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 3783 | 174.7611 | -37.7364 | 174.141196 | -37.45925 | 192.677729 | -36.170962 | 287.45850943 | 22.95048745 | 293.6402 | 53910.7726388889 | 2006-06-24 18:32:36 | 53912.8571412037 | 2006-06-26 20:34:17 | 701033010 | 75.7193 | 75 | 75.7193 | 75.7193 | 75.7193 | 75.7193 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 68.2993 | 68.2993 | 180.0237 | 0 | PROCESSED | 57534.7899652778 | 2016-05-26 18:57:33 | 54401 | 2007-10-28 00:00:00 | 53926.8847453704 | 2006-07-10 21:14:02 | 3.0.22.43 | 4 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 011325 | We propose a 75 ksec Suzaku observation of the bright Seyfert 1 NGC 3783. Absorption due to photo-ionized material in the line of sight is well-established in this source, but can lead to degeneracy during modeling: is 3-6 keV continuum curvature due to photo-ionized absorption or a relativistically broad Fe K component? The simultaneous broadband XIS/HXD coverage is needed to define the continuum emission over a wide bandpass and disentangle the various emitting and absorbing components. We can then study the ionized absorber components, establish whether or not broad Fe K emission exists, and constrain reflection components, including the Compton shoulder. | EXTRAGALACTIC COMPACT SOURCES | 7 | B | ALEX MARKOWITZ | USA | 1 | AO1 | PROBING FE K EMISSION AND IONIZED ABSORPTION IN NGC 3783 | XIS | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/701033010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '701033010'
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