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 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'

Your request has been accepted.
The download will start soon automatically.

Go to top of this page ⏏