-ray spectra are dominated by components that are blurred by strong gravitational effects close (< 20rg) to the central black hole. Models featuring either complex absorption or blurred disk spectra provide equally good parameterizations of the mean X-ray spectrum of many objects. To make progress with current instruments we require observations with a temporal baseline and flux that will allow us to look for key parameter correlations, as the two scenarios predict different time-dependent behavior. To that end, we propose a Suzaku observation of 1H0419-577, a target that exhibits a remarkable degree of spectral variability in the X-ray regime promising some definitive results in this important area. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | TRACEY TURNER | USA | 2 | AO2 | HOW IMPORTANT IS STRONG RELATIVISTIC BLURRING IN SPECTRA OF SEYFERT GALAXIES? | XIS | Y | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/702041010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '702041010'
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