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 | 180.8556 | 44.5807 | 180.217538 | 44.859022 | 159.275193 | 40.404023 | 148.68917976 | 70.06918189 | 135.3482 | 53684.8015509259 | 2005-11-10 19:14:14 | 53687.4315277778 | 2005-11-13 10:21:24 | 700004010 | 119.578 | 150 | 119.61 | 119.61 | 119.586 | 119.578 | 2 | 2 | 2 | 2 | 1 | 0 | 0 | 120.0047 | 120.0047 | 227.1918 | 3 | PROCESSED | 57528.0225810185 | 2016-05-20 00:32:31 | 54247 | 2007-05-27 00:00:00 | 54037.5713078704 | 2006-10-29 13:42:41 | 3.0.22.43 | 3 | Hea_08Feb2016_V6.18_Suzaku_14Nov2013_V22 | 001012 | We propose to obtain a broad band spectrum of the narrow-line Seyfert 1 (NLS1) NGC 4051. NLS1s are often presumed that they host a relatively small black hole with a very high accretion rate. Such a class would have played an important role in the growth of black holes in a cosmological context. We will measure the intrinsic photon index, amount of reflection, and high energy cutoff for the first time to investigate an accretion disk under a high accretion rate and compare them with conventional broad-line Seyferts. | EXTRAGALACTIC COMPACT SOURCES | 7 | A | YUICHI TERASHIMA | JAP | 0 | SWG | THE ACCRETION IN THE NARROW-LINE SEYFERT 1 NGC 4051 PROBED BY A BROAD BAND SPECTRUM | HXD | N | https://data.darts.isas.jaxa.jp/pub/suzaku/ver3.0/700004010/ | Quick Look |
Used SQL
SELECT * FROM suzaku_master_data WHERE observation_id = '700004010'
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